Search Publications

Overview of the DESI Milky Way Survey
DOI: 10.3847/1538-4357/acb3c0 Bibcode: 2023ApJ...947...37C

Miquel, Ramon; Myers, Adam D.; Bailey, Stephen +62 more

We describe the Milky Way Survey (MWS) that will be undertaken with the Dark Energy Spectroscopic Instrument (DESI) on the Mayall 4 m telescope at the Kitt Peak National Observatory. Over the next 5 yr DESI MWS will observe approximately seven million stars at Galactic latitudes |b| > 20°, with an inclusive target selection scheme focused on th…

2023 The Astrophysical Journal
Gaia 122
Life beyond 30: Probing the -20 < M UV < -17 Luminosity Function at 8 < z < 13 with the NIRCam Parallel Field of the MIRI Deep Survey
DOI: 10.3847/2041-8213/acd9d0 Bibcode: 2023ApJ...951L...1P

Henning, Thomas; Pérez-González, Pablo G.; Costantin, Luca +41 more

We present the ultraviolet luminosity function and an estimate of the cosmic star formation rate density at 8 < z < 13 derived from deep NIRCam observations taken in parallel with the MIRI Deep Survey of the Hubble Ultra Deep Field (HUDF), NIRCam covering the parallel field 2. Our deep (40 hr) NIRCam observations reach an F277W magnitude of …

2023 The Astrophysical Journal
Gaia eHST JWST 122
The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations
DOI: 10.3847/1538-4357/acba8a Bibcode: 2023ApJ...945...35T

Papovich, Casey; Cole, Justin W.; Finkelstein, Steven L. +63 more

We present rest-frame optical emission-line flux ratio measurements for five z > 5 galaxies observed by the James Webb Space Telescope Near-Infared Spectrograph (NIRSpec) in the SMACS 0723 Early Release Observations. We add several quality-control and post-processing steps to the NIRSpec pipeline reduction products in order to ensure reliable r…

2023 The Astrophysical Journal
JWST 118
CEERS Key Paper. IV. A Triality in the Nature of HST-dark Galaxies
DOI: 10.3847/2041-8213/acb3a5 Bibcode: 2023ApJ...946L..16P

Papovich, Casey; Yang, Guang; Finkelstein, Steven L. +52 more

The new capabilities that JWST offers in the near- and mid-infrared (IR) are used to investigate in unprecedented detail the nature of optical/near-IR-faint, mid-IR-bright sources, with HST-dark galaxies among them. We gather JWST data from the CEERS survey in the Extended Groth Strip, jointly with HST data, and analyze spatially resolved optical-…

2023 The Astrophysical Journal
Gaia Herschel eHST JWST 117
EIGER. I. A Large Sample of [O III]-emitting Galaxies at 5.3 < z < 6.9 and Direct Evidence for Local Reionization by Galaxies
DOI: 10.3847/1538-4357/acc588 Bibcode: 2023ApJ...950...66K

Simcoe, Robert A.; Kashino, Daichi; Eilers, Anna-Christina +4 more

We present a first sample of 117 [O III] λλ4960, 5008-selected star-forming galaxies at 5.33 < z < 6.93 detected in JWST/NIRCam 3.5 µm slitless spectroscopy of a $6\buildrel{\,\prime}\over{.} 5\,\times \,3\buildrel{\,\prime}\over{.} 4$ field centered on the hyperluminous quasar SDSS J0100+2802, obtained as part of the Emission-line gal…

2023 The Astrophysical Journal
Gaia JWST 116
The JWST Early-release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 µm Spectrum of the Planetary-mass Companion VHS 1256-1257 b
DOI: 10.3847/2041-8213/acb04a Bibcode: 2023ApJ...946L...6M

Henning, Thomas; Fortney, Jonathan J.; Carter, Aarynn L. +108 more

We present the highest fidelity spectrum to date of a planetary-mass object. VHS 1256 b is a <20 M Jup widely separated (~8″, a = 150 au), young, planetary-mass companion that shares photometric colors and spectroscopic features with the directly imaged exoplanets HR 8799c, d, and e. As an L-to-T transition object, VHS 1256 b exists …

2023 The Astrophysical Journal
Gaia JWST 111
High Tide or Riptide on the Cosmic Shoreline? A Water-rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ 486b from JWST Observations
DOI: 10.3847/2041-8213/accb9c Bibcode: 2023ApJ...948L..11M

Sing, David K.; Lustig-Yaeger, Jacob; Fu, Guangwei +21 more

Planets orbiting M-dwarf stars are prime targets in the search for rocky exoplanet atmospheres. The small size of M dwarfs renders their planets exceptional targets for transmission spectroscopy, facilitating atmospheric characterization. However, it remains unknown whether their host stars' highly variable extreme-UV radiation environments allow …

2023 The Astrophysical Journal
JWST 110
Early Results from GLASS-JWST. XIV. A Spectroscopically Confirmed Protocluster 650 Million Years after the Big Bang
DOI: 10.3847/2041-8213/acb99e Bibcode: 2023ApJ...947L..24M

Santini, Paola; Calabrò, Antonello; Castellano, Marco +39 more

We present the spectroscopic confirmation of a protocluster at z = 7.88 behind the galaxy cluster Abell 2744 (hereafter A2744-z7p9OD). Using JWST NIRSpec, we find seven galaxies within a projected radius of 60 kpc. Although the galaxies reside in an overdensity around ≳20× greater than a random volume, they do not show strong Lyα emission. We plac…

2023 The Astrophysical Journal
JWST 106
Excitation and Ionization Properties of Star-forming Galaxies at z = 2.0-9.3 with JWST/NIRSpec
DOI: 10.3847/1538-4357/acedad Bibcode: 2023ApJ...955...54S

Shapley, Alice E.; Reddy, Naveen A.; Sanders, Ryan L. +2 more

We utilize medium-resolution JWST/NIRSpec observations of 164 galaxies at z = 2.0-9.3 from the Cosmic Evolution Early Release Science (CEERS) survey to investigate the evolution of the excitation and ionization properties of galaxies at high redshifts. Our results represent the first statistical constraints on the evolution of the [O III]/Hβ versu…

2023 The Astrophysical Journal
eHST JWST 105
Early Results from GLASS-JWST. XIX. A High Density of Bright Galaxies at z ≈ 10 in the A2744 Region
DOI: 10.3847/2041-8213/accea5 Bibcode: 2023ApJ...948L..14C

Santini, Paola; Calabrò, Antonello; Castellano, Marco +38 more

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. To ensure robust estimates of the lensing magnification µ, we use an improved version of our model that exploits…

2023 The Astrophysical Journal
JWST 101