Search Publications

Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
DOI: 10.3847/1538-4357/acfafd Bibcode: 2023ApJ...958...33F

Chary, Ranga-Ram; Taylor, Peter; Jee, M. James +5 more

We have undertaken a near-IR weak-lensing (NIRWL) analysis of the CANDELS HST/WFC3-IR F160W observations. With the Gaia proper motion–corrected catalog as an astrometric reference, we updated the astrometry of the five CANDELS mosaics and achieved an absolute alignment within 0.″02 ± 0.″02, on average, which is a factor of several superior to exis…

2023 The Astrophysical Journal
Gaia eHST 14
A major asymmetric ice trap in a planet-forming disk. IV. Nitric oxide gas and a lack of CN tracing sublimating ices and a C/O ratio <1
DOI: 10.1051/0004-6361/202245662 Bibcode: 2023A&A...673A...7L

van der Marel, N.; van Dishoeck, E. F.; Tabone, B. +5 more

Context. Most well-resolved disks observed with the Atacama Large Millimeter/submillimeter Array (ALMA) show signs of dust traps. These dust traps set the chemical composition of the planet-forming material in these disks, as the dust grains with their icy mantles are trapped at specific radii and could deplete the gas and dust at smaller radii of…

2023 Astronomy and Astrophysics
Herschel 14
Probing minimal grand unification through gravitational waves, proton decay, and fermion masses
DOI: 10.1007/JHEP04(2023)058 Bibcode: 2023JHEP...04..058S

Saad, Shaikh

Motivated by the direct discovery of gravitational waves (GWs) from black holes and neutron stars, there is a growing interest in investigating GWs from other sources. Among them, GWs from cosmic strings are particularly fascinating since they naturally appear in a large class of grand unified theories (GUTs). Remarkably, a series of pulsar-timing…

2023 Journal of High Energy Physics
Gaia 14
Evidence of an age gradient along the line of sight in the nuclear stellar disc of the Milky Way
DOI: 10.1051/0004-6361/202345941 Bibcode: 2023A&A...671L..10N

Schultheis, M.; Rich, R. M.; Najarro, F. +3 more

Context. The nuclear stellar disc (NSD) is a flat dense stellar structure at the heart of the Milky Way. Recent work has shown that analogous structures are common in the nuclei of external spiral galaxies, where there is evidence of an age gradient that indicates that they form inside-out. However, the characterisation of the age of the NSD stell…

2023 Astronomy and Astrophysics
Gaia 14
SRG/eROSITA discovery of a radio-faint X-ray candidate supernova remnant SRGe J003602.3+605421 = G121.1-1.9
DOI: 10.1093/mnras/stad818 Bibcode: 2023MNRAS.521.5536K

Sunyaev, R. A.; Churazov, E. M.; Khabibullin, I. I. +2 more

We report the discovery of a candidate X-ray supernova remnant SRGe J003602.3+605421 = G121.1-1.9 in the course of the SRG/eROSITA all-sky survey. The object is located at (l, b) = (121.1°, -1.9°), is ≈36 arcmin in angular size, and has a nearly circular shape. Clear variations in the spectral shape of the X-ray emission across the object are dete…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 14
The Physical Thickness of Stellar Disks to z ∼ 2
DOI: 10.3847/1538-4357/acf211 Bibcode: 2023ApJ...956..147H

Heckman, Timothy M.; Snyder, Gregory F.; Simons, Raymond C. +2 more

In local disk galaxies such as our Milky Way, older stars generally inhabit a thicker disk than their younger counterparts. Two competing models have attempted to explain this result: one in which stars first form in thin disks that gradually thicken with time through dynamical heating, and one in which stars form in thick disks at early times and…

2023 The Astrophysical Journal
eHST 14
Characterizing a World Within the Hot-Neptune Desert: Transit Observations of LTT 9779 b with the Hubble Space Telescope/WFC3
DOI: 10.3847/1538-3881/acea77 Bibcode: 2023AJ....166..158E

Ward-Thompson, Derek; Stassun, Keivan G.; France, Kevin +27 more

We present an atmospheric analysis of LTT 9779 b, a rare planet situated in the hot-Neptune desert, that has been observed with Hubble Space Telescope (HST)/WFC3 with G102 and G141. The combined transmission spectrum, which covers 0.8-1.6 µm, shows a gradual increase in transit depth with wavelength. Our preferred atmospheric model shows evi…

2023 The Astronomical Journal
eHST 14
TESS and CHEOPS discover two warm sub-Neptunes transiting the bright K-dwarf HD 15906
DOI: 10.1093/mnras/stad1369 Bibcode: 2023MNRAS.523.3090T

Alonso, R.; Deleuil, M.; Erikson, A. +119 more

We report the discovery of two warm sub-Neptunes transiting the bright (G = 9.5 mag) K-dwarf HD 15906 (TOI 461, TIC 4646810). This star was observed by the Transiting Exoplanet Survey Satellite (TESS) in sectors 4 and 31, revealing two small transiting planets. The inner planet, HD 15906 b, was detected with an unambiguous period but the outer pla…

2023 Monthly Notices of the Royal Astronomical Society
CHEOPS Gaia 14
TOI 4201 b and TOI 5344 b: Discovery of Two Transiting Giant Planets around M-dwarf Stars and Revised Parameters for Three Others
DOI: 10.3847/1538-3881/acf56e Bibcode: 2023AJ....166..163H

Kostov, Veselin B.; Vanderburg, Andrew; Triaud, Amaury H. M. J. +62 more

We present the discovery from the TESS mission of two giant planets transiting M-dwarf stars: TOI 4201 b and TOI 5344 b. We also provide precise radial velocity measurements and updated system parameters for three other M dwarfs with transiting giant planets: TOI 519, TOI 3629, and TOI 3714. We measure planetary masses of 0.525 ± 0.064 M J

2023 The Astronomical Journal
Gaia 14
Molecular Mapping of DR Tau's Protoplanetary Disk, Envelope, Outflow, and Large-scale Spiral Arm
DOI: 10.3847/1538-4357/aca89c Bibcode: 2023ApJ...943..107H

Andrews, Sean M.; Bae, Jaehan; Bergin, Edwin A. +2 more

DR Tau has been noted for its unusually high variability in comparison with other T Tauri stars. Although it is one of the most extensively studied pre-main-sequence stars, observations with millimeter interferometry have so far been relatively limited. We present NOEMA images of 12CO, 13CO, C18O, SO, DCO+

2023 The Astrophysical Journal
Gaia 14