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Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 b
DOI: 10.1051/0004-6361/202142653 Bibcode: 2022A&A...659A..17K

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

We report the discovery of GJ 3929 b, a hot Earth-sized planet orbiting the nearby M3.5 V dwarf star, GJ 3929 (G 180-18, TOI-2013). Joint modelling of photometric observations from TESS sectors 24 and 25 together with 73 spectroscopic observations from CARMENES and follow-up transit observations from SAINT-EX, LCOGT, and OSN yields a planet radius…

2022 Astronomy and Astrophysics
Gaia 16
Estimating the local dark matter density in a non-axisymmetric wobbling disc
DOI: 10.1093/mnras/stac094 Bibcode: 2022MNRAS.511.1977S

Sivertsson, S.; Read, J. I.; Silverwood, H. +6 more

The density of dark matter near the Sun, ρDM, ⊙, is important for experiments hunting for dark matter particles in the laboratory, and for constraining the local shape of the Milky Way's dark matter halo. Estimates to date have typically assumed that the Milky Way's stellar disc is axisymmetric and in a steady-state. Yet the Milky Way d…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
A machine-learning photometric classifier for massive stars in nearby galaxies. I. The method
DOI: 10.1051/0004-6361/202141397 Bibcode: 2022A&A...666A.122M

Yang, Ming; Bonanos, Alceste Z.; Maravelias, Grigoris +3 more

Context. Mass loss is a key parameter in the evolution of massive stars. Despite the recent progress in the theoretical understanding of how stars lose mass, discrepancies between theory and observations still hold. Moreover, episodic mass loss in evolved massive stars is not included in models, and the importance of its role in the evolution of m…

2022 Astronomy and Astrophysics
Gaia 16
High-resolution Hubble Space Telescope Imaging Survey of Local Star-forming Galaxies. I. Spatially Resolved Obscured Star Formation with Hα and Paschen-β Recombination Lines
DOI: 10.3847/1538-4365/ac958c Bibcode: 2022ApJS..263...17G

Perna, Michele; Calzetti, Daniela; Colina, Luis +9 more

We present a sample of 24 local star-forming galaxies observed with broadband and narrowband photometry from the Hubble Space Telescope (HST) that are part of the Great Observatories All-sky Luminous Infrared Galaxies Survey of local luminous and ultraluminous infrared galaxies. With narrowband filters around the emission lines Hα (and [N II]) and…

2022 The Astrophysical Journal Supplement Series
eHST 16
The Pristine survey - XVII. The C-19 stream is dynamically hot and more extended than previously thought
DOI: 10.1093/mnras/stac1399 Bibcode: 2022MNRAS.514.1664Y

Fouesneau, Morgan; Sestito, Federico; Navarro, Julio F. +22 more

The C-19 stream is the most metal-poor stellar system ever discovered, with a mean metallicity [Fe/H] = -3.38 ± 0.06. Its low metallicity dispersion (σ[Fe/H] < 0.18 at the 95 per cent confidence level) and variations in sodium abundances strongly suggest a globular cluster origin. In this work, we use Very Large Telescope (VLT)/UV-Vi…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
Photometric Metallicity Prediction of Fundamental-mode RR Lyrae Stars in the Gaia Optical and K s Infrared Wave Bands by Deep Learning
DOI: 10.3847/1538-4365/ac74ba Bibcode: 2022ApJS..261...33D

Grebel, Eva K.; Dékány, István

RR Lyrae stars are useful chemical tracers thanks to the empirical relationship between their heavy-element abundance and the shape of their light curves. However, the consistent and accurate calibration of this relation across multiple photometric wave bands has been lacking. We have devised a new method for the metallicity estimation of fundamen…

2022 The Astrophysical Journal Supplement Series
Gaia 16
The stable climate of KELT-9b
DOI: 10.1051/0004-6361/202243823 Bibcode: 2022A&A...666A.118J

Alonso, R.; Deleuil, M.; Erikson, A. +76 more

Even among the most irradiated gas giants, so-called ultra-hot Jupiters, KELT-9b stands out as the hottest planet thus far discovered with a dayside temperature of over 4500 K. At these extreme irradiation levels, we expect an increase in heat redistribution efficiency and a low Bond albedo owed to an extended atmosphere with molecular hydrogen di…

2022 Astronomy and Astrophysics
CHEOPS Gaia 16
Antaeus: A Retrograde Group of Tidal Debris in the Milky Way's Disk Plane
DOI: 10.3847/2041-8213/ac86d3 Bibcode: 2022ApJ...936L...3O

Martin, Nicolas; Famaey, Benoit; Viswanathan, Akshara +5 more

We present the discovery of a wide retrograde moving group in the disk plane of the Milky Way using action-angle coordinates derived from the Gaia DR3 catalog. The structure is identified from a sample of its members that are currently almost at the pericenter of their orbit and are passing through the solar neighborhood. The motions of the stars …

2022 The Astrophysical Journal
Gaia 16
MICROSCOPE satellite and its drag-free and attitude control system
DOI: 10.1088/1361-6382/ac09cd Bibcode: 2022CQGra..39t4003R

Bergé, Joel; Chhun, Ratana; Métris, Gilles +14 more

This paper focuses on the description of the design and performance of the MICROSCOPE satellite and its drag-free and attitude control system. The satellite is derived from CNES' Myriade platform family, albeit with significant upgrades dictated by the unprecedented MICROSCOPE's mission requirements. The 300 kg drag-free microsatellite has complet…

2022 Classical and Quantum Gravity
MICROSCOPE 16
To E or Not to E : Numerical Nuances of Global Coronal Models
DOI: 10.3847/1538-4365/ac8eb1 Bibcode: 2022ApJS..263...18B

Poedts, Stefaan; Perri, Barbara; Lani, Andrea +2 more

In recent years, global coronal models have experienced an ongoing increase in popularity as tools for forecasting solar weather. Within the domain of up to 21.5 R , magnetohydrodynamics (MHD) is used to resolve the coronal structure using magnetograms as inputs at the solar surface. Ideally, these computations would be repeated with e…

2022 The Astrophysical Journal Supplement Series
SOHO 16