2025ApJ...983L...4F


Query : 2025ApJ...983L...4F

2025ApJ...983L...4F - Astrophys. J., 983, L4 (2025/April-2)

The Cosmic Evolution Early Release Science Survey (CEERS).

FINKELSTEIN S.L., BAGLEY M.B., ARRABAL HARO P., DICKINSON M., FERGUSON H.C., KARTALTEPE J.S., KOCEVSKI D.D., KOEKEMOER A.M., LOTZ J.M., PAPOVICH C., PEREZ-GONZALEZ P.G., PIRZKAL N., SOMERVILLE R.S., TRUMP J.R., YANG G., YUNG L.Y.A., FONTANA A., GRAZIAN A., GROGIN N.A., KEWLEY L.J., KIRKPATRICK A., LARSON R.L., PENTERICCI L., RAVINDRANATH S., WILKINS S.M., ALMAINI O., AMORIN R.O., BARRO G., BHATAWDEKAR R., BISIGELLO L., BROOKS M., BUAT V., BUITRAGO F., BURGARELLA D., CALABRO A., CASTELLANO M., CHENG Y., CLERI N.J., COLE J.W., COOPER M.C., COOPER O.R., COSTANTIN L., COX I.G., CROTON D., DADDI E., DAVIS K., DEKEL A., ELBAZ D., FERNANDEZ V., FUJIMOTO S., GANDOLFI G., GARDNER J.P., GAWISER E., GIAVALISCO M., GOMEZ-GUIJARRO C., GUO Y., GUPTA A.R., HATHI N.P., HARISH S., HENRY A., HIRSCHMANN M., HU W., HUTCHISON T.A., IYER K.G., JASKOT A.E., JHA S.W., JUNG I., KASSIN S.A., KOKOREV V., KURCZYNSKI P., LEUNG G.C.K., LLERENA M., LONG A.S., LUCAS R.A., LU S., McGRATH E.J., McINTOSH D.H., MERLIN E., MOBASHER B., MORALES A.M., NAPOLITANO L., PACUCCI F., PANDYA V., RAFELSKI M., RODIGHIERO G., ROSE C., SANTINI P., SEILLE L.-M., SIMONS R.C., SHEN L., STRAUGHN A.N., TACCHELLA S., TAYLOR A.J., VANDERHOOF B.N., VEGA-FERRERO J., WEINER B.J., WILLMER C.N.A., ZHU P., BELL E.F., WUYTS S., HOLWERDA B.W., WANG X., WANG W., ZAVALA J.A. (The CEERS Collaboration)

Abstract (from CDS):

We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hr Director's Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates efficient extragalactic surveys using coordinated, overlapping parallel observations with the JWST instrument suite, including NIRCam and MIRI imaging, NIRSpec low- (R ∼ 100) and medium- (R ∼ 1000) resolution spectroscopy, and NIRCam slitless grism (R ∼ 1500) spectroscopy. CEERS targets the Hubble Space Telescope-observed region of the Extended Groth Strip field, supported by a rich set of multiwavelength data. CEERS facilitated immediate community science in both of the extragalactic core JWST science drivers “First Light” and “Galaxy Assembly,” including: (1) the discovery and characterization of large samples of galaxies at z ≳ 10 from ∼90 arcmin2 of NIRCam imaging, constraining their abundance and physical nature; (2) deep spectra of >1000 galaxies, including dozens of galaxies at 6 < z < 10, enabling redshift measurements and constraints on the physical conditions of star formation and black hole growth via line diagnostics; (3) quantifying the first bulge, bar, and disk structures at z > 3; and (4) characterizing galaxy mid-IR emission with MIRI to study dust-obscured star formation and supermassive black hole growth at z ∼ 1-3. As a legacy product for the community, the CEERS team has provided several data releases, accompanied by detailed notes on the data reduction procedures and notebooks to aid in reproducibility. In addition to an overview of the survey and the quality of the data, we provide science highlights from the first two years with CEERS data.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Galaxy evolution - Surveys - Galaxy formation - Supermassive black holes

Simbad objects: 9

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Number of rows : 9
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 NAME GOODS Southern Field reg 03 32 28.0 -27 48 30           ~ 1623 1
2 NAME Hubble Ultra Deep Field reg 03 32 39.0 -27 47 29           ~ 1900 0
3 NGC 1705 Sy2 04 54 13.4661493464 -53 21 39.471592428 12.32 12.96 12.56 12.58 12.9 ~ 692 1
4 NAME COSMOS Field reg 10 00 28.60 +02 12 21.0           ~ 3639 0
5 NAME Hubble Deep Field reg 12 36 49.5 +62 12 58           ~ 1967 1
6 NAME GOODS-N Field reg 12 36 55.0 +62 14 15           ~ 1364 1
7 NAME Extended Groth Strip reg 14 19 +52.8           ~ 1023 0
8 CANDELS EGS F160W J141924.1+525159.1 AGN 14 19 24.13696 +52 51 59.2108           ~ 8 0
9 CEERS J141946.36+525632.8 G 14 19 46.350 +52 56 32.82           ~ 38 0

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