Search Publications

Finding Peas in the Early Universe with JWST
DOI: 10.3847/2041-8213/acaaaf Bibcode: 2023ApJ...942L..14R

Kim, Keunho J.; Malhotra, Sangeeta; Pharo, John +6 more

The Early Release Observations (EROs) of JWST beautifully demonstrate the promise of JWST in characterizing the universe at Cosmic Dawn. We analyze the Near Infrared Spectrograph ERO spectra of three z ~ 8 galaxies to determine their metallicities, gas temperatures, and ionization. These galaxies offer the first opportunity to understand the physi…

2023 The Astrophysical Journal
JWST 75
JADES: Discovery of extremely high equivalent width Lyman-α emission from a faint galaxy within an ionized bubble at z = 7.3
DOI: 10.1051/0004-6361/202346245 Bibcode: 2023A&A...678A..68S

Chevallard, Jacopo; Maseda, Michael V.; Carniani, Stefano +44 more

We report the discovery of a remarkable Lyα emitting galaxy at z = 7.2782, JADES-GS+53.16746−27.7720 (shortened to JADES-GS-z7-LA), with rest-frame equivalent width, EW0(Lyα) = 388.0 ± 88.8 Å and UV magnitude −17.0. The spectroscopic redshift is confirmed via rest-frame optical lines [O II], Hβ and [O III] in its JWST/NIRSpec Micro-Shut…

2023 Astronomy and Astrophysics
JWST 75
Constraints on the Hubble constant from supernova Refsdal's reappearance
DOI: 10.1126/science.abh1322 Bibcode: 2023Sci...380.1322K

Treu, Tommaso; Broadhurst, Tom; Filippenko, Alexei V. +27 more

The gravitationally lensed supernova Refsdal appeared in multiple images produced through gravitational lensing by a massive foreground galaxy cluster. After the supernova appeared in 2014, lens models of the galaxy cluster predicted that an additional image of the supernova would appear in 2015, which was subsequently observed. We use the time de…

2023 Science
eHST 75
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 µm
DOI: 10.3847/2041-8213/acd93e Bibcode: 2023ApJ...951L..20C

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

We present JWST Early Release Science coronagraphic observations of the super-Jupiter exoplanet, HIP 65426b, with the Near-Infrared Camera (NIRCam) from 2 to 5 µm, and with the Mid-Infrared Instrument (MIRI) from 11 to 16 µm. At a separation of ~0.″82 (87 ${}_{-31}^{+108}$ au), HIP 65426b is clearly detected in all seven of our observa…

2023 The Astrophysical Journal
AKARI Gaia JWST 75
A 3D Drizzle Algorithm for JWST and Practical Application to the MIRI Medium Resolution Spectrometer
DOI: 10.3847/1538-3881/acdddc Bibcode: 2023AJ....166...45L

Law, David R.; Vandenbussche, Bart; Patapis, Polychronis +4 more

We describe an algorithm for application of the classic "drizzle" technique to produce 3D spectral cubes using data obtained from the slicer-type integral field unit (IFU) spectrometers on board the James Webb Space Telescope. This algorithm relies upon the computation of overlapping volume elements (composed of two spatial dimensions and one spec…

2023 The Astronomical Journal
JWST 74
Gaia Data Release 3. Specific processing and validation of all sky RR Lyrae and Cepheid stars: The Cepheid sample
DOI: 10.1051/0004-6361/202243990 Bibcode: 2023A&A...674A..17R

Szabados, L.; Audard, M.; Plachy, E. +19 more

Context. Cepheids are pulsating stars that play a crucial role in several astrophysical contexts. Among the different types, the Classical Cepheids are fundamental tools for the calibration of the extragalactic distance ladder. They are also powerful stellar population tracers in the context of Galactic studies. The Gaia Third Data Release (DR3) p…

2023 Astronomy and Astrophysics
Gaia 74
On the ages of bright galaxies 500 Myr after the big bang: insights into star formation activity at z ≳ 15 with JWST
DOI: 10.1093/mnras/stac3535 Bibcode: 2023MNRAS.519..157W

Charlot, Stéphane; Chen, Zuyi; Stark, Daniel P. +3 more

With JWST, new opportunities to study the evolution of galaxies in the early Universe are emerging. Spitzer constraints on rest-optical properties of z ≳ 7 galaxies demonstrated the power of using galaxy stellar masses and star formation histories (SFHs) to indirectly infer the cosmic star formation history. However, only the brightest individual …

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 74
First insights into the ISM at z > 8 with JWST: possible physical implications of a high [O III] λ4363/[O III] λ5007
DOI: 10.1093/mnras/stac2657 Bibcode: 2023MNRAS.518..592K

Carniani, Stefano; Übler, Hannah; D'Eugenio, Francesco +15 more

We present a detailed analysis of the rest-frame optical emission line ratios for three spectroscopically confirmed galaxies at z > 7.5. The galaxies were identified in the James Webb Space Telescope (JWST) Early Release Observations field SMACS J0723.3 - 7327. By quantitatively comparing Balmer and oxygen line ratios of these galaxies with var…

2023 Monthly Notices of the Royal Astronomical Society
JWST 74
Spatially Resolved Properties of Galaxies at 5 < z < 9 in the SMACS 0723 JWST ERO Field
DOI: 10.3847/1538-4357/acc5ea Bibcode: 2023ApJ...948..126G

Fujimoto, Seiji; Heintz, Kasper E.; Suess, Katherine A. +10 more

We present the first spatially resolved measurements of galaxy properties in the JWST ERO SMACS 0723 field. We perform a comprehensive analysis of five 5 < z < 9 galaxies with spectroscopic redshifts from NIRSpec observations. We perform spatially resolved spectral energy distribution fitting with BAGPIPES, using six NIRCam imaging bands spa…

2023 The Astrophysical Journal
JWST 73
High-redshift Galaxy Candidates at z = 9-10 as Revealed by JWST Observations of WHL0137-08
DOI: 10.3847/1538-4357/acecfe Bibcode: 2023ApJ...955...13B

Hutchison, Taylor A.; Larson, Rebecca L.; Mahler, Guillaume +25 more

We report the discovery of four galaxy candidates observed 450-600 Myr after the Big Bang with photometric redshifts between z ~ 8.3 and 10.2 measured using James Webb Space Telescope (JWST) NIRCam imaging of the galaxy cluster WHL0137-08 observed in eight filters spanning 0.8-5.0 µm, plus nine Hubble Space Telescope filters spanning 0.4-1.7…

2023 The Astrophysical Journal
Gaia eHST JWST 73