JWST - 版本历史

2024年8月29日 (四) 01:57 Shen

2024-08-29T01:57:44Z

←上一版本		2024年8月29日 (四) 01:57的版本
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	==projects==		==projects==
	*[[JADES]]		*[[JADES]]

			==data==
			*DAWN JWST Archive [https://dawn-cph.github.io/dja/about/summary/]

Shen：/* MIRI */

2023-12-23T08:51:37Z

MIRI

←上一版本		2023年12月23日 (六) 08:51的版本
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	*[Ne iii]1.56mu/[Ne ii]12.81mu, which is an indicator of the hardness of the local radiation field		*[Ne iii]1.56mu/[Ne ii]12.81mu, which is an indicator of the hardness of the local radiation field
	*“The SFR can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.		*“The SFR can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.
			* 可以用image-registration的方法来把图对齐，从而解天体测量。https://doi.org/10.3847/2041-8213/acaaae

	==sciences==		==sciences==

2023年12月20日 (三) 14:38 Shen

2023-12-20T14:38:08Z

←上一版本		2023年12月20日 (三) 14:38的版本
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	*“The SFR can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.		*“The SFR can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.

			==sciences==
			* 高红移spiral星系的比例挺高的，至少20% @z~3 [https://arxiv.org/pdf/2312.12389.pdf]
	==projects==		==projects==
	*[[JADES]]		*[[JADES]]

2023年6月8日 (四) 07:34 Shen

2023-06-08T07:34:00Z

←上一版本		2023年6月8日 (四) 07:34的版本
第7行：		第7行：
	*[Ne iii]1.56mu/[Ne ii]12.81mu, which is an indicator of the hardness of the local radiation field		*[Ne iii]1.56mu/[Ne ii]12.81mu, which is an indicator of the hardness of the local radiation field
	*“The SFR can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.		*“The SFR can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.

			==projects==
			*[[JADES]]

Shen：创建页面，内容为“==NIRspec== *NIRSpec is equipped with an integral field unit optimized for the spectroscopic study of complex extended objects. It will provide 900 spectra per expos…”

2022-09-15T14:47:28Z

创建页面，内容为“==NIRspec== *NIRSpec is equipped with an integral field unit optimized for the spectroscopic study of complex extended objects. It will provide 900 spectra per expos…”

新页面

==NIRspec==
*NIRSpec is equipped with an integral field unit optimized for the spectroscopic study of complex extended objects. It will provide 900 spectra per exposure over a field of view of 3 x 3 arcminutes.（0.6-5mu）

==MIRI==
*用CAFE拟合，可以得到9.7mu的尘埃光深
*H2的转动线S(1)-S(7)，可以直接测量H2的含量
*[Ne iii]1.56mu/[Ne ii]12.81mu, which is an indicator of the hardness of the local radiation field
*“The SFR can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.