“常用表达”的版本间差异
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:give descriptions of 不用 make descriptions on |
: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. |
* 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. |
*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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* There are several general noteworthy features in Fig. 1. |
* There are several general noteworthy features in Fig. 1. |
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* This procedure is essentially a weighted principal component analysis (PCA), |
* 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 |
* For convenience in the following discussion |
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* Finally, we provide short discussions... |
* 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 |
* 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 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. |
* 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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* The comparison is consistent but inconclusive. |
* The comparison is consistent but inconclusive. |
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* verifying a tentative detection presented in an earlier study. |
* 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 |
* The ubiquity of Lyman-alpha in this sample is puzzling given that |
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* we have initiated a campaign to target U |
* 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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* A is defined as those (不是these) |
* A is defined as those (不是these) |
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* this model yields a good fitting to the observations |
* 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== |
==专业词汇== |
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