Results 1 to 10 of about 218 (186)

Physical Characterization of Early Galaxies in the Webb’s First Deep Field SMACS J0723.3-7327

open access: yesThe Astrophysical Journal Letters, 2023
This paper highlights initial photometric analyses of JWST NIRCam imaging data in the sightline of SMACS0723, aiming to identify galaxies at redshift z > 7.
T. Morishita, M. Stiavelli
doaj   +1 more source

Early Results from GLASS-JWST. XIX. A High Density of Bright Galaxies at z ≈ 10 in the A2744 Region

open access: yesThe Astrophysical Journal Letters, 2023
We report the detection of a high density of redshift z ≈ 10 galaxies behind the foreground cluster A2744, selected from imaging data obtained recently with NIRCam on board JWST by three programs—GLASS-JWST, UNCOVER, and DDT#2756.
Marco Castellano   +40 more
doaj   +1 more source

A Mixture of LBG Overdensities in the Fields of Three 6 < z < 7 Quasars: Implications for the Robustness of Photometric Selection

open access: yesThe Astrophysical Journal, 2023
The most luminous quasars at z > 6 are suspected to be both highly clustered and to reside in the most massive dark matter halos in the early universe, making them prime targets to search for galaxy overdensities and/or protoclusters. We search for Lyman-
Jaclyn B. Champagne   +7 more
doaj   +1 more source

Broad Emission Lines in Optical Spectra of Hot, Dust-obscured Galaxies Can Contribute Significantly to JWST/NIRCam Photometry

open access: yesThe Astrophysical Journal Letters, 2023
Selecting the first galaxies at z > 7 − 10 from JWST surveys is complicated by z < 6 contaminants with degenerate photometry. For example, strong optical nebular emission lines at z < 6 may mimic JWST/NIRCam photometry of z > 7–10 Lyman-break galaxies ...
Jed McKinney   +15 more
doaj   +1 more source

Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations

open access: yesThe Astrophysical Journal Letters, 2023
Lyman-break galaxy (LBG) candidates at z ≳ 10 are rapidly being identified in James Webb Space Telescope (JWST)/NIRCam observations. Due to the (redshifted) break produced by neutral hydrogen absorption of rest-frame UV photons, these sources are ...
Jorge A. Zavala   +124 more
doaj   +1 more source

Early Results From GLASS-JWST. XII. The Morphology of Galaxies at the Epoch of Reionization

open access: yesThe Astrophysical Journal Letters, 2023
Star-forming galaxies can exhibit strong morphological differences between the rest-frame far-UV and optical, reflecting inhomogeneities in star formation and dust attenuation.
T. Treu   +25 more
doaj   +1 more source

Spurious Correlations between Galaxies and Multiepoch Image Stacks in the DESI Legacy Surveys

open access: yesThe Astrophysical Journal Supplement Series, 2023
A nonnegligible source of systematic bias in cosmological analyses of galaxy surveys is the on-sky modulation that is caused by foregrounds and variable image characteristics, such as observing conditions.
Edgar Eggert, Boris Leistedt
doaj   +1 more source

JWST's PEARLS: Bright 1.5–2.0 μm Dropouts in the Spitzer/IRAC Dark Field

open access: yesThe Astrophysical Journal Letters, 2022
Using the first epoch of four-band NIRCam observations obtained by the James Webb Space Telescope (JWST) Prime Extragalactic Areas for Reionization and Lensing Science Program in the Spitzer IRAC Dark Field, we search for F150W and F200W dropouts.
Haojing Yan   +37 more
doaj   +1 more source

Deep Spitzer/IRAC Data for z ∼ 10 Galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ∼500 Myr of Cosmic Time

open access: yesThe Astrophysical Journal, 2023
We present the deepest constraints yet on the median rest-UV+optical spectral energy distribution (SED) of z ∼ 10 galaxies prior to James Webb Space Telescope science operations.
Mauro Stefanon   +5 more
doaj   +1 more source

Nitrogen abundances in star-forming galaxies 2.2 Gyr after the Big Bang are not elevated

open access: yesAstronomy & Astrophysics
Using deep, medium-resolution, JWST rest-optical spectra of a sample of typical star-forming galaxies (Lyman-break galaxies and Lyman-α emitters) from the LyC22 survey at z ∼ 3, we determined the nebular abundances of N, O, and Ne relative to H for a ...
Schaerer D.   +24 more
doaj   +1 more source

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