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Gaia spectroscopic orbits validated with LAMOST and GALAH radial velocities
DOI: 10.1093/mnras/stac2928 Bibcode: 2022MNRAS.517.3888B

Mazeh, T.; Faigler, S.; Jorissen, A. +5 more

The recently published Gaia DR3 catalogue of $181\, 327$ spectroscopic binaries (SB) includes the Keplerian elements of each orbit but not the measured radial velocities (RVs) and their epochs. Instead, the catalogue lists a few parameters that characterize the robustness of each solution. In this work, we use two external sources to validate the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 23
The Deuterium Isotopic Ratio of Water Released From the Martian Caps as Measured With TGO/NOMAD
DOI: 10.1029/2022GL098161 Bibcode: 2022GeoRL..4998161V

Vandaele, Ann Carine; Brines, Adrian; Aoki, Shohei +18 more

We report vertical profiles of water and D/H for one Martian year as measured with the TGO/NOMAD instrument. The observations were performed via solar occultation, providing water profiles up to ∼100 km and D/H up to ∼60 km, with a vertical resolution of 1-2 km. The measurements reveal dramatic variability of water and D/H over short timescales an…

2022 Geophysical Research Letters
ExoMars-16 23
A dynamically discovered and characterized non-accreting neutron star-M dwarf binary candidate
DOI: 10.1038/s41550-022-01766-0 Bibcode: 2022NatAs...6.1203Y

Huang, Yang; Liu, Jifeng; Bai, Yu +26 more

Typically, neutron stars are discovered by observations at radio, X-ray or gamma-ray wavelengths. Unlike radio pulsar surveys and X-ray observations, optical time-domain surveys can unveil and characterize exciting but less explored non-accreting and/or non-beaming neutron stars in binaries. Here we report the discovery of such a neutron star cand…

2022 Nature Astronomy
Gaia IUE 23
VLT/MUSE Observations of SDSS J1029+2623: Toward a High-precision Strong Lensing Model
DOI: 10.3847/1538-4357/ac3d35 Bibcode: 2022ApJ...926...86A

Brammer, Gabriel B.; Acebron, Ana; Nonino, Mario +9 more

We present a strong lensing analysis of the galaxy cluster SDSS J1029+2623 at z = 0.588, one of the few currently known lens clusters with multiple images of a background (z = 2.1992) quasar with a measured time delay. We use archival Hubble Space Telescope multiband imaging and new Multi Unit Spectroscopic Explorer follow-up spectroscopy to build…

2022 The Astrophysical Journal
Gaia eHST 23
The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
DOI: 10.1051/0004-6361/202243834 Bibcode: 2022A&A...664A.199L

Amado, P. J.; Caballero, J. A.; Pallé, E. +64 more

We report the discovery of a multiplanetary system transiting the M0 V dwarf HD 260655 (GJ 239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655 b, with a period of 2.77 d, a radius of Rb = 1.240 ± 0.023 R, a mass of Mb = 2.14 ± 0.34 M, and a bulk density of ρb

2022 Astronomy and Astrophysics
Gaia 23
J-PLUS: Spectral evolution of white dwarfs by PDF analysis
DOI: 10.1051/0004-6361/202141746 Bibcode: 2022A&A...658A..79L

Hernández-Monteagudo, C.; Gänsicke, B. T.; Carrasco, J. M. +17 more


Aims: We estimated the spectral evolution of white dwarfs with effective temperature using the Javalambre Photometric Local Universe Survey (J-PLUS) second data release (DR2), which provides 12 photometric optical passbands over 2176 deg2.
Methods: We analyzed 5926 white dwarfs with r ≤ 19.5 mag in common between a white dwarf…

2022 Astronomy and Astrophysics
Gaia 23
New Photometric Calibration of the Wide Field Camera 3 Detectors
DOI: 10.3847/1538-3881/ac73f0 Bibcode: 2022AJ....164...32C

Mack, Jennifer; Calamida, Annalisa; Medina, Jennifer +6 more

We present a new photometric calibration of the WFC3-UVIS and WFC3-IR detectors based on observations collected from 2009 to 2020 for four white dwarfs-namely, GRW +70 5824, GD 153 , GD 71 , G191B2B-and a G-type star, P330E. These calibrations include recent updates to the Hubble Space Telescope primary standard white dwarf models and a new refere…

2022 The Astronomical Journal
eHST 23
Stellar Loci. V. Photometric Metallicities of 27 Million FGK Stars Based on Gaia Early Data Release 3
DOI: 10.3847/1538-4365/ac3df6 Bibcode: 2022ApJS..258...44X

Huang, Yang; Niu, Zexi; Beers, Timothy C. +3 more

We combine LAMOST DR7 spectroscopic data and Gaia EDR3 photometric data to construct high-quality giant (0.7 < (BP - RP) < 1.4) and dwarf (0.5 < (BP - RP) < 1.5) samples in the high Galactic latitude region, with precise corrections for magnitude-dependent systematic errors in the Gaia photometry and careful reddening corrections using…

2022 The Astrophysical Journal Supplement Series
Gaia 23
Limits on the mass and initial entropy of 51 Eri b from Gaia EDR3 astrometry
DOI: 10.1093/mnras/stab3148 Bibcode: 2022MNRAS.509.4411D

Dupuy, Trent J.; Brandt, Timothy D.; Brandt, G. Mirek

51 Eri b is one of the only young planets consistent with a wide range of possible initial entropy states, including the cold-start scenario associated with some models of planet formation by core accretion. The most direct way to constrain the initial entropy of a planet is by measuring its luminosity and mass at a sufficiently young age that the…

2022 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 23
Bright, relatively isolated star clusters in PHANGS-HST galaxies: Aperture corrections, quantitative morphologies, and comparison with synthetic stellar population models
DOI: 10.1093/mnras/stab3213 Bibcode: 2022MNRAS.510...32D

Kruijssen, J. M. Diederik; Rosolowsky, Erik; Glover, Simon C. O. +14 more

Using PHANGS-HST NUV-U-B-V-I imaging of 17 nearby spiral galaxies, we study samples of star clusters and stellar associations, visually selected to be bright and relatively isolated, for three purposes: to compute aperture corrections for star cluster photometry, to explore the utility of quantitative morphologies in the analysis of clusters and a…

2022 Monthly Notices of the Royal Astronomical Society
eHST 23