Testing the Evolutionary Link Between Submillimetre Galaxies and Quasars CO Observations of
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1081. Wood is an environmentally friendly building material because it _____ carbon dioxide, absorbing it during growth and retaining it even after it has been turned into lumber.A. dispersesB. eradicatesC. sequestersD. respiresE. regulates2. Despite the fact that it is quite difficult to find, in everyday discourse, causal explanations taking the form Hume proposed, many philosophers have regarded Hume’s model as _____ causal accounts.A. paradigmatic ofB. unworkable forC. tendentious aboutD. superfluous toE. irreducible to3. Goodin notes that people have (i)_____ cognitive capacities and that they therefore must consider some factors as (ii)_____ so as to be able to make decisions about other things.4. Some people (i)_____ translations of great literary works—especially those insistent on a literal translation for whom no rendering is ever (ii)_____ enough.5. It was not until 1995 that a planet beyond our solar system was first sighted, a discovery that greatly excited astronomers. Many had supposed that the processes that gave rise to our solar system were not (i)_____, and that there were other planets in the universe. Now, observations had (ii)_____.6. The longer the migratory route, the more fat migrating birds must accumulate as fuel for their flight. The gain in body mass would make birds obese by human standards, and should render them unable to fly, but this gain is (i)_____ premigratory (ii)_____ of digestive organs, inactive during migration, and by the (iii)_____ of the mu scles that power the flight.Soil communities are dependent on plants for organic matter. Plants provide organic matter for soil communities through the decomposition of leaf litter, by oozing nutrients from roots, or through other methods of deposition of organic compounds into the soil environments. As a result of these diverse methods by which plants supply resources, unique soil communities form under different plant species and under plant communities that differ in composition. If a nonnative plant species invades an above-ground community of flora and fauna, it can alter links between the native above-ground community and the below-ground soil community. For example, an invading nonnative plant could alter the quantity of leaf litter production, which would alter nutrient contributions to the soil.7. According to the passage, plants supply resources to soil communities by which of the following methods?A. Some plants supply resources to soil communities by promoting diversity of above-ground flora and fauna.B. Some plants supply resources to soil communities by oozing nutrients from their roots.C. Some plants supply resources to soil communities by depositing leaf litter.8. Which of the following statements about the connection between above-ground plants and below-ground soil communities can be inferred from the passage?A. Because of the nature of the link between above-and below-ground communities, many soil communities are deficient in nutrients.B. The extent to which soil communities are dependent on above-ground plants is extremely variable from one soil community to another.C. Because different plants supply resources to soil communities in different ways, distinctive soil communities form under different plant communities.Based on evidence from tree rings, pollen samples and other records, scientists have for a long time assumed that interglacials—warm interludes between ice ages—were as mild and uniform as the Holocene, the present interglacial, has been for all of its 8,000 to 10,000 years. But new research in Greenland has put this assumption into question.Researchers on two teams, the Greenland Ice-Core Project (GRIP) and the Greenland Ice Sheet Project 2 (GISP2), have analyzed two different cylinders of ice, each about two miles in depth, pulled up from the Greenland ice sheet. Such ice cores trap gases, bits of dust, and other chemicals that were present in the snow that fell over Greenland for thousands of years and then became compressed into ice. By studying these components, scientists have obtained a detailed archive of many aspects of climate, including air temperatures, snowfall, and concentrations of greenhouses gases in the atmosphere.Findings from the upper sections of the cores have confirmed what scientists already knew climate during the last ice age fluctuated rapidly. But scientists were astonished by findings from the lower sections of the GRIP core, which provided a close look at an interglacial period other than our own, the Eemian interglacial, a period that lasted from 135,000 to 115,000 years ago. Data from GRIP seem to indicate that the Eemian climate swung at least as wildly as the climate of ice age periods.Researchers’ clues to the Eemian climate come from measurements of the ratios of two slightly different types of oxygen, isotopes oxygen-16 and oxygen-18, preserved in the GRIP core. These ratios register the fluctuations of air temperatures over the seasons and years. When the air was warm, vapor containing the heavier isotope, oxygen-18, condensed and formed precipitation, in the form of snow, more readily than did vapor containing oxygen-16. Thus, snow that fell during warmer periods contains proportionally more oxygen-18 than snow deposited during cold spells. Evidence of rapid climate shifts was also drawn from other sources, such as measurements of amounts of dust and calcium ions in the ice layers during cold periods: winds were strong, causing calcium-rich dust from loess deposits, which are composed of loose surface sediment, to blow across the ice sheet. Thus, differing amounts of dust in the layers also indicate changing climatic conditions.However, finds from the lower section of GISP 2 do not confirm those of GRIP. The wild climate swings shown by GRIP in the last interglacial are not seen in the GISP2 core. According to a GISP 2 scientist, the weight of flowing glacial ice above has stressed the lower sections of both cores. This may have deformed the lower ice, disrupting its annual layers and thereby causing the discrepancy between the records. Still, some climatologists believe GRIP’s record may be the more reliable of the two. It was drilled closer to a location called the ice divide, where stresses would have been lower, they say.9. The passage is primarily concerned withA. refuting certain scientific theories about Earth’s climatic historyB. outlining new findings concerning Earth’s climate during ice agesC. discussing new research that may challenge a long-held scientific assumption about Earth’s climatic historyD. describing the climatic changes that occurred when Earth moved from an ice age into an interglacial periodE. reconciling conflicting evidence concerning climatic changes.10. Which of the following describes research that is most clearly analogous to the testing done by GRIP scientists?A. Scientists studying the formation of the Sahara desert measure the rate of topsoil erosion in the region"B. Scientists seeking to determine the age of a particular fossil measure the percentage of its carbon atoms that have decayedC. Scientists researching vision in flies measure and compare the amounts of vitamin A found in the retinas of several fly species."D. Scientists investigating the development of life on Earth measure and compare the amount of oxygen used by various organisms along the evolutionary scale.E. Scientists plotting the fluctuations in rainfall in the early rain forests measure the presence of certain gases trapped in tree rings of older trees.11 According to the passage, which of the following is the most accurate statement of what scientists believed, prior to the GRIP findings, about Earth’s climate?"A. Over the c ourse of Earth’s history, interglacials have become progressively milderB. Earth’s overall climate has been generally mild since the planet’s formationC. During both interglacials and ice ages, Earth’s climate has fluctuated violently.D. During ice ages, Earth’s climate has been highly variable, whereas during interglacials it has been mild and stable."E. During interglacials, Earth’s climate has been highly variable, whereas during ice ages it has been uniformly cold and icy.12. The passage suggests that which of the following is most likely to have been true of the oxygen-16 and oxygen-18 isotopes found in the lower sections of the GRIP core?"A. There was significantly more isotope oxygen-18 than isotope oxygen-16 in the ice layers.B. There was significantly more isotope oxygen-16 than isotope oxygen-18 in the ice layers.C. Ratios of isotopes oxygen-18 and oxygen-16 varied in the ice layers.D. Layers containing isotope oxygen-18 placed stress on the layers containing isotope oxygen-16, possibly distorting them."E. Isotope oxygen-16, being lighter, was located mainly in the upper layers, whereas oxygen-18 had settled into the lower layers.13. In spite of her fascination with chance, coincidence, and contingency, Stanning’snovels are _____ constructed, written from the head rather than the heart.A. hastilyB. extravagantlyC. painstakinglyD. meticulouslyE. evocativelyF. i mpulsively14. Although traditionally artists have rightly been seen as the most _____ audience for the work of their colleagues, today taste is also created by critics and curators and occasionally by collectors.A. arbitraryB. volatileC. perceptiveD. impulsiveE. subjectiveF. d iscerning15. Every serious attempt at a historical portrait of the past will subtly absorb the milieu and temperament of its living author, however _____ he or she sets out to be.A. entertainingB. comprehensiveC. objectiveD. engagingE. rigorousF. i mpartial16. Although we no longer have to rely on salt to keep food from spoiling, our appetite for it is _____: most people eat much more salt than they need.A. involuntaryB. inconstantC. unabatedD. unpredictableE. undiminishedF. i nsatiable166Although several ancient cultures practiced mummification, mummies from ancientEgypt are generally more well-preserved than mummies of similar antiquity from other cultures. One possible explanation for this difference is that the mummification techniques or material used by ancient Egyptians were better than those of other cultures. A second, more likely, explanation is that the extremely dry climate of ancient Egypt was largely responsible, given that dryness promotes the preservation of organic remains generally.17. Which is the following provide the most support for the argument?A. The materials used by ancient Egyptians for mummification were not used by any other ancient culture that practiced mummificationB. Some ancient Egyptian mummies are better preserved than other ancient Egyptian mummies form around the same time.C. No ancient people living in very damp areas practiced mummification.D. Bodies from ancient Egyptian tombs dating from before the practice of mummification began are almost as well preserved as ancient Egyptian mummies.E. Ancient mummies discovered in places other than Egypt have typically not been as well protected from the elements as ancient Egyptian mummies were.57Recent studies of the Philippine fruit bat fauna have confirmed some previoushypotheses regarding bats on oceanic islands: for example, species richness[ the number of different species in a particular area] and abundance are generally highest in the lowlands and decrease with increasing elevation. With few exceptions, each endemic species [species native to a particular place] is restricted to the modern islands that made up a single island during periods of low sea level, and genetic differentiation has been influenced by the ecology of the species and the current and past geographic and geological conditions. However, far more previous hypotheses have been overturned than supported. Some endemic Philippine species use disturbed habitat as extensively as nonendemic species that are widespread in Southeast Asia. Levels of genetic variation within all species are high, not low, and rather than showing evidence of an intrinsic vulnerability to extinction from natural causes, independent lineages of these bats have persisted in rather small areas for very long periods of time(often millions of years) in spite of frequent typhoons and volcanic eruptions. While colonization from outside areas has clearly contributed to the high species richness, speciation within the archipelago has contributed at least a quarter of the total species richness, including many of the most abundant species.18. The primary purpose of the passage is toA. draw on studies of the Philippine fruit bat in proposing a new theory regarding bats on oceanic islandsB. show how recent research on the Philippine fruit bat reflects debates about bats on oceanic islandsC. argue for the relevance of certain new evidence pertaining to the Philippine fruit bat or the study of bats on oceanic islandsD. discuss recent investigations of Philippines fruit bat in light of conventional wisdom regarding bats on oceanic islandsE. explain why the Philippine fruit bat is atypical among bats on oceanic islands in terms of genetic variation19. The primary function of the highlighted text is toA. identify a finding from the Philippine fruit bat studies that will have a significant impact on how oceanic bats generally are viewedB. point out a hypothesis that has been the subject of considerable disagreement among researchers studying oceanic batsC. present evidence that is difficult to reconcile with other recent findings regarding the Philippine fruit batD. illustrate a widely held view about oceanic bats generally that was confirmed by the Philippine fruit bat studiesE. identify a feature of the Philippine fruit bat that does not appear to apply to oceanic bats generally20. Which of the following can be inferred from t he passage about the “recent studies”?A. They point to the need for a significantly revised perspective on oceanic island bats generally.B. They were undertaken with the assumption that Philippine fruit bats were somewhat atypical among oceanic bats.C. They remain some what controversial among researchers because of the number of standard hypotheses that they tested.D. They have largely confirmed what scientists thought about the Philippine fruit bat.E. They suggest that bats on oceanic islands are more vulnerable to extinction than previously thought.。
2021年托福阅读真题第14篇Spider Web D… Spider Web DecorationsAn evolutionary puzzle is provided by orb-weaving spiders (weavers of round webs) that incorporate impressive zigzag lines of white ultraviolet silk into their webs. which would seem to make the trap more obvious to the prey that the spider needs to catch.Given that many insects can see ultraviolet light, one wonders how orb weavers could gain by alerting potential victims to the danger posed by their webs. But perhaps these web additions actually attract ultraviolet-reflecting bees that specialize in taking nectar from ultraviolet-reflecting flowers. The fact that bees constitute the large majority of prey of some spiders with ornamented webs supports this hypothesis.On the other hand, it could be that spiders that have been catching many prey. simply because their webs are in a good spot,are the spiders that tend to add decorations to their webs. If this is true, then the correlation between web decorations and higher rates of prey capture need not mean that the decorations cause the increase in prey capture. Instead, perhaps high feeding rates provide the extra energy that the spiders need to spin their web decorations. which they do for some purpose other than prey attraction. This hypothesis can be evaluated by testing the prediction that spiders given an abundance of food should invest more in web decorations than spiders deprived of food. Indeed, in two species of orb-weaving spiders, females that received more food made significantly larger decorations, and in one species.well-ed femaleswere more likely to add decorations to their webs than were food-deprived individuals.If one places an orb-weaving spider in a wooden frame and lets it build a web there, so that the web can be moved to a site chosen by the experimenter, then one can put two such webs side by side in a field. In this way, one can compare the rate of prey capture in an ornamented web with that in another web in the same spot whose decorations have been removed- -something that can be easily accomplished by cutting out the two web lines that support the decoration (two web lines are also cut from the other web, but not those that hold the decoration), Such an experiment controls for the effects of site productivity. Under these conditions, the decorated web catches about a third less prey than the undecorated one. Thus, web decorations involve a cost to foraging (obtaining food), not a benefit, under some conditions.If it is true that decorating one's web carries a cost in lost calories, what counterbalancing benefit exists for this behavior? One possibility is that when passing birds see the bright decorations, they swerve to avoid colliding with the web and getting covered in sticky silk. If this is true, then in the experiment above. webs with decorations should have been less often damaged by birds than webs without any "keep away" signals. And in fact, the actual results from the experiment matched the predicted ones, with decorated webs damaged by birds 45 percent less often than undecorated ones.Another benefit of web decorations might come from having the added silk camouflage (hide) the body of the web builder, making the spider less vulnerable to attack from its predators. Evidence in support of this explanation comes from a set of spiders whose females regularlyincorporate a silky egg sac into their webs. The spider perches (sits) on this moderately conspicuous vertical tube of silk, eggs, and debris in ways that make her much less visible to human observers, especially because the spider's color pattern matches that of the egg sac so closely. Moreover, when the egg sac is experimentally removed, the spider replaces it with a vertical strip composed entirely of silk, on which she perches as if it were an eggs sac. Given that the egg sac seems to be used as a concealment aid. its replacement can be assumed to serve the same function.More data on this point come from a study in which orb-weaving spiders that had built webs with or without extra silk decorations in an enclosed area were exposed to wasps. which hunt spiders and feed them to their offspring. In one experiment, only 32 percent of the spiders with web decorations were captured , as opposed to 68 percent of thosewithout.1.An evolutionary puzzle is provided by orb-weaving spiders (weavers of round webs) that incorporate impressive zigzag lines of white ultraviolet silk into their webs. which would seem to make the trap more obvious to the prey that the spider needs to catch.Given that many insects can see ultraviolet light, one wonders how orb weavers could gain by alerting potential victims to the danger posed by their webs. But perhaps these web additions actually attract ultraviolet-reflecting bees that specialize in taking nectar from ultraviolet-reflecting flowers. The fact that bees constitute the large majority of prey of some spiders with ornamented webs supports this hypothesis.2.On the other hand, it could be that spiders that have been catching many prey. simply because their webs are in a good spot,are the spiders that tend to add decorations to their webs. If this is true, then the correlation between web decorations and higher rates of prey capture need not mean that the decorations cause the increase in prey capture. Instead, perhaps high feeding rates provide the extra energy that the spiders need to spin their web decorations. which they do for some purpose other than prey attraction. This hypothesis can be evaluated by testing the prediction that spiders given an abundance of food should invest more in web decorations than spiders deprived of food. Indeed, in two species of orb-weaving spiders, females that received more food made significantly larger decorations, and in one species.well-ed females were more likely to add decorations to their webs than were food-deprived individuals.3.On the other hand, it could be that spiders that have been catching many prey. simply because their webs are in a good spot,are the spiders that tend to add decorations to their webs. If this is true, then the correlation between web decorations and higher rates of prey capture need not mean that the decorations cause the increase in prey capture. Instead, perhaps high feeding rates provide the extra energy that the spiders need to spin their web decorations. which they do for some purpose other than prey attraction. This hypothesis can be evaluated by testing the prediction that spiders given an abundance of food should invest more in web decorations than spiders deprived of food. Indeed, in two species of orb-weaving spiders, females that received more food made significantly larger decorations, and in one species.well-ed females were more likely to add decorations to their webs than were food-deprived individuals.4.On the other hand, it could be that spiders that have been catching many prey. simply because their webs are in a good spot,are the spiders that tend to add decorations to their webs. If this is true, then the correlation between web decorations and higher rates of prey capture need not mean that the decorations cause the increase in prey capture. Instead, perhaps high feeding rates provide the extra energy that the spiders need to spin their web decorations. which they do for some purpose other than prey attraction. This hypothesis can be evaluated by testing the prediction that spiders given an abundance of food should invest more in web decorations than spiders deprived of food. Indeed, in two species of orb-weaving spiders, females that received more food made significantly larger decorations, and in one species.well-ed females were more likely to add decorations to their webs than were food-deprived individuals.5.If one places an orb-weaving spider in a wooden frame and lets it build a web there, so that the web can be moved to a site chosen by the experimenter, then one can put two such webs side by side in a field. In this way, one can compare the rate of prey capture in an ornamented web with that in another web in the same spot whose decorations have been removed- -something that can be easily accomplished by cutting out the two web lines that support the decoration (two web lines are also cut from the other web, but not those that hold the decoration), Such an experiment controls for the effects of site productivity. Under these conditions, the decorated web catches about a third less prey than the undecorated one. Thus, web decorations involve a cost to foraging (obtaining food), not a benefit, under some conditions.6.If it is true that decorating one's web carries a cost in lost calories, what counterbalancing benefit exists for this behavior? One possibility is that when passing birds see the bright decorations, they swerve to avoid colliding with the web and getting covered in sticky silk. If this is true, then in the experiment above. webs with decorations should have been less often damaged by birds than webs without any "keep away" signals. And in fact, the actual results from the experiment matched the predicted ones, with decorated webs damaged by birds 45 percent less often than undecorated ones.7.Another benefit of web decorations might come from having the added silk camouflage (hide) the body of the web builder, making the spider less vulnerable to attack from its predators. Evidence in support of this explanation comes from a set of spiders whose females regularly incorporate a silky egg sac into their webs. The spider perches (sits) on this moderately conspicuous vertical tube of silk, eggs, and debris in ways that make her much less visible to human observers, especially because the spider's color pattern matches that of the egg sac so closely. Moreover, when the egg sac is experimentally removed, the spider replaces it with a vertical strip composed entirely of silk, on which she perches as if it were an eggs sac. Given that the egg sac seems to be used as a concealment aid. its replacement can be assumed to serve the same function.8.Another benefit of web decorations might come from having the added silk camouflage (hide) the body of the web builder, making the spider less vulnerable to attack from its predators. Evidence in support of this explanation comes from a set of spiders whose females regularly incorporate a silky egg sac into their webs. The spider perches (sits) onthis moderately conspicuous vertical tube of silk, eggs, and debris in ways that make her much less visible to human observers, especially because the spider's color pattern matches that of the egg sac so closely. Moreover, when the egg sac is experimentally removed, the spider replaces it with a vertical strip composed entirely of silk, on which she perches as if it were an eggs sac. Given that the egg sac seems to be used as a concealment aid. its replacement can be assumed to serve the same function.More data on this point come from a study in which orb-weaving spiders that had built webs with or without extra silk decorations in an enclosed area were exposed to wasps. which hunt spiders and feed them to their offspring. In one experiment, only 32 percent of the spiders with web decorations were captured , as opposed to 68 percent of those without.9.If it is true that decorating one's web carries a cost in lost calories, what counterbalancing benefit exists for this behavior?⬛One possibility is that when passing birds see the bright decorations, they swerve to avoid colliding with the web and getting covered in sticky silk. ⬛If this is true, then in the experiment above. webs with decorations should have been less often damaged by birds than webs without any "keep away" signals. ⬛And in fact, the actual results from the experiment matched the predicted ones, with decorated webs damaged by birds 45 percent less often than undecorated ones.⬛10.1.B2.C3.A4.C5.C6.D7.B8.C9.A10.BCD。
2020届高三英语专项训练——阅读理解D篇(一)A new study shows that rising levels of planet-warming gases may reduce important nutrients in food crops.Researchers studied the effects of one such gas—carbon dioxide—on rice. The researchers grew rice plants in a controlled environment. They set carbon dioxide levels to what scientists are predicting for our planet by the end of the century. They found that the resulting rice crops had lower than normal levels of vitamins, minerals and protein. The researchers said the effects of planet-warming gases would be most severe for the poorest citizens in some of the least developed countries. These people generally eat the most rice and have the least complex diets, they noted.In the experiment, scientists grew 18 kinds of rice in fields in China and Japan. They pumped carbon dioxide gas over the plants in an effort to create the atmosphere of the future. Rice grown under high carbon dioxide conditions had, on average, 13 to 30 percent lower levels of four B vitamins and 10 percent less protein. The crops also had 8 percent less iron and 5 percent less zinc(锌)an rice grown under normal conditions.However,vitamin E levels increased by about 13 percent on average.The results are bad news, “especially for the nutrition of the poorer po pulation in less-developed countries,” said the University of Tokyo’s Kazuhiko Kobayashi, who helped to write the report. That includes about 600 million people in Indonesia, Cambodia, Myanmar, Bangladesh, Laos and other nations, mainly in Southeast Asia, the report said.One of the scientists is Sam Myers of Harvard University in the American state of Massachusetts. He said that findings like this are an example of the surprises climate change create. “My concern is there are many more surprises to come,” he said.Myers noted that pollution, loss of some species, destruction of forests, and other human activities are likely to produce unexpected problems. He said that you cannot completely change all the natural systems that living organisms have grown to depend on over millions of years without having effects come back to affect our own health.The new study suggests a way to lower the nutritional harm of climate change. One way,Kobayashi said, is grow different forms of rice that have shown to be more resistant to higher carbon dioxide levels.32. Which county would be influenced most by planet-warming gases according to the text?A. ChinaB. MyanmarC. AmericaD. Britain33. How is Paragraph 3 mainly developed?A. By comparison.B. By giving examples.C. By analyzing causes.D. By describing a process.34. What does the underlined sentence in Paragraph 5 mean?A. Climate change will be difficult to predict.B. Climate change will lead to more good effects.C. Climate change will be harmful to environment.D. Climate change will cause more unexpected problems.35. Which of the following statements is true according to the text?A. Myerssaid we could change all the natural systems for the sake of our health.B. The poorest people in all the least developed countries would be influenced most.C. The researchers grew 18 kinds of rice in China and Japan in a controlled environment.D. Protein in rice grown under high carbon dioxide conditions is increased by 10 percent.BADC(二)Plants are boring. They just sit there (光合作用)while animals have all the fun. Right? Not so much. A new study has found that there is a long history of interactions between ants and plants. The ant and plant co-evolution(协同进化)started with ants feeding on plants and plants evolving ant-friendly features.Plants make a number of different structures that are specific for ant use. Some plants have evolved features that persuade ants into defending them from attack from other insects and even mаmmаlѕ. Тhеѕе іnсludе hollow thorns that аntѕ will live іnѕіdе, or ехtra nесtаr (琼浆) оn lеаvеѕ or stems for the ants to eat. Some ants will just cheat and take the nectar and run, but some will stick around and attack anything that tries to hurt the plant. Other plants get ants to help them move their seeds around, by providing them with rich food packets attached to the seeds. The antwill pick up the seed and carry it away, eat the food packet, and leave the seed - often in a nutrient-rich area where it'll grow better, and since it's farther away from its parent, they won't have to compete for resources.But scientists weren't sure how the evolutionary relationship between ants and plants got started. If evolution is an arms race between species developing ways to make use of their neighbors, then scientists wanted to know whether plants or ants fired the first shot. It was a chicken-and-egg question, whether things started with ants developing behaviors to take advantage of plants, or plants evolving structures to take advantage of ants.The history of ants and plants evolving together goes back to the time of the dinosaurs, and it's not easy to tell from fossils who fired the first shot. However, it is a question of little significance. Scientists say their study maters because it provides a look at how these widespread and complex interactions evolved.32.Some plants attach food packets to their seeds in order to.A.reward the ants B.get the seeds moved aroundC.make a fool of ants D.provide nutrition for the seeds33.What does Paragraph 2 mainly tell us?A.How plants and ants interact.B.What ants do to protect plants.C.How plants and ants survive attacks.D.Why plants and ants need co-evolution.34.Which is true about the evolutionary relationship between ants and plants?A.Ants depended more upon plants.B.It caused a race for better evolution.C.How it got started was uncertain.D.It was of little value for future studies.35.What's the author’s purpose of writing the passage?A.To introduce a science research method.B.To inform readers of a latest research findingC.To arouse readers' interest in science research.D.To criticize people's traditional views about plants.BACB(三)An experimental cleanup device called RemoveDEBRIS has successfully casta net around a dummy (仿真的) satellite, imitating a technique that could one day collect spaceborne garbage.The test, which was carried out this week, is widely believed to be the first successful demonstration of space cleanup technology, experts told CNN. And it symbolizes an early step toward solving what has already been a critical issue: junk in space.Millions of pieces of junk are turning around in orbit, the result of 50 years of spacetravel and few regulations to keep space clean. At orbital speeds, even a small bit of paint crashing with a satellite can cause critical damage.Various companies have plans to send thousands of new satellites into low-Earth orbit, already the most crowded area.The RemoveDEBRIS experiment is run by a company and researchers led by the U. K.’s Surrey Space Center and includes Airbus,Airbus-owned Surrey Satellite Technology Ltd. and France’sArianeGroup.Guglielmo Aglietti, the director of Surrey Space Center, said that an operational version of the RemoveDEBRlS technology would cast a net that remains fastened to the main satellite so the deb ris can be dragged out of orbit. It could target large pieces of junk, including dead satellites up to 10 meters long.The RemoveDEBRIS satellite will conduct a few more experiments in the coming months, including testing navigation features that could help guide the satellite to a specific piece of debris.Jonathan McDowell, an astrophysicist at the Harvard-Smithsonian Center for Astrophysics, said the successof this week’s experiment was ex c iting, but he cautioned against“over- publicizing” it.There are still enormous barriers to clear before operational cleanup tasks are underway, he said, and the most discouraging is figuring out how to fund such projects.Aglietti, the Surrey professor who helped lead the RemoveDEBRIS project, said “The challenge will lie in persuading the relevant authorities to sponsor these tasks.”Aglietti said he hopes RemoveDEBRIS will conduct a few cleanup tasks per year, targeting the largest pieces ofjunk in the most crowded orbits.32. What is the use of the RemoveDEBRIS satellite?A. Demonstrating space technology.B. Imitating a developing technique.C. Collecting wastes existing in space.D. Symbolizing great progress in space.33. How does the RemoveDEBRlS satellite work?A. By throwing a net to take the junk from orbit.B. By fastening it to the main satellite tightly.C. By dragging satellites up to 10 meters long.D. By targeting large pieces of junk carefully.34. What does the underlined word “sponsor” in the last paragraph probably mean?A. Accomplish.B. Support.C. Oppose.D. Provide.35. What’s the best title for the text?A. The RemoveDEBRIS Project Is PerfectB. How RemoveDEBRIS Is Invented in the LabC. Why the RemoveDEBRIS Satellite Is InventedD. Satellite Collects Space Junk for the First TimeCABD(四)China’s cancer researcher Zhu Chen, together with two French researchers Anne Dejean and Hugues de The, received Sjoberg Prize 2018 in Stockholm Concert Hall, Sweden on Friday.“We used wisdom from both Chinese and Western medicine and offered a cure for one of the most deadly cancers,” Chen told Xinhua, “I feel that Chinese medicine has the potential to contribute more to human health. There are no borders in medicine, because it struggles for benefiting all mankind. It’s a language of peace, and of development and progress.” Chen recalled the cooperation with the two French researchers for over 30 years.This year’s Sjobe rg winners have developed a new and targeted treatment for a specific form of blood cancer called acute promyelocytic leukaemia (急性早幼粒白血病). It was once one of themost deadly forms of cancer, but it is now possible to cure nine out of ten patients who receive the new treatment. The winners have made this revolutionary development possible by methodically mapping the molecular mechanisms responsible for the disease.The prize is awarded by the Royal Swedish Academy of Sciences and is funded by the Sjoberg Foundation. The foundation, with a donation of 2.5 billion US dollars, was founded in 2016, and serves to promote scientific research that focuses on cancer, health and the environment.The prize is an annual international prize in cancer research awarded to individual researchers or research groups. The prize amounts to one million US dollars, of which 100,000 US dollars is the prize sum and 900,000 US dollars is funding for future research.32.W hy was Zhu Chen awarded Sjoberg Prize?A.For the research into a language.B.For the promotion of Chinese medicine.C.For the treatment for a once fatal cancer.D.For the cooperation with French researchers.33.W hat can we know about the Sjoberg Foundation?A. It funds research in certain fields.B. It favors individual researchers.C. It donates 2.5 million US dollars.D. It awards the prize annually.34. What can the text be classified as?A. A biography.B. A news report.C. A science fiction.D. An advertisement.35. What is the best title for the text?A. New Cure for CancerB. No Borders in MedicineC. Great Contributions to Human HealthD. Chinese Scientist Receiving Sjoberg PrizeCABD(五)Few people, these days would disagree with the theory that it's vital to take time for yourself. Creating some space for enjoyment and restoration each day or atleast every week, is a win-winproposal: it’ll make you both happier and more effective in fulfilling your responsibilities at work andhome. In practice, itrarely happens, though. For some, that's because deep down theyfeet they don'tdeserve it. For others, it's simply that busy life makes it seem impossible to press pause. Either way,making sure you actually get a. moment to yourself requires a shift in perspective.Don't wait until it feels right. It's unpleasant to have unfinished tasks bothering at your mind, soit's tempting to tell yourself you'll only relax once everything is under control. But since both workand family life generate an infinite number of to-dos, that strategy is doomed to failure. Astime-management writer Laura Vanderkarn points out, it's far more useful to learn to tolerate thediscomfort of knowing your email inbox is filling up, or that the living room is still a pigsty. Choose true enjoyment. It's all too easy to fill `me time' with things you think you should enjoy,above all exercise. If you genuinely love such activities, they're perfect. But if the truth is that youdon't, you'll only get resentful: we rebel against being told what to do, even when the person doingthe telling is ourselves. Make sure at least a small part of your week is spent doing something you canhonestly say you enjoy for itself.Pay attention to good feelings. Once you do get some restorative time, borrow a Buddhist technique for making it count: when you realize you're enjoying yourself, spend half a minuteconsciously paying attention to the feelings of pleasure. For one thing, you'll often find that thosefeelings increase as a result. For another, you'll encode the memory of the experience in more detailso, looking back, it'll feel like you had even more time to yourself.32. Why is it hard for some people to find time for themselves practically?A. They think they aren't worth itB. They have a lot of pressure.C. They are in financial trouble.D. They can't spare any time33. Which of the following is acceptable according to Paragraph two?A. Never put off what you should do.B. Take a rest when it's time toC. Relax yourself with all work done.D. Put up with others' shortcomings.34. Which is the closest to "resentful" in paragraph three?A. pleased.B. relaxed.C. relieved.D. annoyed.35. What is best title of the passage?A. Learn to Manage TimeB. Find Time for YourselfC. Squeeze Time to ExerciseD. Strengthen Time ConsciousnessABDB。
2024年高考英语模拟试卷注意事项:1.答题前,考生先将自己的姓名、准考证号填写清楚,将条形码准确粘贴在考生信息条形码粘贴区。
2.选择题必须使用2B铅笔填涂;非选择题必须使用0.5毫米黑色字迹的签字笔书写,字体工整、笔迹清楚。
3.请按照题号顺序在各题目的答题区域内作答,超出答题区域书写的答案无效;在草稿纸、试题卷上答题无效。
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第一部分(共20小题,每小题1.5分,满分30分)1._____ his homework in time, he had to stay up late into the night.A.Finishing B.Having finished C.To finish D.To have finished2.I writing the paper as scheduled, but my mother’s illness interfered. I hope you will excuse me.A.am to have finished B.was to have finishedC.was to finish D.ought to finish3.We packed all the hooks in wooden boxes so that they damaged.A.don’t get B.won’t getC.didn’t get D.wouldn’t get4.Chinese President Hu Jintao called for an immediate cease-fire in Libya _____ an even worse humanitarian crisis in the country at the BRICS Summit in Hainan Province.A.to prevent B.to have prevented C.preventing D.having prevented5.---- What do you think of zoology?---- In my opinion, zoology is ______ botany.A.a subject so interesting as B.as a interesting subject asC.as interesting a subject as D.interesting as a subject as6.It is through years of research ________ scientists have discovered the relationship between social media addiction and depression.A.since B.before C.that D.when7.I have often thought it would be a blessing if each human being _______ blind and deaf for a few days at some time in his life.A.has been stricken B.were strickenC.had been D.would be8.Many people fall into panic due to the earthquake and tsunami in Japan but experts don’t expect this to be ________ as proper measures have been taken.A.compulsory B.contemporary C.temporary D.permanent9.Lifting off at sunrise, the hot air balloon goes wherever the wind blow.A.may B.must C.need D.should10.Mother told me in a phone call that she had written to me a week before, but I haven’t received__________.A.one B.it C.something D.anything11.After college, he was employed in a middle school and there ever since.A.would worked B.had workedC.worked D.has worked12.We are living in an age________ QR codes(二维码)are becoming more and more popular in our daily life. A.why B.thatC.whose D.when13.The days are gone physical strength was all you needed to make a living.A.that B.whenC.where D.which14.—How I wish I had worked harder when I was in that company.—If you had, you _________ a department manager now.A.are B.would beC.would have been D.were15.The petrol in the car _____ on our way to the beach, so we had to walk there.A.gave up B.gave off C.gave in D.gave out16.She seems to prefer American TV Shows to talking to me.A.to watch B.to be watching C.watching D.having watched17.I like these English songs and they ________ many times on the radio.A.taught B.have taughtC.are taught D.have been taught18.To tell the truth, I didn’t expect that there were so many people ______ the idea.A.supported B.supporting C.to support D.having supported19.I ________ able to catch the first flight home, but my watch betrayed me.A.were B.had beenC.would be D.would have been20.I am sorry I am very busy now. If I time, I would certainly go to the movies with you.A.have B.hadC.have had D.had had第二部分阅读理解(满分40分)阅读下列短文,从每题所给的A、B、C、D四个选项中,选出最佳选项。
生命在于运动英语作文七年级Life is in MotionMovement is a fundamental aspect of our existence. From the smallest subatomic particles to the grandest celestial bodies, everything in the universe is in a constant state of motion. This innate drive to move, to change, to evolve is what defines life itself. Whether it's the rhythmic beating of our hearts, the ebb and flow of the tides, or the cycling of the seasons, the principle of motion is woven into the fabric of our world.At the most basic level, life is defined by the ability to move. Unicellular organisms such as bacteria and protozoa propel themselves through their environments, seeking out resources and evading threats. Even the simplest forms of life possess the capacity for locomotion, a testament to the primal importance of movement. As we move up the evolutionary ladder, this capacity for motion becomes increasingly sophisticated, culminating in the complex, coordinated movements of higher lifeforms.Consider the animal kingdom, where movement is essential for survival. Predators must chase down their prey, while prey must flee from their hunters. Migratory birds traverse vast distances, driven by an innate urge to follow the changing seasons. Whales, dolphins, and other marine creatures undertake epic journeys across the oceans, navigating through currents and tides. In each case, the ability to move is not just a luxury, but a matter of life and death.Even within the confines of a single organism, motion is a fundamental aspect of life. Our bodies are a symphony of movement, from the involuntary contractions of our muscles to the deliberate actions of our limbs. We breathe, we blink, we swallow, we fidget –all in a constant, unconscious dance of motion. And when we consciously choose to move, to exercise, to engage in physical activity, we tap into a deeper well of vitality and well-being.The connection between movement and health is well-established. Regular physical activity has been shown to reduce the risk of a wide range of diseases, from heart disease and diabetes to certain types of cancer. Exercise strengthens our muscles, improves our cardiovascular fitness, and boosts our mental well-being. It is no coincidence that the word "animation" is derived from the Latin word for "life" – the act of moving, of being in motion, is a fundamental expression of our aliveness.But the importance of movement extends beyond the physical realm. Our minds, too, are in a constant state of motion, processing information, generating ideas, and navigating the complexities of our inner and outer worlds. The ability to think, to problem-solve, to imagine – these are all forms of mental motion, of the mind's ceaseless activity.Indeed, many of our greatest thinkers and innovators have recognized the vital role that movement plays in the life of the mind. The ancient Greek philosopher Plato believed that the soul was in a constant state of motion, and that true knowledge could only be attained through the active engagement of the mind. The Romantic poet William Wordsworth extolled the virtues of walking, arguing that it was essential for the creative process.In our own lives, we can attest to the power of movement to stimulate the mind. When we are physically active, whether it's through exercise, dance, or even just a leisurely stroll, we often find that our thoughts become clearer, our ideas more fluid, and our creativity more vibrant. The act of moving, of engaging our bodies, seems to unlock new pathways in our minds, allowing us to see the world in fresh and unexpected ways.But the significance of movement extends beyond the individual, touching on the very fabric of our social and cultural existence. Thehistory of human civilization is a story of movement, of migrations,of the exchange of ideas, goods, and peoples across vast distances. The great trade routes of the ancient world, the voyages of exploration and discovery, the mass movements of populations –these are all manifestations of the deep-seated human drive to move, to explore, to connect.In our own time, the pace of global movement has only accelerated. Advances in transportation and communication technology have shrunk the world, allowing us to traverse continents and oceans with unprecedented speed and ease. The flow of information, ideas, and cultural influences across borders has become a defining feature of our age, shaping the way we work, learn, and interact with one another.Yet, even as we celebrate the remarkable achievements of human mobility, we must also grapple with the challenges it presents. The displacement of populations due to war, famine, and climate change has led to unprecedented humanitarian crises, testing the limits of our compassion and our capacity for collective action. The environmental toll of our relentless movement – from the carbon emissions of air travel to the plastic waste of our consumer culture –has put the very future of our planet at risk.These challenges, however, do not diminish the fundamentalimportance of movement in our lives. Rather, they underscore the need to cultivate a more thoughtful, sustainable, and equitable approach to the way we move through the world. By recognizing the centrality of motion to the human experience, we can work to harness its power in service of a better future – one where the freedom to move is balanced with the responsibility to protect our shared home.In the end, the truth remains: life is in motion. It is a fundamental principle that governs the universe, from the subatomic to the cosmic scale. And within this grand, eternal dance, we humans find our place, our bodies and minds in perpetual motion, our spirits yearning to explore, to discover, to connect. It is a truth that has inspired artists, philosophers, and scientists alike, and one that continues to shape the course of our individual and collective journeys. So let us embrace this truth, and let it guide us as we navigate the ever-changing landscape of our lives.。
2020届高三英语专项训练——阅读理解D篇(一)A new study shows that rising levels of planet-warming gases may reduce important nutrients in food crops.Researchers studied the effects of one such gas—carbon dioxide—on rice. The researchers grew rice plants in a controlled environment. They set carbon dioxide levels to what scientists are predicting for our planet by the end of the century. They found that the resulting rice crops had lower than normal levels of vitamins, minerals and protein. The researchers said the effects of planet-warming gases would be most severe for the poorest citizens in some of the least developed countries. These people generally eat the most rice and have the least complex diets, they noted.In the experiment, scientists grew 18 kinds of rice in fields in China and Japan. They pumped carbon dioxide gas over the plants in an effort to create the atmosphere of the future. Rice grown under high carbon dioxide conditions had, on average, 13 to 30 percent lower levels of four B vitamins and 10 percent less protein. The crops also had 8 percent less iron and 5 percent less zinc(锌)an rice grown under normal conditions.However,vitamin E levels increased by about 13 percent on average.The results are bad news, “especially for the nutrition of the poorer po pulation in less-developed countries,” said the University of Tokyo’s Kazuhiko Kobayashi, who helped to write the report. That includes about 600 million people in Indonesia, Cambodia, Myanmar, Bangladesh, Laos and other nations, mainly in Southeast Asia, the report said.One of the scientists is Sam Myers of Harvard University in the American state of Massachusetts. He said that findings like this are an example of the surprises climate change create. “My concern is there are many more surprises to come,” he said.Myers noted that pollution, loss of some species, destruction of forests, and other human activities are likely to produce unexpected problems. He said that you cannot completely change all the natural systems that living organisms have grown to depend on over millions of years without having effects come back to affect our own health.The new study suggests a way to lower the nutritional harm of climate change. One way, Kobayashi said, is grow different forms of rice that have shown to be more resistant to highercarbon dioxide levels.32. Which county would be influenced most by planet-warming gases according to the text?A. ChinaB. MyanmarC. AmericaD. Britain33. How is Paragraph 3 mainly developed?A. By comparison.B. By giving examples.C. By analyzing causes.D. By describing a process.34. What does the underlined sentence in Paragraph 5 mean?A. Climate change will be difficult to predict.B. Climate change will lead to more good effects.C. Climate change will be harmful to environment.D. Climate change will cause more unexpected problems.35. Which of the following statements is true according to the text?A. Myerssaid we could change all the natural systems for the sake of our health.B. The poorest people in all the least developed countries would be influenced most.C. The researchers grew 18 kinds of rice in China and Japan in a controlled environment.D. Protein in rice grown under high carbon dioxide conditions is increased by 10 percent.BADC(二)Plants are boring. They just sit there (光合作用)while animals have all the fun. Right? Not so much. A new study has found that there is a long history of interactions between ants and plants. The ant and plant co-evolution(协同进化)started with ants feeding on plants and plants evolving ant-friendly features.Plants make a number of different structures that are specific for ant use. Some plants have evolved features that persuade ants into defending them from attack from other insects and even mаmmаlѕ. Тhеѕе іnсludе hollow thorns that аntѕ will live іnѕіdе, or ехtra nесtаr (琼浆) оn lеаvеѕ or stems for the ants to eat. Some ants will just cheat and take the nectar and run, but some will stick around and attack anything that tries to hurt the plant. Other plants get ants to help them move their seeds around, by providing them with rich food packets attached to the seeds. The ant will pick up the seed and carry it away, eat the food packet, and leave the seed - often in anutrient-rich area where it'll grow better, and since it's farther away from its parent, they won't have to compete for resources.But scientists weren't sure how the evolutionary relationship between ants and plants got started. If evolution is an arms race between species developing ways to make use of their neighbors, then scientists wanted to know whether plants or ants fired the first shot. It was a chicken-and-egg question, whether things started with ants developing behaviors to take advantage of plants, or plants evolving structures to take advantage of ants.The history of ants and plants evolving together goes back to the time of the dinosaurs, and it's not easy to tell from fossils who fired the first shot. However, it is a question of little significance. Scientists say their study maters because it provides a look at how these widespread and complex interactions evolved.32.Some plants attach food packets to their seeds in order to.A.reward the ants B.get the seeds moved aroundC.make a fool of ants D.provide nutrition for the seeds33.What does Paragraph 2 mainly tell us?A.How plants and ants interact.B.What ants do to protect plants.C.How plants and ants survive attacks.D.Why plants and ants need co-evolution.34.Which is true about the evolutionary relationship between ants and plants?A.Ants depended more upon plants.B.It caused a race for better evolution.C.How it got started was uncertain.D.It was of little value for future studies.35.What's the author’s purpose of writing the passage?A.To introduce a science research method.B.To inform readers of a latest research findingC.To arouse readers' interest in science research.D.To criticize people's traditional views about plants.BACB(三)An experimental cleanup device called RemoveDEBRIS has successfully casta net around a dummy (仿真的) satellite, imitating a technique that could one day collect spaceborne garbage.The test, which was carried out this week, is widely believed to be the first successful demonstration of space cleanup technology, experts told CNN. And it symbolizes an early step toward solving what has already been a critical issue: junk in space.Millions of pieces of junk are turning around in orbit, the result of 50 years of spacetravel and few regulations to keep space clean. At orbital speeds, even a small bit of paint crashing with a satellite can cause critical damage.Various companies have plans to send thousands of new satellites into low-Earth orbit, already the most crowded area.The RemoveDEBRIS experiment is run by a company and researchers led by the U. K.’s Surrey Space Center and includes Airbus,Airbus-owned Surrey Satellite Technology Ltd. and France’sArianeGroup.Guglielmo Aglietti, the director of Surrey Space Center, said that an operational version of the RemoveDEBRlS technology would cast a net that remains fastened to the main satellite so the deb ris can be dragged out of orbit. It could target large pieces of junk, including dead satellites up to 10 meters long.The RemoveDEBRIS satellite will conduct a few more experiments in the coming months, including testing navigation features that could help guide the satellite to a specific piece of debris.Jonathan McDowell, an astrophysicist at the Harvard-Smithsonian Center for Astrophysics, said the successof this week’s experiment was ex c iting, but he cautioned against“over- publicizing” it.There are still enormous barriers to clear before operational cleanup tasks are underway, he said, and the most discouraging is figuring out how to fund such projects.Aglietti, the Surrey professor who helped lead the RemoveDEBRIS project, said “The challenge will lie in persuading the relevant authorities to sponsor these tasks.”Aglietti said he hopes RemoveDEBRIS will conduct a few cleanup tasks per year, targeting the largest pieces of junk in the most crowded orbits.32. What is the use of the RemoveDEBRIS satellite?A. Demonstrating space technology.B. Imitating a developing technique.C. Collecting wastes existing in space.D. Symbolizing great progress in space.33. How does the RemoveDEBRlS satellite work?A. By throwing a net to take the junk from orbit.B. By fastening it to the main satellite tightly.C. By dragging satellites up to 10 meters long.D. By targeting large pieces of junk carefully.34. What does the underlined word “sponsor” in the last paragraph probably mean?A. Accomplish.B. Support.C. Oppose.D. Provide.35. What’s the best title for the text?A. The RemoveDEBRIS Project Is PerfectB. How RemoveDEBRIS Is Invented in the LabC. Why the RemoveDEBRIS Satellite Is InventedD. Satellite Collects Space Junk for the First TimeCABD(四)China’s cancer researcher Zhu Chen, together with two French researchers Anne Dejean and Hugues de The, received Sjoberg Prize 2018 in Stockholm Concert Hall, Sweden on Friday.“We used wisdom from both Chinese and Western medicine and offered a cure for one of the most deadly cancers,” Chen told Xinhua, “I feel that Chinese medicine has the potential t o contribute more to human health. There are no borders in medicine, because it struggles for benefiting all mankind. It’s a language of peace, and of development and progress.” Chen recalled the cooperation with the two French researchers for over 30 years.This year’s Sjoberg winners have developed a new and targeted treatment for a specific form of blood cancer called acute promyelocytic leukaemia (急性早幼粒白血病). It was once one of the most deadly forms of cancer, but it is now possible to cure nine out of ten patients who receive thenew treatment. The winners have made this revolutionary development possible by methodically mapping the molecular mechanisms responsible for the disease.The prize is awarded by the Royal Swedish Academy of Sciences and is funded by the Sjoberg Foundation. The foundation, with a donation of 2.5 billion US dollars, was founded in 2016, and serves to promote scientific research that focuses on cancer, health and the environment.The prize is an annual international prize in cancer research awarded to individual researchers or research groups. The prize amounts to one million US dollars, of which 100,000 US dollars is the prize sum and 900,000 US dollars is funding for future research.32.W hy was Zhu Chen awarded Sjoberg Prize?A.For the research into a language.B.For the promotion of Chinese medicine.C.For the treatment for a once fatal cancer.D.For the cooperation with French researchers.33.W hat can we know about the Sjoberg Foundation?A. It funds research in certain fields.B. It favors individual researchers.C. It donates 2.5 million US dollars.D. It awards the prize annually.34. What can the text be classified as?A. A biography.B. A news report.C. A science fiction.D. An advertisement.35. What is the best title for the text?A. New Cure for CancerB. No Borders in MedicineC. Great Contributions to Human HealthD. Chinese Scientist Receiving Sjoberg PrizeCABD(五)Few people, these days would disagree with the theory that it's vital to take time for yourself. Creating some space for enjoyment and restoration each day or atleast every week, is a win-winproposal: it’ll make you both happier and more effective in fulfilling your responsibilities at work andhome. In practice, itrarely happens, though. For some, that's because deep down they feet they don'tdeserve it. For others, it's simply that busy life makes it seem impossible to presspause. Either way,making sure you actually get a. moment to yourself requires a shift in perspective.Don't wait until it feels right. It's unpleasant to have unfinished tasks bothering at your mind, soit's tempting to tell yourself you'll only relax once everything is under control. But since both workand family life generate an infinite number of to-dos, that strategy is doomed to failure. Astime-management writer Laura Vanderkarn points out, it's far more useful to learn to tolerate thediscomfort of knowing your email inbox is filling up, or that the living room is still a pigsty. Choose true enjoyment. It's all too easy to fill `me time' with things you think you should enjoy,above all exercise. If you genuinely love such activities, they're perfect. But if the truth is that youdon't, you'll only get resentful: we rebel against being told what to do, even when the person doingthe telling is ourselves. Make sure at least a small part of your week is spent doing something you canhonestly say you enjoy for itself.Pay attention to good feelings. Once you do get some restorative time, borrow a Buddhist technique for making it count: when you realize you're enjoying yourself, spend half a minuteconsciously paying attention to the feelings of pleasure. For one thing, you'll often find that thosefeelings increase as a result. For another, you'll encode the memory of the experience in more detailso, looking back, it'll feel like you had even more time to yourself.32. Why is it hard for some people to find time for themselves practically?A. They think they aren't worth itB. They have a lot of pressure.C. They are in financial trouble.D. They can't spare any time33. Which of the following is acceptable according to Paragraph two?A. Never put off what you should do.B. Take a rest when it's time toC. Relax yourself with all work done.D. Put up with others' shortcomings.34. Which is the closest to "resentful" in paragraph three?A. pleased.B. relaxed.C. relieved.D. annoyed.35. What is best title of the passage?A. Learn to Manage TimeB. Find Time for YourselfC. Squeeze Time to ExerciseD. Strengthen Time ConsciousnessABDB。
《⾼级英汉翻译》课程终结考试试卷(样题及答案和评分标准)Get ready for the final exams of English/ChineseTranslation (1&2)Part I E-C Translation Test1. Composition of the Test Papers & useful skills in coping with the tests“⾼级英汉翻译”课程●评价⽬标:重点测试学⽣英汉笔译的技巧,包括增译法、减译法、词类转移法、词序调整法、分译法、重译法、正说反译,反说正译法和习语翻译等。
同时也考查相关的翻译理论知识、英语理解和汉语表达能⼒。
●命题原则:根据教材所涵盖的⽂章主题、体裁、翻译技巧以及与教材难度相当的书⾯语⾔材料命题。
英译汉的课外材料必须是从英语原著上选来的未经简化的⽂字。
涉及教材内容不少于50%。
●试题结构:“⾼级英汉翻译”课程终结考试试卷(样题)课程编号:ENBAE3 1001______ 学籍号:________________ 学习中⼼:________________ 姓名:________________ Information for the Examinees:This examination consists of FOUR sections. They are:Section I: Understanding of Theories (10 points, 15 minutes)Section II: Phrase Translation (25 points, 20 minutes)Section III: Sentence Translation (30 points, 25 minutes)Section IV: Passage Translation (35 points, 60 minutes)The total marks for this examination are 100 points. Time allowed forcompleting this examination is 2 hours (120 minutes)YOU MUST WRITE ALL YOUR ANSWERS ON THE ANSWER SHEET. Section I Understanding of Theories[10 points] Questions 1-10. (10 points)The following statements are about some translation theories you are familiar with. Decide whether these statements are true or false by writing T for "true" and F for "false" on your Answer Sheet.______1. Since Chinese and English belong to two different language families, one has to make some adjustments in lexicon and sentence structure to make the translated version smooth and natural.______2. Translating consists in reproducing in the receptor language the closest natural equivalent of the source-language message, first in terms of meaning and second in terms of style.______3. Every language adopts the same system of classifying its experience.______4. It widely agreed that there are three stages in the procedure of translation: analysis, transfer, and restructuring.______5. A word may have several meanings, but its linguistic context will help to point out the exact meaning of that word. ______6. Semotactic marking, one aspect of linguistic context, refers to the situation when the meaning of a word in a sentence is specified by the grammatical construction of that sentence.______7. In translating from English to Chinese, one must repeat key words including nouns, verbs, and pronouns.______8. In the process of transfer, the conceptual content of the message has the highest priority. Therefore, there is no need to keep the original form of the source-language text.______9. The situational factors relate to the occasion and circumstances of the speech event and to the relationships between speakers.______10. Nida believes that in testing the translation, one must focus attention not upon the extent of verbal correspondence but upon the amount of dynamic equivalence.Section II Phrase Translation[25 points]Part 1. Questions 11-20. (10 points)Choose a better version of Chinese translation for each of the following phrases. Write your answers on the Answer Sheet.11. the journey across AfricaA. 遍及⾮洲的旅⾏B. 穿越⾮洲的旅⾏12. be behind scheduleA. 落后于计划B. 在计划后⾯13. play the fluteA. 玩笛⼦B. 吹笛⼦14. black teaA. 红茶B. ⿊茶15. like a cat on hot bricksA. 烫砖上的猫B. 热锅上的蚂蚁16. a concept inconceivable beforeA. ⼀个以前⽆法想象的概念B. ⼀个概念,在以前⽆法想象17. Dutch treatA. 打平伙B. 荷兰式的招待18. political campaignA. 政治运动B. 竞选活动19. mountain lionA. ⼭狮B. 美洲豹20. an instrument designed to extend the range of people's sensesA. ⼀个⽤来拓展⼈们感觉范围的⼯具B. ⼀个⼯具,⽤来拓展⼈们的感觉范围Part 2. Questions 21-30. (15 points)Translate the following phrases and write your answers on the Answer Sheet.21. a hard question ____________________22. hard water ____________________23. the last ten-day period of a month ____________________24. a good Christian ____________________25. a well-managed company ____________________26. particles moving around their atomic nucleus ____________________27. generations of painstaking observation ____________________28. an unlikely coalition of university professors ____________________29. a computer genius ____________________30. as much with courtesy as with force ____________________Section III Sentence Translation [30 points]Questions 31-40: Translate the following sentences using the translation skills and techniques you have learned from this course. Write your answers on the Answer Sheet.31. Nobody could count on his restraint or rationality.____________________________________________________________32. Modern skyscrapers began to appear in the city, taking away much of its ancient charm and mystery, which was considered as a great pity by many people.____________________________________________________________33. The news had already spread along the streets and lanes.____________________________________________________________34. The examination left no doubt that the victim had not died of a heart attack but had been killed.____________________________________________________________35. There was no use arguing. The die was cast.____________________________________________________________36. Twentieth century history shows the impressive adaptive capacity of international relations based on multinational principles and norms.____________________________________________________________37. We are very grateful to you for your effort to come all the way from China to present his document to us.____________________________________________________________38. The problem of refugees should be dealt with in an integrated manner.____________________________________________________________39. It is exciting to visit your great country.____________________________________________________________40. No one was more willing to do a favor for friend or neighbour than he.____________________________________________________________Section IV Passage Translation[35 points]Part 1. Question 41. (15 points)The following passage is about problems with Darwinian Theory. Please translate it into Chinese on your Answer Sheet. You may refer to the new words and expressions provided in the box below.If Darwinian Theory works so well, why challenge it? There are several reasons to do so. Although Darwinian Theory explains many of the facts of evolution better than any other theory, it does not necessarily explain the whole process. Also, some of the results of evolution do not match what Darwinian Theory would predict.For example, if evolution leads to a perfect adaptation through natural selection acting on random hereditary changes, the process ought to slow down as it gets closer to the optimum for each species because fewer favorable changes can be made. Indeed, someorganisms-cockroaches and sponges, for example, are so well adapted that they have changed very little in many millions of years.Their evolutionary rate does seem to have slowed down. We should also see decrease in the number of species as they compete with one another and unsuccessful species are eliminated. But we see no such slowing down, and the number of species appears to be at least as great now as in the geologic past and perhaps even greater.Part 2. Question 42. (20 points)The following passage is an excerpt from a book talking about the special joys of slow reading. Please translate it into Chinese on your Answer Sheet.I discovered the worth of super-slow reading years ago. Previously, if I had been really interested in a book, I would race from page to page, eager to know what came next. Now, I decided, I had to become a miser with words and stretch every sentence like a poor man spending his last dollar. I had started with the practical object of making my book last. But by the end of the second week I began to realize how much I was getting fromsuper-slow-reading itself. Sometimes just a particular phrase caught my attention, sometimes a sentence. I would read it slowly, analyze it, read it again-perhaps changing down into an even lower gear-and then sit for 20 minutes thinking about it before moving on. I was like a pianist studying a piece of music, phrase by phrase, rehearsing it, trying to discover and recreate exactly what the composer was trying to convey.参考答案与评分标准(样题)Section I Understanding of Theories[10 points] Questions 1-10. (10 points, 1 point each)1.T2.T3. F4.T5.T6. F7. F8. F9.T 10.T Section II Phrase Translation[25 points] Part 1. Questions 11-20. (10 points, 1 point each) 11. B 12. A 13. B 14. A 15. B16. A 17. A 18. B 19. B 20. APart 2. Questions 21-30. (15 points, 1.5 points each.)Marking guide:评分标准(共15分,每个1.5分):1.译⽂应准确、完整。
基因的重要性英语作文The significance of genes in our lives is immense and it is a topic that has garnered considerable attention in the scientific community and beyond. Here is an essay on the importance of genes in EnglishTitle The Importance of GenesIntroductionGenes are the fundamental units of heredity carrying the information that determines the traits and characteristics of living organisms. They are segments of DNA located on chromosomes within the nucleus of a cell. The understanding of genes has revolutionized the fields of biology medicine and agriculture and continues to shape our understanding of life itself.Body Paragraph 1 Genetic Influence on HealthOne of the most profound impacts of genes is on human health. Genetic disorders such as cystic fibrosis sickle cell anemia and Huntingtons disease are caused by mutations in an individuals DNA. The study of these genetic conditions has led to advancements in genetic testing and counseling allowing for early detection and sometimes prevention of these diseases. Moreover the knowledge of how genes influence susceptibility to common illnesses like cancer and heart disease has paved the way for personalized medicine where treatments are tailored to an individuals genetic profile.Body Paragraph 2 Genetic Diversity and EvolutionGenetic diversity is crucial for the survival and adaptation of species. It provides the raw material for natural selection to act upon leading to the evolution of new traits that can enhance an organisms ability to survive in its environment. The study of genetic variation has also shed light on the evolutionary relationships between different species helping us understand the history of life on Earth.Body Paragraph 3 Genetic Engineering and AgricultureIn agriculture genetic engineering has allowed for the development of crops that are more resistant to pests diseases and environmental stress. This has increased crop yields andreduced the need for chemical pesticides which is beneficial for both the environment and human health. Additionally genetic modification can enhance the nutritional content of food addressing malnutrition in parts of the world where certain nutrients are scarce.Body Paragraph 4 Ethical Considerations and Future ProspectsWhile the benefits of genetic research are vast they also raise ethical questions. The potential for genetic discrimination where individuals are treated differently based on their genetic information is a concern. Furthermore the possibility of designer babies where parents select traits for their children raises questions about the moral implications of such choices. As we delve deeper into the realm of genetics it is essential to have ongoing discussions about the ethical use of this powerful knowledge.ConclusionIn conclusion genes are the building blocks of life and their study has opened up new frontiers in science and medicine. They influence our health our understanding of the natural world and even our food supply. As we continue to unlock the secrets of the genome it is imperative that we do so responsibly considering the ethical implications and ensuring that the benefits of genetic knowledge are accessible to all. The importance of genes is not just scientific it is a key to our future.。
2023—2024 学年度第一学期期末学业水平诊断高二英语注意事项:1. 答卷前, 考生务必将自己的姓名、考生号等填写在答题卡和试卷指定位置上。
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第一节(共5小题; 每小题1.5分, 满分7.5分)听下面5段对话。
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1. What is the man doing?A. Planning a trip.B. Giving some advice.C. Sharing his travel experiences.2. What time is it now in Beijing?A. 8:30 p. m.B.5:30 a. m.C.11:30 a. m.3. What is the weather like now?A. Sunny.B. Cloudy.C. Windy.4. What's the relationship between the speakers?A. Salesman and customer.B. Boss and employee.C. Husband and wife.5. Why does the woman want to borrow money?A. To buy clothes.B. To make a donation.C. To get a pair of shoes.第二节(共15小题; 每小题 1.5分, 满分22.5分)听下面5 段对话或独白。
a r X i v :0806.0618v 2 [a s t r o -p h ] 8 J u l 2008Mon.Not.R.Astron.Soc.000,000–000(0000)Printed 8July 2008(MN L A T E X style file v2.2)Testing the evolutionary link between submillimetregalaxies and quasars:CO observations of QSOs at z ∼2K.E.K.Coppin 1, A.M.Swinbank 1,R.Neri 2,P.Cox 2, D.M.Alexander 3,Ian Smail 1,M.J.Page 4,J.A.Stevens 5,K.K.Knudsen 6,R.J.Ivison 7,8,A.Beelen 9,F.Bertoldi 6,A.Omont 101Institute for Computational Cosmology,Durham University,South Road,Durham,DH13LE 2Institut de RadioAstronomie Millim´e trique (IRAM),300rue de la Piscine,Domaine Universitaire,38406Saint Martin d’H`e res,France 3Department of Physics,Durham University,South Road,Durham,DH13LE4UCL,Mullard Space Science Laboratory,Holmbury St.Mary,Dorking,Surrey RH56NT5Centre for Astrophysics Research,University of Hertfordshire,College Lane,Hatfield,AL109AB 6Argelander-Institut f¨u r Astronomie,University of Bonn,Auf dem H¨u gel 71,D-53121Bonn,Germany7Institute for Astronomy,University of Edinburgh,Royal Observatory,Blackford Hill,Edinburgh,EH93HJ 8UK Astronomy Technology Centre,Royal Observatory,Blackford Hill,Edinburgh,EH93HJ 9Institut d’Astrophysique Spatiale,Universit´e Paris-Sud,F-91405Orsay,France 10Institut d’Astrophysique de Paris,Universit´e Pierre &Marie Curie,98bis Boulevard Arago,F-75014Paris,France8July 2008ABSTRACTWe have used the IRAM Plateau de Bure millimeter interferometer and the UKIRT 1–5µm Imager Spectrometer (UIST)to test the connection between the major phases of spheroid growth and nuclear accretion by mapping CO emission in nine submillimetre-detected QSOs at z =1.7–2.6with black hole (BH)masses derived from near-infrared spectroscopy.When combined with one QSO obtained from the literature,we present sensitive CO(3–2)or CO(2–1)observations of 10submillimetre-detected QSOs se-lected at the epoch of peak activity in both QSOs and submillimetre (submm)galaxies (SMGs).CO is detected in 5/6very optically luminous (M B ∼−28)submm-detected QSOs with BH masses M BH ≃109–1010M ⊙,confirming the presence of large gas reser-voirs of M gas ≃3.4×1010M ⊙.Our BH masses and dynamical mass constraints on the host spheroids suggest,at face value,that these optically luminous QSOs at z =2lie about an order of magnitude above the local BH-spheroid relation,M BH /M sph ,al-though this result is dependent on the size and inclination of the CO-emitting region.However,we find that their BH masses are ∼30times too large and their surface density is ∼300times too small to be related to typical SMGs in an evolutionary sequence.Conversely,we measure weaker CO emission in four fainter (M B ∼−25)submm-detected QSOs with properties,BH masses (M BH ≃5×108M ⊙),and surface densities similar to SMGs.These QSOs appear to lie near the local M BH /M sph rela-tion,making them plausible ‘transition objects’in the proposed evolutionary sequence linking QSOs to the formation of massive young galaxies and BHs at high-redshift.We show that SMGs have a higher incidence of bimodal CO line profiles than seen in our QSO sample,which we interpret as an effect of their relative inclinations,with the QSOs seen more face-on.Finally,we find that the gas masses of the four fainter submm-detected QSOs imply that their star formation episodes could be sustained for ∼10Myr,and are consistent with representing a phase in the formation of mas-sive galaxies which overlaps a preceding SMG starburst phase,before subsequently evolving into a population of present-day massive ellipticals.Key words:galaxies:high-redshift –galaxies:evolution –galaxies:formation –galaxies:kinematics and dynamics –quasars:emission lines –submillimetre2Coppin et al.1INTRODUCTIONIt has been established that every massive,local spheroid harbours a supermassive black hole(SMBH)in its cen-tre whose mass is proportional to that of its host(e.g. Magorrian et al.1998;Gebhardt et al.2000).This suggests that the black holes(BHs)and their surrounding galaxies were formed synchronously.This hypothesis has found sup-port from hydrodynamical simulations of galaxy formation, which use feedback from winds and outflows from active galactic nuclei(AGN)to link the growth of the SMBH to that of its host(e.g.Di Matteo,Springel&Hernquist2005; Hopkins et al.2005;Bower et al.2006).Thus these models support a picture,first presented by Sanders et al.(1988), where a starburst-dominated ultra-luminous infrared galaxy (ULIRG),arising from a merger,evolvesfirst into an ob-scured QSO and then into an unobscured QSO,beforefi-nally becoming a passive spheroid.The high-redshift population of ULIRGs in this proposed evolutionary cycle are the submillimetre (submm)galaxies(SMGs;Smail,Ivison&Blain1997; Chapman et al.2005;Coppin et al.2006).These systems have ULIRG-like bolometric luminosities,L IR≥1012L⊙(Kov´a cs et al.2006;Coppin et al.2008),and they have many of the properties expected for gas-rich mergers (Swinbank et al.2004,2006;Tacconi et al.2006).This population evolves rapidly out to a peak at z∼2.3,crudely matching the evolution of QSOs(Chapman et al.2005) and providing additional circumstantial evidence for a link between SMBH growth and spheroids.Two further results have shed light on the evolutionary link between SMGs and QSOs.Firstly,a modest fraction of optically luminous QSOs at z∼2are detected in the submm/mm (∼(25±10)%;Omont et al.2003)showing that the QSO-and SMG-phases do not overlap significantly,given the lifetime estimates of the two populations(QSOs make up ∼4%offlux-limited samples of SMGs;Chapman et al. 2005).But when a QSO is detected in the submm/mm then it could to be in the transition phase from an SMG to an unobscured QSO,making its properties a powerful probe of the evolutionary cycle(e.g.Stevens et al.2005;Page et al. 2004).Secondly,the evolutionary state of the SMBHs within SMGs can also be judged using the2-Ms Chandra Deep Field North observations(Alexander et al.2003)to derive accurate AGN luminosities and hence lower limits on the BH masses(M BH)in those SMGs with precise redshifts in this region(Alexander et al.2005a,b;Borys et al.2005). These studies suggest that the AGN in typical SMGs are growing almost continuously–but that the SMBHs in these galaxies appear to be several times less massive than seen in comparably massive galaxies at z∼0(Alexander et al. 2008).Together these results argue for a fast transition from a star-formation-dominated SMG-phase to the AGN-dominated QSO-phase(Page et al.2004).The latter phase will result in the rapid BH growth necessary to account for the present-day relation between spheroid and SMBH masses(e.g.Magorrian et al.1998;Gebhardt et al.2000). Can we confirm this and more generally test the proposed evolutionary link between SMGs and QSOs at the peak of their activity at z∼2?verse by comparing the properties of QSOs and ULIRGs (e.g.Tacconi et al.2002).However,both of these popula-tions are1000×less abundant in the local Universe than they were at the era of their peak activity at z∼2and so we have to be cautious about extrapolating from local examples to the high-redshift progenitors of the bulk of to-day’s massive spheroids(Genzel et al.2003;Swinbank et al. 2006).Thus,to properly test the validity of this cycle for typical spheroids we have to compare QSOs and ULIRGs at the era where their populations peaked:z∼2.The critical pieces of information needed to test the link between SMGs and QSOs are the relative dynamical, gas and SMBH masses of these two populations.In prin-ciple the dynamical masses can be derived from optical or near-infrared observations of emission line gas in the SMGs or QSOs(see Swinbank et al.2004,2005,2006).However, there is the problem of removing the QSO emission in these observations,as well as the effects of dust obscuration and outflows.In contrast,molecular CO emission line profiles are relatively immune to the effects of obscuration and out-flows,while at the same time yielding additional constraints on the relationship between QSOs and SMGs from their gas masses.There is currently a lack of sensitive CO observations of QSOs at z∼1–3,with data published on only eight sources (e.g.Frayer et al.1998;Guilloteau et al.1999;Beelen et al. 2004;Hainline et al.2004).Instead the focus has been on CO studies of QSOs at z>∼4(e.g.Omont et al.1996; Walter et al.2004;Riechers et al.2006),although these QSOs have little overlap with the redshift range where SMGs are typically detected.The paucity of CO constraints for z>1QSOs also reflects the difficulty in determining their systemic redshifts with sufficient precision to guarantee that the CO emission falls within the bandwidth of typical mil-limetre(mm)correlators.However,sensitive near-infrared spectroscopy of the C iv,Mg ii,and[O iii]5007emission lines in QSOs can provide redshifts with required precision as well as Hαor Hβfluxes and line widths to yield M BH estimates (Takata et al.2006;Alexander et al.2008).We have carried out a quantitative test of the proposed link between SMGs and QSOs at z∼2where both popula-tions are most common.We have obtained precise systemic redshifts from near-infrared spectroscopy of potential transi-tion QSOs(i.e.submm/mm-detected QSOs)and then used the IRAM Plateau de Bure Interferometer(PdBI)to search for CO emission.We relate their dynamical,gas and SMBH masses to SMGs from the PdBI CO survey(Greve et al. 2005).We test:a)whether the cold gas masses in these QSOs are similar to those in SMGs;b)whether the line widths and dynamical masses of these two populations are comparable; and c)how the ratio of SMBH to dynamical masses for these submm-detected QSOs relate to the estimates for SMGs and those for optically luminous QSOs(which lie on the present-day M BH–Mσrelation;McLure&Dunlop2004).Together these observations can constrain the proposed evolution-ary sequence which links QSOs to the formation of massive young galaxies and SMBHs at high redshift.We describe the sample selection,observations and data reduction in§2.The results of the near-infrared and mm CO spectra are given in§3.The CO properties of the submm-detected QSOs are compared and contrasted withGas and BHs of QSOs and SMGs at z ∼231618202224R magR e d s h i f tFigure 1.R -band apparent magnitude versus redshift for our sample of submm-detected QSOs.We show that these lie within the interquartile range (shaded region)of the redshift distribution of SMGs (median <z >≃2.3;dashed line)from Chapman et al.(2005).This shows that we are probing a wide range in optical luminosities (and potentially a wide range in M BH )at the epoch where the QSO and SMG populations peak.submm-detected QSOs in §5.Our conclusions are given in §6.We adopt cosmological parameters from the WMAP fits in Spergel et al.(2003):ΩΛ=0.73,Ωm =0.27,and H 0=71km s −1Mpc −1.All quoted magnitudes are on the Vega system.2OBSER V ATIONS,REDUCTION AND REDSHIFTS 2.1Sample SelectionThe objective of this study is to test the link between SMGs and QSOs at the era where these populations peaked.We have therefore selected radio-quiet QSOs with a redshift distribution matched to SMGs ( z ∼2.3,Chapman et al.2005)and with 850µm fluxes >∼5mJy.The S 850µm >∼5mJy flux limit selects comparatively bright QSOs and SMGs and is imposed so that the sources would be sufficiently bright to be detected in CO.We choose submm-detected QSOs from three main samples:we select five QSOs from a submm photometry survey of optically-bright QSOs by Omont et al.(2003)–HS1002+4400,J140955.5+562827,J154359.3+535903,HS1611+4719,and J164914.9+530316,we select two QSOs from the submm photometry sur-vey of X-ray absorbed QSOs by Stevens et al.(2005)–RXJ121803.82+470854.6and RXJ124913.86–055906.2,and finally we include two QSOs found in blank-field submm surveys by Chapman et al.(2005)and Greve et al.(2004),SMM J131222.35+423814.1and MM J163655+4059,selected QSO targetted in submm photometry mode by Chapman et al.(2005).The final sample comprises 10submm-detected QSOs with similar fluxes to the SMG sample (Greve et al.2005;>∼5mJy at 850µm,assuming 850µm/1.2mm colours typi-cal of SMGs;Greve et al.2004),with a median of 10mJy.The SEDs of these QSOs demonstrate that the bulk of the mm/submm luminosity arises from dust emission and is very likely associated with star formation,rather than an AGN (Beelen et al.2006;Omont et al.2003).Our sample spans six orders of magnitude in QSO R -band brightness,enabling us to potentially trace how CO properties depend on QSO luminosity or M BH (see Fig.1).2.2Near-Infrared SpectroscopyThe QSOs in this sample were spectroscopically identi-fied through rest-frame UV spectroscopy.However,since the rest-frame UV emission lines can be extremely broad (FWHM ∼5000km s −1),and can be offset in velocity with respect to the systemic redshift,precise systemic redshifts are required to ensure the CO emission falls within the PdBI receiver bandwidth.To obtain precise systemic redshifts for our targets we use the nebular emission lines of [O iii ]λ5007and H βwhich are redshifted to near-infrared wavelengths.Seven of our submm-detected QSOs were observed with the United Kingdom InfraRed Telescope (UKIRT)1–5µm Imager Spectrometer (UIST;Howatt et al.2004).We used the HK grism which provides a spectral resolution of λ/∆λ∼1000and covers a wavelength range 1.4–2.4µm,thus allowing us to cover H β,[O iii ]λ4959,5007and H αsi-multaneously for most of our QSOs.The QSOs were ob-served between 2006Feb and 2006Oct.All observationswere taken in <∼0.8′′seeing and clear conditions,and were carried out using the standard ABBA configuration where the QSO was nodded by 6–12′′along the slit to achieve sky subtraction.Individual exposures were 240s and the total integration times varied between 1.2ks and 4.8ks depend-ing on the K -band magnitude of the QSO (see Table 1).In addition,three QSOs in our sample have suitable archival spectroscopy from Takata et al.(2006)and Swinbank et al.(2004,2006).The relevant orac-dr pipeline (Cavanagh et al.2003)was used to sky-subtract,extract,wavelength calibrate,flat-field and flux calibrate the data (and in the case of integral field unit observations,forms the datacube).Spectra for the QSOs in our sample are shown in Fig.2.To derive systemic redshifts,we simultaneously fit the H βand [O iii ]λ4959,5007emission lines with Gaussian profiles.The emission line flux ratio of the [O iii ]λ4959,5007emission lines is fixed such that I 4959/I 5007=2.9,and the [O iii ]λ4959,5007line widths are as-sumed to be the same.The fit assumes a linear continuum plus Gaussian emission line profiles allowing the velocity centroid,flux and width of the H βline profile to be dif-ferent from [O iii ].This makes a total of seven parameters to be fitted.We also derive emission line fluxes and widths for the H αemission line (which are important for deriving M BH using the method of Greene &Ho 2005)in a similar manner,fitting a single Gaussian emission line profile superimposed on a linear continuum.The resulting redshifts and fluxes are given in Table 2.These redshifts were subsequently used to4Coppin et al.Table1.Summary of the new near-infrared spectroscopy and mm-wave PdBI CO observations of submm-detected2<z<3QSOs,including nine new CO observations and one published object from Beelen et al.(2004).The CO t exp corresponds to the on-sourceintegration time with the equivalent of a6-element array.Date(s)t exp Dates t exp Noise per channel f Beam FWHM Detected?(ks)(hrs)(mJy beam−1)Notes:(a)All observed in the CO(3–2)transition,except for RXJ121803.82+470854.6observed in CO(2–1)(b)From UIST spectroscopy(this work)(c)From Swinbank et al.(2004)(d)From Takata et al.(2006)and Alexander et al.(2008)(e)From Beelen et al.(2004)(f)With a channel width of20MHzDue to the very weak[O iii]λ5007emission in RXJ124913.86,it was very difficult to measure a reliable redshift for the CO observations,and thus a range of possi-ble redshifts were covered on this QSO(z∼2.24–2.26).During the course of assembling the data for this project,we obtained a CO detection of HS1611after se-curing a systemic redshift from identification of[O iii]with UIST.The positional centroid of the CO was offset by ∼1.3arcsec north of the optical and near-infrared QSO po-sition,possibly indicating a companion,and HS1611was re-observed with the UIST integralfield unit(IFU)for a total of3.6ks on2006Sep01.The UIST IFU uses an im-age slicer to take a3.3′′×6.0′′field and divides it into14 slices of width0.24′′.The dispersed spectra from the slices are reformatted on the detector to provide two-dimensional spectro-imaging,in our case also using the HK grism.We reduced the data using the relevant orac-dr pipeline which extracts,flatfields,wavelength calibrates the data and forms the datacube.We discuss these data in§3.1.8.2.3Millimetre InterferometryWe surveyed seven QSOs for CO emission using IRAM PdBI between2006June to2007June and two QSOs between 2001December and2002April in conditions with good at-mospheric phase stability and reasonable transparency.The observations were carried out using3,4,5,and6anten-nae in the D configuration,giving a total of3,6,10,and 15baselines,respectively.For uniformity with the previous observations observations of SMGs,which will comprise our comparison sample,we have aimed to achieve the same1-σsensitivity as for the SMG survey(Greve et al.2005)for the new CO observations of our sample of submm-detected QSOs:S CO∆v∼0.3Jy km s−1.We also include results on a single QSO from the literature,J140955.5from Beelen et al. (2004),to yield afinal sample of10QSOs.The PdBI obser-vations are summarised in Table1.For data taken prior to2007January,the spectral corre-tion of2.5MHz at a bandwidth of580MHz.For data taken after January2007,the spectral correlator was adjusted to detect the line with a frequency resolution of2.5MHz in the 1GHz band of the new generation receivers.The visibilities were resampled to a frequency resolution of5MHz.The data were calibrated,mapped and analyzed in the IRAM gildas1software package(Guilloteau&Lucas 2000).Anomalous and high phase-noise visibilities were flagged.Passband calibrations were typically made using a nearby bright quasar.Phase and amplitude calibration within each observation were calibrated using frequent ob-servations of nearby quasars approximately every20min. Theflux calibration was done using standard calibrators,in-cluding3C273,MWC349,1637+574,1749+096,0923+392, 1243-072,and CRL618,for example.We estimate a conser-vative error on theflux calibration of10–15%.For each QSO the central observing frequency of the 3.1mm band receiver was tuned to either the redshifted CO(3–2)or CO(2–1)rotational transition,depending on the systemic near-infrared redshift derived from our spec-troscopy given in Table2.In the case of RXJ124913.86, the uncertainty on the redshift was large enough that we performed two separate observations with different central frequency tunings of106.160and106.720GHz to ensure that the CO(3–2)line was covered.We have combined these data to cover more effective bandwidth and have centered the resulting spectrum at the mean central observed fre-quency,106.435GHz,corresponding to CO(3–2)redshifted to z≃2.2487.Naturally weighted datacubes were made and inspected for line emission close to the QSO position.Fig.3shows the velocity-integrated mm emission maps over the line in each field.In Fig.4,we show the spectra of the CO emission in the brightest pixel of the central source in each velocity-integrated mm emission map,centered on the systemic red-shift of each system.We have included the maps and spec-Gas and BHs of QSOs and SMGs at z ∼25Figure 2.Restframe UV–near-infrared spectra for our sample of submm-detected QSOs.The insets show the region around the H βand [O iii ]λ5007emission lines (all insets cover the wavelength range 4675–5100˚A ),except in the case of J163655,and the redshifts derived from the [O iii ]λ5007emission are indicated.The redshift for J163655was taken from the redshifted H αdue to ambiguity in the [O iii ]λ5007emission lying near the edge of the wavelength coverage of the spectrograph;the inset therefore shows the region around H α.The region around 5100–5500˚A in J1409has been masked due to strong atmospheric absorption.tra of non-detections and in the latter cases we show the maps averaged over the central 500km s −1of the spectra (the average line width of our sample)and spectra extracted at the phase tracking centre (or at the continuum peak for J164914.9).In all cases,we ignore the small correction for the primary beam attenuation,given that the detected sources are all close to the phase centres of the maps.3ANALYSIS AND RESULTS 3.1CO propertiesWe present new CO data for nine QSOs,including five new CO detections.Four of our QSOs have CO detections with S/N >∼5,and an additional QSO is marginally detected in CO with S/N ≃2.5with emission coincident with the phase centre (see Fig.4).None of the QSOs appear to be resolved a previous CO detection reported by Beelen et al.(2004)in our sample of submm-detected QSOs.In total therefore this gives six detections in our sample of 10QSOs,yielding a detection rate comparable to that for SMGs by Greve et al.(2005)of ∼60%.Looking at the non-detections,it is unlikely that the cause of the failure to detect CO emission in these four QSOs is due to the systemic redshifts being wrong,as the quality of the optical/near-infrared spectral data for these is high and similar to the successful detections (see Fig.2).Similarly,it is unlikely that the velocity offset of the CO emission and the systemic redshift are larger than the correlator coverage (the rms deviation of z NIR and z CO for our CO-detected QSOs is 0.0046),since only a few systems detected at high-redshift so far show larger offsets (e.g.Hainline et al.2004).It is also unlikely that the CO line widths are ≫1000km s −1since our typical detected lines are 550km s −1which is6Coppin et al.CO line widths could be one reason for some of the non-detections,the most likely reason appears to be that the QSOs are simply too faint in CO to be detected given the depth of our observations.However,the non-detections do still provide useful upper limits on the CO luminosity and gas masses and therefore we include them in our analysis.Other than one QSO(J164914.9;§3.1.10),we do not detect the continuum at3.1mm in any of the QSOs.This is consistent with the measured submm/mmfluxes and grey-body dust emission with a spectral form Sν∝ν2+βin the Rayleigh-Jeans regime of the spectral energy distribution with a dust emissivityβ=1.5.The luminosity,velocity width and spatial extent of the CO line emission can be used to place limits on the gas and dynamical mass of each system.For each CO-detected QSO a Gaussian profile isfit to either20-or30-MHz binned data by minimising theχ2statistic.The1σerrors on the best-fitting parameters are quoted where appropriate.To calcu-late the velocity-integratedflux density of the CO emission, we integrate the best-fitting Gaussian profile(note that we do notfit the line and continuum simultaneously).The error on the velocity-integratedflux density is calculated by boot-strapping from a Normal distribution centered on the best fitting amplitude above,with a width given by the1σerror in thefitted amplitude,while holding the FWHM and cen-tral velocity of the best-fitting Gaussian profilefixed.The noise in the averaged channel maps,constructed from the av-erage emission over the full width at zero intensity(FWZI) in each QSO,is determined by summing over the weights and takes into account the phase noise visibilities.For the non-detections we calculate3σupper lim-its S CO=3σ(δv∆v FWHM)1/2,whereσis the channel-to-channel rms noise,δv is the velocity resolution and ∆v FWHM is the line width(see e.g.Greve et al.2005; Seaquist,Ivison&Hall1995).We use the channel-to-channel rms noise of the spectra binned to a resolution of 100MHz and adopt a line width of500km s−1.Since our de-tections have typical line widths 550km s−1,this is a con-servative assumption.In addition,this line width assump-tion facilitates the direct comparison of our non-detections with those of SMGs in Greve et al.(2005).We have summarised the line properties of each source (the CO position,z CO,L′CO(3−2)and FWHM)in Tables3 and4.Offsets of the CO emission from the radio position are given in Table3,assuming that the source is unresolved us-ing equation B2in Ivison et al.(2007),and are less than2σsignificant in most cases.We note that we discover serendip-itous>∼4σsources in two of thefields surveyed which may be associated with gas-rich companions to the QSOs (SMM J123716.01and SMM J131222.35).Overdensities of submm sources have already been found by Stevens et al. (2004)around similar QSOs on slightly bigger scales than those probed here.We now discuss the CO properties of each QSO detection and non-detection in detail,as well as any serendipitous detections.3.1.1HS1002+4400The integrated CO emission in this QSO is detected at ≃6σ,0.8′′north of the Sloan Digital Sky Survey(SDSS; Fan et al.1999)position(see Fig.3).The CO(3–2)spec-olution of20MHz(54km s−1)and is shown in Fig.4.The CO emission line is wellfitted by a Gaussian profile with a FWHM of640±160km s−1,a velocity-integratedflux den-sity of S CO(3−2)=1.7±0.3Jy km s−1,and a CO redshift of z CO=2.1015±0.0007,offset by20±65km s−1from the near-infrared systemic redshift.No significant contin-uum emission is detected from the line-free region down to a1-σlimit of0.4mJy.3.1.2RXJ121803.82+470854.6Neither CO(2–1)emission at the systemic redshift nor con-tinuum emission are seen in the map near the QSO posi-tion.To calculate a3σupper limit to the velocity-integrated CO(2–1)lineflux of RXJ121803.82,we extract a spectrum at the QSO position(Table2)and rebin the spectrum to a frequency resolution of100MHz(360km s−1),resulting ina channel rms of0.5mJy,and so derive an upper limit of0.6Jy km s−1,assuming a line width of500km s−1,centred on the z NIR=1.7416.No significant continuum emission is detected down to a1-σlimit of0.2mJy.We dofind two≃4σserendipitous detections in the datacube,offset in velocity from the central frequency tun-ing,and approximately10-20arcsec away from the phase centre.Neither show strong broad line detections in the spec-tra extracted at the peak locations,so we believe these are unlikely to be true sources.3.1.3SMM J123716.01+620323.3Neither CO(3–2)emission nor continuum emission are seen in the datacube near the QSO position.To calculate a3σupper limit to the velocity-integrated CO(3–2)lineflux, we extract a spectrum at the radio position(Table2)and rebin the spectrum to a frequency resolution of100MHz (270km s−1),resulting in a channel rms of0.2mJy,giving an upper limit of0.3Jy km s−1,assuming a line width of 500km s−1at the systemic redshift from[O iii]λ5007(Ta-ble2).No significant continuum emission is detected down to a1-σlimit of0.2mJy.Wefind a≃4σdetection in the datacube,offset in velocity from the central frequency tuning and approxi-mately18arcsec2south of the nominal pointing position at123715.36,620306.5(J2000),indicating a redshift of z CO=2.0597±0.0001,which is close to the QSO z NIR, suggesting it may be a gas-rich companion of the QSO with a separation of170kpc.See Fig. 5.This position corresponds to within0.5arcsec of an I=24.7counter-part(Smail et al.2004)with a radioflux of≤15µJy (Biggs&Ivison2006)which is also undetected in the Chan-dra observations(Alexander et al.2003).The CO line has an integratedflux of S CO(3−2)=0.2±0.06Jy km s−1and is very narrow(FWHM=100±30km s−1).2Note that the map noise at this distance from the phase centre is only slightly degraded since the primary half power beam width。