Search Publications

A super-massive Neptune-sized planet
DOI: 10.1038/s41586-023-06499-2 Bibcode: 2023Natur.622..255N

Schlieder, Joshua E.; Howell, Steve B.; Cubillos, Patricio E. +54 more

Neptune-sized planets exhibit a wide range of compositions and densities, depending on factors related to their formation and evolution history, such as the distance from their host stars and atmospheric escape processes. They can vary from relatively low-density planets with thick hydrogen-helium atmospheres1,2 to higher-density planet…

2023 Nature
Gaia 21
Dynamical Evolution of White Dwarfs in Triples in the Era of Gaia
DOI: 10.3847/2041-8213/acf76b Bibcode: 2023ApJ...955L..14S

Angelo, Isabel; Naoz, Smadar; Hansen, Bradley M. S. +3 more

The Gaia mission has detected many white dwarfs (WDs) in binary and triple configurations, and while observations suggest that triple-stellar systems are common in our Galaxy, not much attention was devoted to WDs in triples. For stability reasons, these triples must have hierarchical configurations, i.e., two stars are on a tight orbit (the inner…

2023 The Astrophysical Journal
Gaia 21
Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
DOI: 10.3847/1538-4357/acc029 Bibcode: 2023ApJ...948..104P

Patel, Ekta; Mandel, Kaisey S.

We present new mass estimates for Andromeda (M31) using the orbital angular momenta of four satellite galaxies (M33, NGC 185, NGC 147, and IC 10) derived from existing proper motions, distances, and line-of-sight velocities. We infer two masses for M31: ${M}_{\mathrm{vir}}={2.85}_{-0.77}^{+1.47}\times {10}^{12}\,{M}_{\odot }$ using satellite galax…

2023 The Astrophysical Journal
Gaia eHST 21
Fast Radio Bursts as Probes of Magnetic Fields in Galaxies at z < 0.5
DOI: 10.3847/1538-4357/ace7bb Bibcode: 2023ApJ...954..179M

Simha, Sunil; Prochaska, J. Xavier; Rafelski, Marc +6 more

We present a sample of nine fast radio bursts (FRBs) from which we derive magnetic field strengths of the host galaxies represented by normal, z < 0.5 star-forming galaxies with stellar masses M * ≈ 108-1010.5 M . We find no correlation between the FRB rotation measure (RM) and redshift, which indica…

2023 The Astrophysical Journal
eHST 21
Stepped partially acoustic dark matter: likelihood analysis and cosmological tensions
DOI: 10.1088/1475-7516/2023/11/005 Bibcode: 2023JCAP...11..005B

Marques-Tavares, Gustavo; Buen-Abad, Manuel A.; Chacko, Zackaria +2 more

We generalize the recently proposed Stepped Partially Acoustic Dark Matter (SPartAcous) model by including additional massless degrees of freedom in the dark radiation sector. We fit SPartAcous and its generalization against cosmological precision data from the cosmic microwave background, baryon acoustic oscillations, large-scale structure, super…

2023 Journal of Cosmology and Astroparticle Physics
Gaia 21
Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon
DOI: 10.3847/1538-4357/aca807 Bibcode: 2023ApJ...943...54J

Giavalisco, Mauro; Ji, Zhiyuan

We use the spectral energy distribution fitting code PROSPECTOR to reconstruct the nonparametric star formation history (SFH) of massive ( $\mathrm{log}{M}_{* }\gt 10.3$ ) star-forming galaxies (SFGs) and quiescent galaxies (QGs) at redshift z obs ~ 2 to investigate the joint evolution of star formation activity and structural propertie…

2023 The Astrophysical Journal
eHST 21
CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 deg2 field and the impact of field-to-field variance
DOI: 10.1051/0004-6361/202245151 Bibcode: 2023A&A...670A..16G

Hu, W.; Catalano, A.; Lagache, G. +29 more

In the submillimeter regime, spectral line scans and line intensity mapping (LIM) are new promising probes for the cold gas content and star formation rate of galaxies across cosmic time. However, both of these two measurements suffer from field-to-field variance. We study the effect of field-to-field variance on the predicted CO and [CII] power s…

2023 Astronomy and Astrophysics
Herschel 21
Dissecting the interstellar medium of a z = 6.3 galaxy. X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A
DOI: 10.1051/0004-6361/202244205 Bibcode: 2023A&A...671A..84S

Covino, S.; Campana, S.; Salvaterra, R. +35 more

The study of the properties of galaxies in the first billion years after the Big Bang is one of the major topics of current astrophysics. Optical and near-infrared spectroscopy of the afterglows of long gamma-ray bursts (GRBs) provides a powerful diagnostic tool to probe the interstellar medium (ISM) of their host galaxies and foreground absorbers…

2023 Astronomy and Astrophysics
eHST 21
JWST-TST Proper Motions. I. High-precision NIRISS Calibration and Large Magellanic Cloud Kinematics
DOI: 10.3847/1538-4357/acd04f Bibcode: 2023ApJ...950..101L

Anderson, Jay; Stevenson, Kevin B.; MacDonald, Ryan J. +27 more

We develop and disseminate effective point-spread functions and geometric-distortion solutions for high-precision astrometry and photometry with the JWST NIRISS instrument. We correct field dependencies and detector effects, and assess the quality and the temporal stability of the calibrations. As a scientific application and validation, we study …

2023 The Astrophysical Journal
Gaia eHST JWST 21
The Orbital and Physical Properties of Five Southern Be+sdO Binary Systems
DOI: 10.3847/1538-3881/acc6ca Bibcode: 2023AJ....165..203W

Gies, Douglas R.; Wang, Luqian; Peters, Geraldine J. +1 more

Close binary interactions may play a critical role in the formation of the rapidly rotating Be stars. Mass transfer can result in a mass gainer star spun up by the accretion of mass and angular momentum, while the mass donor is stripped of its envelope to form a hot and faint helium star. Far-UV spectroscopy has led to the detection of about 20 su…

2023 The Astronomical Journal
Gaia IUE eHST 21