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Characterisation of the upper atmospheres of HAT-P-32 b, WASP-69 b, GJ 1214 b, and WASP-76 b through their He I triplet absorption
DOI: 10.1051/0004-6361/202245649 Bibcode: 2023A&A...673A.140L

Sánchez-López, A.; López-Puertas, M.; Amado, P. J. +14 more

Characterisation of atmospheres undergoing photo-evaporation is key to understanding the formation, evolution, and diversity of planets. However, only a few upper atmospheres that experience this kind of hydrodynamic escape have been characterised. Our aim is to characterise the upper atmospheres of the hot Jupiters HAT-P-32b and WASP-69 b, the wa…

2023 Astronomy and Astrophysics
Gaia eHST 24
A Mars orbital catalog of aqueous alteration signatures (MOCAAS)
DOI: 10.1016/j.icarus.2022.115164 Bibcode: 2023Icar..38915164C

Bibring, Jean-Pierre; Langevin, Yves; Gondet, Brigitte +3 more

We describe the completion of the MOCAAS project providing a global repository of secondary minerals formed through interaction with water on Mars. This work is based on the analysis of orbital imaging spectroscopy data from the OMEGA/Mars Express and CRISM/MRO near-infrared instruments. A database and a set of high-resolution global maps (200 m/p…

2023 Icarus
MEx 24
Minor Merger Growth in Action: JWST Detects Faint Blue Companions around Massive Quiescent Galaxies at 0.5 ≤ z ≤ 3.0
DOI: 10.3847/2041-8213/acf5e6 Bibcode: 2023ApJ...956L..42S

Carniani, Stefano; Übler, Hannah; D'Eugenio, Francesco +17 more

Minor mergers are thought to drive the structural evolution of massive quiescent galaxies; however, existing Hubble Space Telescope (HST) imaging is primarily sensitive to stellar mass ratios ≳1:10. Here, we report the discovery of a large population of low-mass companions within 35 kpc of known $\mathrm{log}{M}_{* }/{M}_{\odot }\gtrsim 10.5$ quie…

2023 The Astrophysical Journal
eHST JWST 24
The bright extragalactic ALMA redshift survey (BEARS) - II. Millimetre photometry of gravitational lens candidates
DOI: 10.1093/mnras/stac3771 Bibcode: 2023MNRAS.522.2995B

Berta, S.; Andreani, P.; Pérez-Fournon, I. +49 more

We present 101- and 151-GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500-µm flux densities >80 mJy and 250-500-µm colours consistent with z > 2, most of which are expected to be gravitationally lensed or hyperluminous infrared galaxies. Approximately half of the Herschel 500-µm sourc…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 24
Combining the CLAUDS and HSC-SSP surveys. U + grizy(+YJHKs) photometry and photometric redshifts for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields
DOI: 10.1051/0004-6361/202243363 Bibcode: 2023A&A...670A..82D

Ilbert, O.; Paltani, S.; Furusawa, H. +21 more

We present the combination of the Canada-France-Hawaii Telescope (CHFT) Large Area U-bands Deep Survey (CLAUDS) and the Hyper-Suprime-Cam (HSC) Subaru Strategic Program (HSC-SSP) data over their four deep fields. We provide photometric catalogs for u, u* (CFHT-MegaCam), g, r, i, z, and y (Subaru-HSC) bands over ~20 deg2, comp…

2023 Astronomy and Astrophysics
eHST 24
The SPIRou legacy survey. Rotation period of quiet M dwarfs from circular polarization in near-infrared spectral lines: The SPIRou APERO analysis
DOI: 10.1051/0004-6361/202345839 Bibcode: 2023A&A...672A..52F

Moutou, C.; Carmona, A.; Donati, J. -F. +21 more

Context. The rotation period of stars is an important parameter together with mass, radius, and effective temperature. It is an essential parameter for any radial velocity monitoring, as stellar activity can mimic the presence of a planet at the stellar rotation period. Several methods exist to measure it, including long sequences of photometric m…

2023 Astronomy and Astrophysics
Gaia 24
The Giant Accreting Protoplanet Survey (GAPlanetS)-Results from a 6 yr Campaign to Image Accreting Protoplanets
DOI: 10.3847/1538-3881/acc183 Bibcode: 2023AJ....165..225F

Weinberger, Alycia J.; De Rosa, Robert J.; Macintosh, Bruce +21 more

Accreting protoplanets are windows into planet formation processes, and high-contrast differential imaging is an effective way to identify them. We report results from the Giant Accreting Protoplanet Survey (GAPlanetS), which collected Hα differential imagery of 14 transitional disk host stars with the Magellan Adaptive Optics System. To address t…

2023 The Astronomical Journal
Gaia 24
An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244)
DOI: 10.1051/0004-6361/202346550 Bibcode: 2023A&A...675A..52C

Deleuil, M.; Zapatero Osorio, M. R.; Allende Prieto, C. +34 more

Context. Small planets located at the lower mode of the bimodal radius distribution are generally assumed to be composed of iron and silicates in a proportion similar to that of the Earth. However, recent discoveries are revealing a new group of low-density planets that are inconsistent with that description.
Aims: We intend to confirm and ch…

2023 Astronomy and Astrophysics
Gaia 24
The Hubble Space Telescope Survey of M31 Satellite Galaxies. II. The Star Formation Histories of Ultrafaint Dwarf Galaxies
DOI: 10.3847/1538-4357/acf46f Bibcode: 2023ApJ...956...86S

Lewis, Geraint F.; Cooper, M. C.; Brown, Thomas M. +34 more

We present the lifetime star formation histories (SFHs) for six ultrafaint dwarf (UFD; M V > - 7.0, $4.9\lt {\mathrm{log}}_{10}({M}_{* }(z=0)/{M}_{\odot })\lt 5.5$ ) satellite galaxies of M31 based on deep color-magnitude diagrams constructed from Hubble Space Telescope imaging. These are the first SFHs obtained from the oldest mai…

2023 The Astrophysical Journal
eHST 24
The Quest for the Missing Dust. II. Two Orders of Magnitude of Evolution in the Dust-to-gas Ratio Resolved within Local Group Galaxies
DOI: 10.3847/1538-4357/acbb66 Bibcode: 2023ApJ...946...42C

Gordon, Karl D.; Bot, Caroline; Clark, Christopher J. R. +3 more

We explore evolution in the dust-to-gas ratio with density within four well-resolved Local Group galaxies-the LMC, SMC, M31, and M33. We do this using new Herschel maps, which restore extended emission that was missed by previous Herschel reductions. Combining this sensitivity to diffuse dust emission with excellent physical resolution allows us t…

2023 The Astrophysical Journal
Herschel 23