Search Publications

JWST NIRCam Defocused Imaging: Photometric Stability Performance and How It Can Sense Mirror Tilts
DOI: 10.1088/1538-3873/aca718 Bibcode: 2023PASP..135a8001S

Gennaro, Mario; Espinoza, Néstor; Perrin, Marshall D. +25 more

We use JWST NIRCam short-wavelength photometry to capture a transit lightcurve of the exoplanet HAT-P-14 b to assess performance as part of instrument commissioning. The short-wavelength precision is 152 ppm per 27 s integration as measured over the full time series compared to a theoretical limit of 107 ppm, after corrections to spatially correla…

2023 Publications of the Astronomical Society of the Pacific
JWST 17
A hidden population of white dwarfs with atmospheric carbon traces in the Gaia bifurcation
DOI: 10.1051/0004-6361/202346628 Bibcode: 2023A&A...674A.213C

Rebassa-Mansergas, Alberto; Hollands, Mark; Althaus, Leandro G. +4 more

Context. The high-quality photometric and astrometric capabilities of the ESA Gaia space mission have revealed a bifurcation of the white dwarf sequence on the color magnitude diagram with two branches: A and B. While the A branch consists mostly of white dwarfs with hydrogen(H)-rich atmospheres, the B branch is not completely understood. Although…

2023 Astronomy and Astrophysics
Gaia 17
TOI-5678b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS★
DOI: 10.1051/0004-6361/202245478 Bibcode: 2023A&A...674A..43U

Alonso, R.; Bouchy, F.; Deleuil, M. +92 more

Context. A large sample of long-period giant planets has been discovered thanks to long-term radial velocity surveys, but only a few dozen of these planets have a precise radius measurement. Transiting gas giants are crucial targets for the study of atmospheric composition across a wide range of equilibrium temperatures and, more importantly, for …

2023 Astronomy and Astrophysics
CHEOPS Gaia 17
Two decades of optical timing of the shortest-period binary star system HM Cancri
DOI: 10.1093/mnras/stac3385 Bibcode: 2023MNRAS.518.5123M

Dhillon, V. S.; Hollands, Mark; Parsons, Steven G. +15 more

The shortest-period binary star system known to date, RX J0806.3+1527 (HM Cancri), has now been observed in the optical for more than two decades. Although it is thought to be a double degenerate binary undergoing mass transfer, an early surprise was that its orbital frequency, f0, is currently increasing as the result of gravitational …

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 17
Benchmarking MESA isochrones against the Hyades single star sequence
DOI: 10.1093/mnras/stac2247 Bibcode: 2023MNRAS.518..662B

Brandner, Wolfgang; Calissendorff, Per; Kopytova, Taisiya

Based on GAIA Early Data Release 3 (EDR3), we revisit and update our sample of bonafide single stars in the Hyades open cluster. The small observational uncertainties in parallax and photometry of EDR3 result in a tightly defined stellar sequence, which is ideal for the testing and calibration of theoretical stellar evolutionary tracks and isochro…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 17
Beyond Spectroscopy. II. Stellar Parameters for over 20 Million Stars in the Northern Sky from SAGES DR1 and Gaia DR3
DOI: 10.3847/1538-4357/ace628 Bibcode: 2023ApJ...957...65H

Tan, Ke-Feng; Zhao, Gang; Fan, Zhou +18 more

We present precise photometric estimates of stellar parameters, including effective temperature, metallicity, luminosity classification, distance, and stellar age, for nearly 26 million stars using the methodology developed in the first paper of this series, based on the stellar colors from the Stellar Abundances and Galactic Evolution Survey (SAG…

2023 The Astrophysical Journal
Gaia 17
The ALMA REBELS Survey: discovery of a massive, highly star-forming, and morphologically complex ULIRG at z = 7.31
DOI: 10.1093/mnras/stad1212 Bibcode: 2023MNRAS.524.1775H

Inami, H.; Bowler, R. A. A.; Rybak, M. +27 more

We present Atacama Large Millimeter/Submillimeter Array (ALMA) [C II] and ~158 $\rm \mu m$ continuum observations of REBELS-25, a massive, morphologically complex ultra-luminous infrared galaxy (ULIRG; LIR = $1.5^{+0.8}_{-0.5} \times 10^{12}$ L) at z = 7.31, spectroscopically confirmed by the Reionization Era Bright Emission…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 17
Estimating reddening of the continuum and broad-line region of active galactic nuclei: the mean reddening of NGC 5548 and the size of the accretion disc
DOI: 10.1093/mnras/stac3333 Bibcode: 2023MNRAS.519.4082G

Gaskell, C. Martin; Anderson, Frances C.; Birmingham, Sufia Á. +1 more

We use seven different methods to estimate broad-line and continuum reddenings of NGC 5548. We investigate two possible reddening curves considered for active galactic nuclei (AGNs): the mean AGN reddening curve of Gaskell & Benker (2007) which is relatively flat in the ultraviolet, and a curve that rises strongly into the ultraviolet like a S…

2023 Monthly Notices of the Royal Astronomical Society
eHST 17
Analytic model for off-axis GRB afterglow images - geometry measurement and implications for measuring H0
DOI: 10.1093/mnras/stad1628 Bibcode: 2023MNRAS.524..403G

Nakar, Ehud; Govreen-Segal, Taya

We present an analytic model for measuring the jet core angle (θc) and viewing angle (θobs) of off-axis gamma-ray bursts independently of the jet angular structure outside of the core. We model the images of off-axis jets, and using this model, we show that θobs and θc can be measured using any two of th…

2023 Monthly Notices of the Royal Astronomical Society
eHST 17
Characterizing three-dimensional magnetic field, turbulence, and self-gravity in the star-forming region L1688
DOI: 10.1093/mnras/stad2158 Bibcode: 2023MNRAS.524.4431H

Lazarian, A.; Hu, Yue

Interaction of three-dimensional magnetic fields, turbulence, and self-gravity in the molecular cloud is crucial in understanding star formation but has not been addressed so far. In this work, we target the low-mass star-forming region L1688 and use the spectral emissions of 12CO, 13CO, C18O, and H I, as well as p…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 17