2022ApJ...935..110T

Query : 2022ApJ...935..110T

2022ApJ...935..110T - Astrophys. J., 935, 110 (2022/August-3)

The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans.

TREU T., ROBERTS-BORSANI G., BRADAC M., BRAMMER G., FONTANA A., HENRY A., MASON C., MORISHITA T., PENTERICCI L., WANG X., ACEBRON A., BAGLEY M., BERGAMINI P., BELFIORI D., BONCHI A., BOYETT K., BOUTSIA K., CALABRO A., CAMINHA G.B., CASTELLANO M., DRESSLER A., GLAZEBROOK K., GRILLO C., JACOBS C., JONES T., KELLY P.L., LEETHOCHAWALIT N., MALKAN M.A., MARCHESINI D., MASCIA S., MERCURIO A., MERLIN E., NANAYAKKARA T., NONINO M., PARIS D., POGGIANTI B., ROSATI P., SANTINI P., SCARLATA C., SHIPLEY H.V., STRAIT V., TRENTI M., TUBTHONG C., VANZELLA E., VULCANI B. and YANG L.

Abstract (from CDS):

The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program will obtain and make publicly available the deepest extragalactic data of the ERS campaign. It is primarily designed to address two key science questions, namely, “what sources ionized the universe and when?” and “how do baryons cycle through galaxies?”, while also enabling a broad variety of first look scientific investigations. In primary mode, it will obtain NIRISS and NIRSpec spectroscopy of galaxies lensed by the foreground Hubble Frontier Field cluster, Abell 2744. In parallel, it will use NIRCam to observe two fields that are offset from the cluster center, where lensing magnification is negligible, and which can thus be effectively considered blank fields. In order to prepare the community for access to this unprecedented data, we describe the scientific rationale, the survey design (including target selection and observational setups), and present pre-commissioning estimates of the expected sensitivity. In addition, we describe the planned public releases of high-level data products, for use by the wider astronomical community.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Galaxy formation - Galaxy evolution - Reionization

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 ACO 2744 ClG 00 14 20.03 -30 23 17.8           ~ 1077 0

Query : 2022ApJ...935..110T

Basic data :
ACO 2744 -- Cluster of Galaxies
Other object types: otypes_help 		ClG (2004A&A,ACO,...), gLe (2001ApJ), C?G (2014A&A,XCLASS), X (2020ApJ,RBS,...), G (AM)
ICRS coord. (ep=J2000) : 		00 14 20.03 -30 23 17.8 [ ] E 2002MNRAS.329...87D
FK4 coord. (ep=B1950 eq=1950) : 		00 11 48.51 -30 39 58.6 [ ]
Gal coord. (ep=J2000) : 		008.89623 -81.24283 [ ]
Radial velocity / Redshift / cz : 		V(km/s) 78187 [~] / z(spectroscopic) 0.306 [~] / cz 91736 [~]
   (Opt) D 2019ApJS..240...39G
Angular size (arcmin): 		7.0 7.0 ~ (Rad) D 2015ApJ...813...77Y
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
: 2691 		: 650 Display criteria :

Identifiers (18) :
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ACO 2744 MCS J0014.3-3022 PSZRX G008.92-81.24 SPT-CL J0014-3022
ACCG 118 MCXC J0014.3-3023 RBS 34 XCLASS 20073
ACT-CL J0014.3-3022 PLCKESZ G008.93-81.23 RXC J0014.3-3022 [DBG99] 5
AM 0011-303 PSZ1 G009.02-81.22 RXC J0014.3-3023
BAX 003.5813-30.3887 PSZ2 G008.94-81.22 1RXS J001419.1-302216

References (1077 between 1850 and 2026) (Total 1077)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 7   

   

Observing logs
Herschel : 3    ISO : 2    XMM : 1   

   

External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : ACO 2744

Link by name to the catalogue in VizieR :

ACO 2744 RXC J0014.3-3022 RXC J0014.3-3023 1RXS J001419.1-302216

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