Search Publications

The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
DOI: 10.3847/1538-4357/ad97bc Bibcode: 2025ApJ...979..140W

Maseda, Michael V.; Franx, Marijn; Labbé, Ivo +15 more

We present the PANORAMIC survey, a pure parallel extragalactic imaging program with JWST/NIRCam observed during Cycle 1. The survey obtained ∼530 square arcmin of NIRCam imaging from 1–5 µm, totaling ∼192 hr of science integration time. This represents the largest on-sky time investment of any Cycle 1 GO extragalactic NIRCam imaging program …

2025 The Astrophysical Journal
Gaia 9
A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at z = 4–6
DOI: 10.3847/1538-4357/ad9d0e Bibcode: 2025ApJ...980...12S

Hennawi, Joseph F.; Shen, Yue; Fan, Xiaohui +25 more

We present a stringent measurement of the dust-obscured star formation rate density (SFRD) at z = 4–6 from the ASPIRE JWST Cycle-1 medium and ALMA Cycle-9 large program. We obtained JWST/NIRCam grism spectroscopy and ALMA 1.2 mm continuum map along 25 independent quasar sightlines, covering a total survey area of ∼35 arcmin2 where we se…

2025 The Astrophysical Journal
Gaia 8
Detection of a Highly Ionized Outflow in the Quasiperiodically Erupting Source GSN 069
DOI: 10.3847/1538-4357/ad9249 Bibcode: 2025ApJ...978...10K

Pinto, C.; Miniutti, G.; Brenneman, L. +8 more

Quasiperiodic eruptions (QPEs) are high-amplitude, soft X-ray bursts recurring every few hours, associated with supermassive black holes. Many interpretations for QPEs were proposed since their recent discovery in 2019, including extreme mass ratio inspirals and accretion disk instabilities. But, as of today, their nature still remains debated. We…

2025 The Astrophysical Journal
XMM-Newton 8
Stream Members Only: Data-driven Characterization of Stellar Streams with Mixture Density Networks
DOI: 10.3847/1538-4357/ad94f2 Bibcode: 2025ApJ...980..253S

Bovy, Jo; Bonaca, Ana; Webb, Jeremy J. +4 more

Stellar streams are sensitive probes of the Milky Way's gravitational potential. The mean track of a stream constrains global properties of the potential, while its fine-grained surface density constrains galactic substructure. A precise characterization of streams from potentially noisy data marks a crucial step in inferring galactic structure, i…

2025 The Astrophysical Journal
Gaia 7
Exploring Simple-population and Multiple-population Globular Clusters in the Outer Galactic Halo Using the Hubble Space Telescope
DOI: 10.3847/1538-4357/ad98ee Bibcode: 2025ApJ...979...30L

Milone, A. P.; Cordoni, G.; Marino, A. F. +13 more

The pseudo two-color diagram, known as chromosome map (ChM), is a valuable tool for identifying globular clusters (GCs), which consist of single or multiple stellar populations (MPs). Recent surveys of Galactic GCs using ChMs have provided stringent observational constraints on the formation of GCs and their stellar populations. However, these sur…

2025 The Astrophysical Journal
Gaia 7
Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy
DOI: 10.3847/1538-4357/ad8eba Bibcode: 2025ApJ...979..164C

Geha, M.; James, D. J.; Li, T. S. +37 more

We present the discovery of Aquarius III, an ultra-faint Milky Way satellite galaxy identified in the second data release of the DECam Local Volume Exploration survey. Based on deeper follow-up imaging with DECam, we find that Aquarius III is a low-luminosity ( ), extended (

2025 The Astrophysical Journal
Gaia 6
Closing the Stellar Labels Gap: Stellar Label independent Evidence for [α/M] Information in Gaia BP/RP Spectra
DOI: 10.3847/1538-4357/ad9607 Bibcode: 2025ApJ...979....5L

Speagle, Joshua S.; Laroche, Alexander

Data-driven models for stellar spectra that depend on stellar labels suffer from label systematics which decrease model performance: the stellar labels gap. To close the stellar labels gap, we present a stellar label independent model for Gaia BP/RP spectra. We develop a novel implementation of a variational auto-encoder, which learns to generate …

2025 The Astrophysical Journal
Gaia 6
The Size of Accretion Disks from Self-consistent X-Ray Spectra and UV/Optical/NIR Photometry Fitting: Applications to ASASSN–14li and HLX–1
DOI: 10.3847/1538-4357/ad990a Bibcode: 2025ApJ...978..167G

Mummery, Andrew; Guolo, Muryel

We implement a standard thin disk model with the outer disk radius (Rout) as a free parameter, integrating it into a standard X-ray fitting package to enable self-consistent and simultaneous fitting of X-ray spectra and Ultraviolet (UV), Optical, and Near-infrared (NIR) photometry. We apply the model to the late-time data (Δt ≈ 350–1300…

2025 The Astrophysical Journal
XMM-Newton 6
Einstein Probe Discovery of EP J005245.1‑722843: A Rare Be–White Dwarf Binary in the Small Magellanic Cloud?
DOI: 10.3847/2041-8213/ad9580 Bibcode: 2025ApJ...980L..36M

Liu, Y.; Haberl, F.; Ness, J. -U. +32 more

On 2024 May 27, the Wide-field X-ray Telescope on board the Space Sciences, University of Chinese Academy of Einstein Probe (EP) mission detected enhanced X-ray emission from a new transient source in the Small Magellanic Cloud during its commissioning phase. Prompt follow-up with the EP Follow-up X-ray Telescope, the Swift X-ray Telescope. and NI…

2025 The Astrophysical Journal
XMM-Newton 6
RIOJA. Complex Dusty Starbursts in a Major Merger B14-65666 at z = 7.15
DOI: 10.3847/1538-4357/adb02a Bibcode: 2025ApJ...981..135S

Costantin, Luca; Arribas, Santiago; Inoue, Akio K. +20 more

We present JWST NIRCam imaging of B14-65666 ("Big Three Dragons"), a bright Lyman-break galaxy system (MUV = ‑22.5 mag) at z = 7.15. The high angular resolution of NIRCam reveals the complex morphology of two galaxy components: galaxy E has a compact core (E-core), surrounded by diffuse, extended, rest-frame optical emission, which is l…

2025 The Astrophysical Journal
Gaia 5