Search Publications

LISA Galactic Binaries with Astrometry from Gaia DR3
DOI: 10.3847/1538-4357/ad2068 Bibcode: 2024ApJ...963..100K

Ramsay, Gavin; Kupfer, Thomas; Pala, Anna F. +11 more

Galactic compact binaries with orbital periods shorter than a few hours emit detectable gravitational waves (GWs) at low frequencies. Their GW signals can be detected with the future Laser Interferometer Space Antenna (LISA). Crucially, they may be useful in the early months of the mission operation in helping to validate LISA's performance in com…

2024 The Astrophysical Journal
Gaia 52
The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S
DOI: 10.3847/1538-4357/ad0da7 Bibcode: 2024ApJ...962..124H

Maiolino, Roberto; Willott, Chris; Johnson, Benjamin D. +28 more

We report the discovery of an extreme galaxy overdensity at z = 5.4 in the GOODS-S field using James Webb Space Telescope (JWST)/NIRCam imaging from JADES and JEMS alongside JWST/NIRCam wide-field slitless spectroscopy from FRESCO. We identified potential members of the overdensity using Hubble Space Telescope+JWST photometry spanning λ = 0.4–5.0 …

2024 The Astrophysical Journal
Gaia eHST JWST 51
The JWST Discovery of the Triply Imaged Type Ia "Supernova H0pe" and Observations of the Galaxy Cluster PLCK G165.7+67.0
DOI: 10.3847/1538-4357/ad1034 Bibcode: 2024ApJ...961..171F

Grogin, Norman A.; Koekemoer, Anton M.; Pirzkal, Nor +38 more

A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hub…

2024 The Astrophysical Journal
Gaia eHST JWST 51
Undermassive Host Galaxies of Five z ∼ 6 Luminous Quasars Detected with JWST
DOI: 10.3847/1538-4357/ad2a57 Bibcode: 2024ApJ...964...90S

Lyu, Jianwei; Rieke, George H.; Alberts, Stacey +2 more

We measure host galaxy stellar masses for a sample of five luminous quasars at z ∼ 5–7. Using JWST/NIRCam medium-band images of nearby point-spread function reference stars, we carefully subtract the contribution from the quasar light to place upper and lower limits on the flux of each host galaxy. We find that the members of our sample of quasar …

2024 The Astrophysical Journal
JWST 50
The Small Sizes and High Implied Densities of "Little Red Dots" with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus
DOI: 10.3847/2041-8213/ad90b8 Bibcode: 2024ApJ...977L..13B

Maseda, Michael V.; Franx, Marijn; Labbé, Ivo +10 more

Early JWST studies found an apparent population of massive, compact galaxies at redshifts z ≳ 7. Recently three of these galaxies were shown to have prominent Balmer breaks, demonstrating that their light at λrest ∼ 3500 Å is dominated by a stellar population that is relatively old (∼200 Myr). All three also have broad Hβ emission with …

2024 The Astrophysical Journal
JWST 50
A More Precise Measurement of the Radius of PSR J0740+6620 Using Updated NICER Data
DOI: 10.3847/1538-4357/ad5f1e Bibcode: 2024ApJ...974..295D

Bogdanov, Slavko; Wolff, Michael T.; Arzoumanian, Zaven +9 more

PSR J0740+6620 is the neutron star with the highest precisely determined mass, inferred from radio observations to be 2.08 ± 0.07 M . Measurements of its radius therefore hold promise to constrain the properties of the cold, catalyzed, high-density matter in neutron star cores. Previously, Miller et al. and Riley et al. reported measur…

2024 The Astrophysical Journal
XMM-Newton 50
Evolution of the Size–Mass Relation of Star-forming Galaxies Since z = 5.5 Revealed by CEERS
DOI: 10.3847/1538-4357/ad20ed Bibcode: 2024ApJ...962..176W

Papovich, Casey; Finkelstein, Steven L.; Arrabal Haro, Pablo +19 more

We combine deep imaging data from the CEERS early release JWST survey and Hubble Space Telescope imaging from CANDELS to examine the size–mass relation of star-forming galaxies and the morphology–quenching relation at stellar masses M ≥ 109.5 M over the redshift range 0.5 < z < 5.5. In this study with a s…

2024 The Astrophysical Journal
Gaia eHST JWST 50
JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H 0
DOI: 10.3847/1538-4357/ad8c21 Bibcode: 2024ApJ...977..120R

Casertano, Stefano; Filippenko, Alexei V.; Li, Siyang +16 more

We cross-check the Hubble Space Telescope (HST) Cepheid/Type Ia supernova (SN Ia) distance ladder, which yields the most precise local H 0, against early James Webb Space Telescope (JWST) subsamples (∼1/4 of the HST sample) from SH0ES and CCHP, calibrated only with NGC 4258. We find HST Cepheid distances agree well (∼1σ) with all combin…

2024 The Astrophysical Journal
eHST JWST 49
Quantifying the Effects of Known Unknowns on Inferred High-redshift Galaxy Properties: Burstiness, IMF, and Nebular Physics
DOI: 10.3847/1538-4357/ad187c Bibcode: 2024ApJ...963...74W

Labbé, Ivo; Bezanson, Rachel; Price, Sedona H. +15 more

The era of the James Webb Space Telescope ushers stellar population models into uncharted territories, particularly at the high-redshift frontier. In a companion paper, we apply the Prospector Bayesian framework to jointly infer galaxy redshifts and stellar population properties from broadband photometry as part of the UNCOVER survey. Here we pres…

2024 The Astrophysical Journal
eHST JWST 48
A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function
DOI: 10.3847/1538-4357/ad35bc Bibcode: 2024ApJ...966...74W

Willott, Chris J.; Martis, Nicholas S.; Rihtaršič, Gregor +15 more

We present a new sample of 158 galaxies at redshift z > 7.5 selected from deep James Webb Space Telescope (JWST) NIRCam imaging of five widely separated sight lines in the CANUCS survey. Two-thirds of the pointings and 80% of the galaxies are covered by 12–14 NIRCam filters, including seven to nine medium bands, providing accurate photometric r…

2024 The Astrophysical Journal
eHST JWST 46