Search Publications

Evidence for mass-dependent peculiar velocities in compact object binaries: towards better constraints on natal kicks
DOI: 10.1093/mnras/stad2226 Bibcode: 2023MNRAS.525.1498Z

Maccarone, Thomas J.; Gandhi, Poshak; Zhao, Yue +4 more

We compile a catalogue of low-mass and high-mass X-ray binaries, some recently reported binaries that likely host a neutron star (NS) or a black hole (BH), and binary pulsars (a pulsar and a non-degenerated companion) that have measured systemic radial velocities (γ). Using Gaia and radio proper motions together with γ, we integrate their Galactic…

2023 Monthly Notices of the Royal Astronomical Society
Gaia INTEGRAL 18
The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars
DOI: 10.3847/1538-4357/aca322 Bibcode: 2023ApJ...943...23S

Beers, Timothy C.; Placco, Vinicius M.; Holmbeck, Erika M. +8 more

Orbital characteristics based on Gaia Early Data Release 3 astrometric parameters are analyzed for ~1700 r-process-enhanced (RPE; [Eu/Fe] > +0.3) metal-poor stars ([Fe/H] ≤ -0.8) compiled from the R-Process Alliance, the GALactic Archaeology with HERMES (GALAH) DR3 survey, and additional literature sources. We find dynamical clusters of these s…

2023 The Astrophysical Journal
Gaia 18
Metal-enriched Neutral Gas Reservoir around a Strongly Lensed Low-mass Galaxy at z = 4 Identified by JWST/NIRISS and VLT/MUSE
DOI: 10.3847/2041-8213/aca1c4 Bibcode: 2023ApJ...944L..59L

Chevallard, Jacopo; Fan, Xiaohui; Schaerer, Daniel +19 more

Direct observations of low-mass, low-metallicity galaxies at z ≳ 4 provide an indispensable opportunity for detailed inspection of the ionization radiation, gas flow, and metal enrichment in sources similar to those that reionized the universe. Combining the James Webb Space Telescope (JWST), Very Large Telescope/MUSE, and Atacama Large Millimeter…

2023 The Astrophysical Journal
eHST JWST 18
X-ray polarimetry of the accreting pulsar GX 301−2
DOI: 10.1051/0004-6361/202346994 Bibcode: 2023A&A...678A.119S

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +102 more

The phase- and energy-resolved polarization measurements of accreting X-ray pulsars (XRPs) allow us to test different theoretical models of their emission, and they also provide an avenue to determine the emission region geometry. We present the results of the observations of the XRP GX 301−2 performed with the Imaging X-ray Polarimetry Explorer (…

2023 Astronomy and Astrophysics
Gaia 18
The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging
DOI: 10.3847/1538-4365/acb8ae Bibcode: 2023ApJS..265...40R

Papovich, Casey; Henry, Alaina; Rafelski, Marc +18 more

We present extremely deep Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) observations of the MUSE Ultra Deep Field. This unique region of the sky contains two quasars at z ≈ 3.22 that are separated by only ~500 kpc, providing a stereoscopic view of gas and galaxies in emission and absorption across ~10 billion years of cosmic time. We hav…

2023 The Astrophysical Journal Supplement Series
Gaia eHST 18
Updated radial velocities and new constraints on the nature of the unseen source in NGC1850 BH1
DOI: 10.1093/mnras/stad764 Bibcode: 2023MNRAS.521.3162S

Usher, C.; Bastian, N.; Saracino, S. +7 more

A black hole candidate orbiting a luminous star in the Large Magellanic Cloud young cluster NGC 1850 (~100 Myr) has recently been reported based on radial velocity and light-curve modelling. Subsequently, an alternative explanation has been suggested for the system: a bloated post-mass transfer secondary star (Minitial ~ 4-5 M

2023 Monthly Notices of the Royal Astronomical Society
eHST 18
An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in 1.3 ≤z ≤2.6 Star-forming Galaxies from MOSDEF
DOI: 10.3847/1538-4357/accdd1 Bibcode: 2023ApJ...951...29L

Barro, Guillermo; Siana, Brian; Shapley, Alice E. +10 more

We investigate dust attenuation and its dependence on viewing angle for 308 star-forming galaxies at 1.3 ≤ z ≤ 2.6 from the MOSFIRE Deep Evolution Field survey. We divide galaxies with a detected Hα emission line and coverage of Hβ into eight groups by stellar mass, star formation rate (SFR), and inclination (i.e., axis ratio), and we then stack t…

2023 The Astrophysical Journal
eHST 18
Scaling K2. VI. Reduced Small-planet Occurrence in High-galactic-amplitude Stars
DOI: 10.3847/1538-3881/acd24c Bibcode: 2023AJ....165..262Z

Rice, Malena; Howard, Andrew W.; Petigura, Erik A. +13 more

In this study, we performed a homogeneous analysis of the planets around FGK dwarf stars observed by the Kepler and K2 missions, providing spectroscopic parameters for 310 K2 targets -including 239 Scaling K2 hosts-observed with Keck/HIRES. For orbital periods less than 40 days, we found that the distribution of planets as a function of orbital pe…

2023 The Astronomical Journal
Gaia 18
A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants
DOI: 10.3847/1538-4357/acb13d Bibcode: 2023ApJ...944..168L

Li, Wenhao; Ryan, Russell; Drory, Niv +9 more

We investigate the role of galaxy mergers in triggering active galactic nuclei (AGN) in the nearby universe. Our analysis is based on a sample of 79 post-merger remnant galaxies with deep X-ray observations from Chandra/XMM-Newton capable of detecting a low-luminosity AGN of ≥1040.5 erg s-1. This sample is derived from a visu…

2023 The Astrophysical Journal
XMM-Newton 18
55 Cancri e's occultation captured with CHEOPS
DOI: 10.1051/0004-6361/202244894 Bibcode: 2023A&A...669A..64D

Alonso, R.; Deleuil, M.; Erikson, A. +73 more

Past occultation and phase-curve observations of the ultra-short period super-Earth 55 Cnc e obtained at visible and infrared wavelengths have been challenging to reconcile with a planetary reflection and emission model. In this study, we analyse a set of 41 occultations obtained over a two-year timespan with the CHEOPS satellite. We report the de…

2023 Astronomy and Astrophysics
CHEOPS 18