Search Publications

The Gas and Stellar Content of a Metal-poor Galaxy at z = 8.496 as Revealed by JWST and ALMA
DOI: 10.3847/2041-8213/acb2cf Bibcode: 2023ApJ...944L..30H

Schaerer, D.; Magdis, G. E.; Bauer, F. E. +27 more

We present a joint analysis of the galaxy S04590 at z = 8.496 based on NIRSpec, NIRCam, and NIRISS observations obtained as part of the Early Release Observations program of the James Webb Space Telescope (JWST) and the far-infrared [C II] 158 µm emission line detected by dedicated Atacama Large Millimeter/submillimeter Array (ALMA) observat…

2023 The Astrophysical Journal
JWST 44
Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged inside the Debris Disk of the Young Star AF Lep
DOI: 10.3847/2041-8213/acd6f6 Bibcode: 2023ApJ...950L..19F

Jensen-Clem, Rebecca; Crepp, Justin R.; Zhou, Yifan +13 more

We present the direct-imaging discovery of a giant planet orbiting the young star AF Lep, a 1.2 M member of the 24 ± 3 Myr β Pic moving group. AF Lep was observed as part of our ongoing high-contrast imaging program targeting stars with astrometric accelerations between Hipparcos and Gaia that indicate the presence of substellar compa…

2023 The Astrophysical Journal
Gaia Hipparcos 44
Dusty-wind-clear JWST Super-early Galaxies
DOI: 10.3847/2041-8213/acb5f2 Bibcode: 2023ApJ...943L..27F

Ferrara, Andrea; Fiore, Fabrizio; Travascio, Andrea +2 more

The JWST discovery of a number of super-early (redshift z > 10) blue galaxies requires these systems to be essentially dust free in spite of their large stellar masses. A possible explanation is that dust is evacuated by radiatively driven outflows. We test this hypothesis by deriving the Eddington ratio λ E = L bol/L

2023 The Astrophysical Journal
eHST JWST 43
Early Results from GLASS-JWST. XXI. Rapid Asembly of a Galaxy at z = 6.23 Revealed by Its C/O Abundance
DOI: 10.3847/2041-8213/acd938 Bibcode: 2023ApJ...951L..17J

Santini, Paola; Pentericci, Laura; Treu, Tommaso +22 more

The abundance of carbon relative to oxygen (C/O) is a promising probe of star formation history in the early universe, as the ratio changes with time due to production of these elements by different nucleosynthesis pathways. We present a measurement of $\mathrm{log}({\rm{C}}/{\rm{O}})=-1.01\pm 0.12$ (stat) ±0.15 (sys) in a z = 6.23 galaxy observed…

2023 The Astrophysical Journal
eHST JWST 42
From Images to Dark Matter: End-to-end Inference of Substructure from Hundreds of Strong Gravitational Lenses
DOI: 10.3847/1538-4357/aca525 Bibcode: 2023ApJ...942...75W

Marshall, Philip J.; Birrer, Simon; Darragh-Ford, Elise +4 more

Constraining the distribution of small-scale structure in our universe allows us to probe alternatives to the cold dark matter paradigm. Strong gravitational lensing offers a unique window into small dark matter halos (<1010 M ) because these halos impart a gravitational lensing signal even if they do not host luminous ga…

2023 The Astrophysical Journal
eHST 42
Optimized Photometric Redshifts for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS)
DOI: 10.3847/1538-4357/ac9f12 Bibcode: 2023ApJ...942...36K

Finkelstein, Steven L.; Pérez-González, Pablo G.; Santini, Paola +27 more

We present the first comprehensive release of photometric redshifts (photo- z's) from the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS) team. We use statistics based upon the Quantile-Quantile (Q-Q) plot to identify biases and signatures of underestimated or overestimated errors in photo- z probability density functions …

2023 The Astrophysical Journal
eHST 41
Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus
DOI: 10.3847/1538-4357/aca1c3 Bibcode: 2023ApJ...942..111C

Zenteno, A.; James, D. J.; Li, T. S. +31 more

We report the discovery of Pegasus IV, an ultra-faint dwarf galaxy found in archival data from the Dark Energy Camera processed by the DECam Local Volume Exploration Survey. Pegasus IV is a compact, ultra-faint stellar system ( ${r}_{1/2}={41}_{-6}^{+8}$ pc; M V = -4.25 ± 0.2 mag) located at a heliocentric distance of ${90}_{-6}^{+4}\…

2023 The Astrophysical Journal
Gaia 41
The Fundamental Signature of Star Formation Quenching from AGN Feedback: A Critical Dependence of Quiescence on Supermassive Black Hole Mass, Not Accretion Rate
DOI: 10.3847/1538-4357/acac7c Bibcode: 2023ApJ...944..108B

Maiolino, Roberto; Bluck, Asa F. L.; Piotrowska, Joanna M.

We identify the intrinsic dependence of star formation quenching on a variety of galactic and environmental parameters, utilizing a machine-learning approach with Random Forest classification. We have previously demonstrated the power of this technique to isolate causality, not mere correlation, in complex astronomical data. First, we analyze thre…

2023 The Astrophysical Journal
eHST 41
Confirmation of Subsolar Metallicity for WASP-77Ab from JWST Thermal Emission Spectroscopy
DOI: 10.3847/2041-8213/ace828 Bibcode: 2023ApJ...953L..24A

Bean, Jacob L.; Zhang, Michael; Line, Michael +4 more

We present the dayside thermal emission spectrum of WASP-77Ab from 2.8 to 5.2 µm as observed with the NIRSpec instrument on the James Webb Space Telescope (JWST). WASP-77Ab was previously found to have a subsolar metallicity and a solar carbon-to-oxygen (C/O) ratio from H2O and CO absorption lines detected using high-resolution sp…

2023 The Astrophysical Journal
eHST JWST 40
Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE
DOI: 10.3847/1538-4357/acc582 Bibcode: 2023ApJ...949...44S

Lewis, Geraint F.; Erkal, Denis; Bland-Hawthorn, Joss +20 more

We present the first detailed comparison of populations of dwarf galaxy stellar streams in cosmological simulations and the Milky Way. In particular, we compare streams identified around 13 Milky Way analogs in the FIRE-2 simulations to streams observed by the Southern Stellar Stream Spectroscopic Survey (S 5). For an accurate compariso…

2023 The Astrophysical Journal
Gaia 40