Hubble Frontier Field - 版本历史

Shen：/* MUSE observation */

2021-12-12T14:56:47Z

MUSE observation

←上一版本		2021年12月12日 (日) 14:56的版本
第7行：		第7行：
	* M0416: the deep pointing as the MUSE Deep Lensed Field (MDLF) centred in the north-east part of the cluster (17.1h integration time, 0100.A-0763(A), PI: Vanzella) and the observation in the south-west (11-hour integration, 094.A0525(A), PI: Bauer).		* M0416: the deep pointing as the MUSE Deep Lensed Field (MDLF) centred in the north-east part of the cluster (17.1h integration time, 0100.A-0763(A), PI: Vanzella) and the observation in the south-west (11-hour integration, 094.A0525(A), PI: Bauer).
	* A2744 was observed with MUSE between September 2014 and October 2015 as part of the GTO Program (094.A-0115, PI:Richard). The MUSE pointings cover a 2*2 arcmin2 mosaic with the purpose of covering the entire multiple image area.		* A2744 was observed with MUSE between September 2014 and October 2015 as part of the GTO Program (094.A-0115, PI:Richard). The MUSE pointings cover a 2*2 arcmin2 mosaic with the purpose of covering the entire multiple image area.
	* A370 was observed with MUSE using a large mosaic covering � 4 arcmin2.		* A370 was observed with MUSE using a large mosaic covering ~4 arcmin2.

2021年12月12日 (日) 14:56 Shen

2021-12-12T14:56:36Z

←上一版本		2021年12月12日 (日) 14:56的版本
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	:*Taking into account the gravitational lensing effects, the effective depths of the HFF observations are 30~33 magnitudes over very small volumes.		:*Taking into account the gravitational lensing effects, the effective depths of the HFF observations are 30~33 magnitudes over very small volumes.
	:*For all the HFF targets, HST obtained images with the ACS and WFC3, in a total of seven broad-band �filters (F435W, F606W, F814W, F105W, F125W, F140W, F160W).		:*For all the HFF targets, HST obtained images with the ACS and WFC3, in a total of seven broad-band �filters (F435W, F606W, F814W, F105W, F125W, F140W, F160W).

			==[[MUSE]] observation==
			* M0416: the deep pointing as the MUSE Deep Lensed Field (MDLF) centred in the north-east part of the cluster (17.1h integration time, 0100.A-0763(A), PI: Vanzella) and the observation in the south-west (11-hour integration, 094.A0525(A), PI: Bauer).
			* A2744 was observed with MUSE between September 2014 and October 2015 as part of the GTO Program (094.A-0115, PI:Richard). The MUSE pointings cover a 2*2 arcmin2 mosaic with the purpose of covering the entire multiple image area.
			* A370 was observed with MUSE using a large mosaic covering � 4 arcmin2.

2021年12月12日 (日) 14:47 Shen

2021-12-12T14:47:19Z

←上一版本		2021年12月12日 (日) 14:47的版本
第1行：		第1行：
	*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank field images (6 arcmins from the cluster core).		*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank field images (6 arcmins from the cluster core).
	*HST employed 840 orbits (140 orbits for each galaxy cluster) to observe the HFF galaxy clusters, achieving a superb depth of � 28.7~29 magnitudes (5 sigma).		:*HST employed 840 orbits (140 orbits for each galaxy cluster) to observe the HFF galaxy clusters, achieving a superb depth of � 28.7~29 magnitudes (5 sigma).
	:*Taking into account the gravitational lensing effects, the effective depths of the HFF observations are 30~33 magnitudes over very small volumes.		:*Taking into account the gravitational lensing effects, the effective depths of the HFF observations are 30~33 magnitudes over very small volumes.
	:*For all the HFF targets, HST obtained images with the ACS and WFC3, in a total of seven broad-band �filters (F435W, F606W, F814W, F105W, F125W, F140W, F160W).		:*For all the HFF targets, HST obtained images with the ACS and WFC3, in a total of seven broad-band �filters (F435W, F606W, F814W, F105W, F125W, F140W, F160W).

2021年12月12日 (日) 14:47 Shen

2021-12-12T14:47:07Z

←上一版本		2021年12月12日 (日) 14:47的版本
第1行：		第1行：
	*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank field images (6 arcmins from the cluster core).		*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank field images (6 arcmins from the cluster core).
	:HST employed 840 orbits (140 orbits for each galaxy cluster) to observe the HFF galaxy clusters, achieving a superb depth of � 28.7~29 magnitudes (5 sigma).		*HST employed 840 orbits (140 orbits for each galaxy cluster) to observe the HFF galaxy clusters, achieving a superb depth of � 28.7~29 magnitudes (5 sigma).
	:Taking into account the gravitational lensing effects, the effective depths of the HFF observations are 30~33 magnitudes over very small volumes.		:*Taking into account the gravitational lensing effects, the effective depths of the HFF observations are 30~33 magnitudes over very small volumes.
	:For all the HFF targets, HST obtained images with the ACS and WFC3, in a total of seven broad-band �filters (F435W, F606W, F814W, F105W, F125W, F140W, F160W).		:*For all the HFF targets, HST obtained images with the ACS and WFC3, in a total of seven broad-band �filters (F435W, F606W, F814W, F105W, F125W, F140W, F160W).

2021年12月12日 (日) 14:45 Shen

2021-12-12T14:45:08Z

←上一版本		2021年12月12日 (日) 14:45的版本
第1行：		第1行：
	*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank field images (6 arcmins from the cluster core).		*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank field images (6 arcmins from the cluster core).
			:HST employed 840 orbits (140 orbits for each galaxy cluster) to observe the HFF galaxy clusters, achieving a superb depth of � 28.7~29 magnitudes (5 sigma).
			:Taking into account the gravitational lensing effects, the effective depths of the HFF observations are 30~33 magnitudes over very small volumes.
			:For all the HFF targets, HST obtained images with the ACS and WFC3, in a total of seven broad-band �filters (F435W, F606W, F814W, F105W, F125W, F140W, F160W).

2021年12月12日 (日) 14:37 Shen

2021-12-12T14:37:26Z

←上一版本		2021年12月12日 (日) 14:37的版本
第1行：		第1行：
	*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank		*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank field images (6 arcmins from the cluster core).
	�eld images (6 arcmins from the cluster core).

Shen：创建页面，内容为“*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parall…”

2021-12-12T14:37:13Z

创建页面，内容为“*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parall…”

新页面

*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parallel blank
�eld images (6 arcmins from the cluster core).

Hubble Frontier Field - 版本历史

Shen：​/* MUSE observation */

2021年12月12日 (日) 14:56 Shen

2021年12月12日 (日) 14:47 Shen

2021年12月12日 (日) 14:47 Shen

2021年12月12日 (日) 14:45 Shen

2021年12月12日 (日) 14:37 Shen

Shen：​创建页面，内容为“*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parall…”

Shen：/* MUSE observation */

Shen：创建页面，内容为“*The HFF program (Koekemoer et al. 2016; Lotz et al. 2017) consists of multi-cycle HST observations to target six galaxy lensing clusters in parallel with six parall…”