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无编辑摘要  | 
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| (未显示同一用户的38个中间版本) | |||
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==句式==  | 
  ==句式==  | 
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*A description of the relevant processes and related parameters is given below.  | 
  *A description of the relevant processes and related parameters is given below.  | 
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:give descriptions of 不用 make descriptions on  | 
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*Although ... is the result of a complex interplay among a variety of different physical processes, we can still capture some basic trends.  | 
  *Although ... is the result of a complex interplay among a variety of different physical processes, we can still capture some basic trends.  | 
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*Contains a wealth of information that has not yet been exploited  | 
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*Effectively, the ... can be considered as a free parameter.  | 
  *Effectively, the ... can be considered as a free parameter.  | 
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* iterating back and forth between solving for the per-star and global parameters until converged.  | 
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*Equation 1 '''is vulnerable to''' outliers.  | 
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*Fig.1 is a collection of 3 panels. The top, left panel reports the ..relation, as labelled for ...  | 
  *Fig.1 is a collection of 3 panels. The top, left panel reports the ..relation, as labelled for ...  | 
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* Fig. 1 reveals a first glimpse of the result of this paper.  | 
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*For the rest of the paper we will mainly focus our attention on...  | 
  *For the rest of the paper we will mainly focus our attention on...  | 
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*For reasons that will become clear in Section 2.2, we place a flat prior on the reddening of each star.  | 
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* Given the importance of wind, '''additional study is warranted'''.  | 
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* Hα emission '''is arguably one of the'''  most sensitive tracers of the warm ionized gas in galaxies.  | 
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*In order to.., we take advantage of ..  | 
  *In order to.., we take advantage of ..  | 
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* The aim of this exercise is to/is not meant to   | 
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*The error on the median is computed by dividing the 1 sigma uncertainty of the same distribution by the square root of the number of  galaxies in that bin.  | 
  *The error on the median is computed by dividing the 1 sigma uncertainty of the same distribution by the square root of the number of  galaxies in that bin.  | 
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* The reason could be many, including but not limited to....  | 
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* The issue of .. is not yet understood.  | 
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* This procedure is essentially a weighted principal component analysis (PCA),]  | 
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* can be found in *** (不要用seen)  | 
  * can be found in *** (不要用seen)  | 
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* For convenience in the following discussion  | 
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* Finally, we provide short discussions...  | 
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* It has already been pointed out....  | 
  * It has already been pointed out....  | 
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* It  is clear from Figure 1  that ...  | 
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* Overall, IMF observations have not yet converged to a single view  | 
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* Our aim is to figure out...  | 
  * Our aim is to figure out...  | 
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* We will anyway discuss ** where relevant.  | 
  * We will anyway discuss ** where relevant.  | 
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* We will anyhow briefly discuss * in Appendix.  | 
  * We will anyhow briefly discuss * in Appendix.  | 
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* We have so far identified several physical effects which can cause a variation  | 
  * We have so far identified several physical effects which can cause a variation  | 
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* We have determined the values of these parameters by trial and error so as to match the observations.  | 
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* We conclude the section by emphasizing that even if ...  | 
  * We conclude the section by emphasizing that even if ...  | 
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* We investigate the location of X-ray selected sample with respect to main sequence star-forming galaxies using the SFR from where the AGN contamination  has been removed.  | 
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===委婉表达===  | 
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* The comparison is consistent but inconclusive.  | 
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* verifying a tentative detection presented in an earlier study.  | 
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* consider this result on ** to be tentative  | 
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* The ubiquity of Lyman-alpha in this sample is puzzling given that  | 
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* we have initiated a campaign to target U  | 
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* This is to our knowledge the first time that gaseous properties of such faint galaxies at z>=3 are reported.  | 
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* The exact origin of this structure remains unclear but the leading options include a classical accreted halo or tidally stripped outer disk material  | 
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*The parameter space of the simulated data is degenerate and not entirely physical. We therefore refrain from further tuning of the model.  | 
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* We find tentative evidence  | 
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* Although the physical picture in ?? is qualitatively consistent with the observations, we caution that (as with any empirical model) consistency does not automatically imply correctness  | 
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* Although ... it is not entirely surprising in light of ...  | 
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==搭配==  | 
  ==搭配==  | 
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* constant scatter of 0.5 in the distribution of  | 
  * constant scatter of 0.5 in the distribution of  | 
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* in line with what assumed by   | 
  * in line with what assumed by   | 
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* introduce bias into ...  | 
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* it is not trivial 不可忽视的,重要的  it becomes non-trivial to ...  | 
  * it is not trivial 不可忽视的,重要的  it becomes non-trivial to ...  | 
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* making them ideal,complementary tools for studies such as the one undertaken here.   | 
  * making them ideal,complementary tools for studies such as the one undertaken here.   | 
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* provide useful additional physical insights  | 
  * provide useful additional physical insights  | 
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* the sum of A plus B  | 
  * the sum of A plus B  | 
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* A decreases with a decrease of B  | 
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* A is defined as those (不是these)  | 
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* this model yields a good fitting to the observations  | 
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* These panels clearly illustrate...  | 
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* Last but not least,最后同样重要的是  | 
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==专业词汇==  | 
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*starburst 不是 star burst  | 
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*timescale 不是 time scale  | 
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*online 不是on-line  | 
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2022年7月25日 (一) 03:26的最新版本
句式
- A description of the relevant processes and related parameters is given below.
 
- give descriptions of 不用 make descriptions on
 
- Although ... is the result of a complex interplay among a variety of different physical processes, we can still capture some basic trends.
 - Contains a wealth of information that has not yet been exploited
 - Effectively, the ... can be considered as a free parameter.
 - iterating back and forth between solving for the per-star and global parameters until converged.
 - Equation 1 is vulnerable to outliers.
 - Fig.1 is a collection of 3 panels. The top, left panel reports the ..relation, as labelled for ...
 - Fig. 1 reveals a first glimpse of the result of this paper.
 - For the rest of the paper we will mainly focus our attention on...
 - For reasons that will become clear in Section 2.2, we place a flat prior on the reddening of each star.
 - Given the importance of wind, additional study is warranted.
 - Hα emission is arguably one of the most sensitive tracers of the warm ionized gas in galaxies.
 - In order to.., we take advantage of ..
 - The aim of this exercise is to/is not meant to
 - The error on the median is computed by dividing the 1 sigma uncertainty of the same distribution by the square root of the number of galaxies in that bin.
 - The reason could be many, including but not limited to....
 - The issue of .. is not yet understood.
 - There are several general noteworthy features in Fig. 1.
 - This procedure is essentially a weighted principal component analysis (PCA),]
 - can be found in *** (不要用seen)
 - For convenience in the following discussion
 - Finally, we provide short discussions...
 - It has already been pointed out....
 - It is clear from Figure 1 that ...
 - Overall, IMF observations have not yet converged to a single view
 - Our aim is to figure out...
 - We will anyway discuss ** where relevant.
 - We discuss whether there are other possibilities other than ..
 - We will discuss a realization of the * model with the identical prescriptions as the one just described by with no..
 - We will anyhow briefly discuss * in Appendix.
 - We have so far identified several physical effects which can cause a variation
 - We have determined the values of these parameters by trial and error so as to match the observations.
 - We conclude the section by emphasizing that even if ...
 - We investigate the location of X-ray selected sample with respect to main sequence star-forming galaxies using the SFR from where the AGN contamination has been removed.
 
委婉表达
- The comparison is consistent but inconclusive.
 - verifying a tentative detection presented in an earlier study.
 - consider this result on ** to be tentative
 - The ubiquity of Lyman-alpha in this sample is puzzling given that
 - we have initiated a campaign to target U
 - This is to our knowledge the first time that gaseous properties of such faint galaxies at z>=3 are reported.
 - The exact origin of this structure remains unclear but the leading options include a classical accreted halo or tidally stripped outer disk material
 - The parameter space of the simulated data is degenerate and not entirely physical. We therefore refrain from further tuning of the model.
 - We find tentative evidence
 - Although the physical picture in ?? is qualitatively consistent with the observations, we caution that (as with any empirical model) consistency does not automatically imply correctness
 - Although ... it is not entirely surprising in light of ...
 
搭配
- act as a useful supplement in ... studies
 - assume to be, find to be, expect sth to do
 - as detailed below/In the following/ To start off with
 - constant scatter of 0.5 in the distribution of
 - in line with what assumed by
 - introduce bias into ...
 - it is not trivial 不可忽视的,重要的 it becomes non-trivial to ...
 - making them ideal,complementary tools for studies such as the one undertaken here.
 - marked by dotted line
 - may be prone to 倾向于
 - plalying a significant role in shaping...
 - provide useful additional physical insights
 - the sum of A plus B
 - A decreases with a decrease of B
 - A is defined as those (不是these)
 - this model yields a good fitting to the observations
 - These panels clearly illustrate...
 - Last but not least,最后同样重要的是
 
专业词汇
- starburst 不是 star burst
 - timescale 不是 time scale
 - online 不是on-line