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Warm terrestrial planet with half the mass of Venus transiting a nearby star
DOI: 10.1051/0004-6361/202140728 Bibcode: 2021A&A...653A..41D

Bouchy, F.; Rebolo, R.; Pallé, E. +42 more

In recent years, the advent of a new generation of radial velocity instruments has allowed us to detect planets with increasingly lower mass and to break the one Earth-mass barrier. Here we report a new milestone in this context by announcing the detection of the lowest-mass planet measured so far using radial velocities: L 98-59 b, a rocky planet…

2021 Astronomy and Astrophysics
Gaia 77
Gaia EDR3 Reveals the Substructure and Complicated Star Formation History of the Greater Taurus-Auriga Star-forming Complex
DOI: 10.3847/1538-3881/ac0632 Bibcode: 2021AJ....162..110K

Rizzuto, Aaron C.; Kraus, Adam L.; Krolikowski, Daniel M.

The Taurus-Auriga complex is the prototypical low-mass star-forming region, and provides a unique testbed of the star formation process, which left observable imprints on the spatial, kinematic, and temporal structure of its stellar population. Taurus's rich observational history has uncovered peculiarities that suggest a complicated star-forming …

2021 The Astronomical Journal
Gaia 77
Three Lyman-α-emitting filaments converging to a massive galaxy group at z = 2.91: discussing the case for cold gas infall
DOI: 10.1051/0004-6361/202038700 Bibcode: 2021A&A...649A..78D

Finoguenov, A.; Daddi, E.; Elbaz, D. +21 more

We have discovered a 300 kpc-wide giant Lyman-α (Lyα) nebula centered on the massive galaxy group RO-1001 at z = 2.91 in the Cosmic Evolution Survey field. Keck Cosmic Web Imager observations reveal three cold gas filaments converging into the center of the potential well of its ∼4 × 1013 M dark matter halo, hosting 1200 M

2021 Astronomy and Astrophysics
Herschel XMM-Newton eHST 77
The Extragalactic Distance Database: The Color-Magnitude Diagrams/Tip of the Red Giant Branch Distance Catalog
DOI: 10.3847/1538-3881/ac0440 Bibcode: 2021AJ....162...80A

Dolphin, Andrew E.; Wu, Po-Feng; Anand, Gagandeep S. +7 more

The Extragalactic Distance Database (EDD) was created as a repository for high-quality, redshift-independent distances. A key component of EDD is the Color-Magnitude Diagrams/Tip of the Red Giant Branch (CMDs/TRGB) catalog, which provides information on the stellar content of nearby galaxies observed with the Hubble Space Telescope (HST). Here we …

2021 The Astronomical Journal
Gaia eHST 77
Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
DOI: 10.1103/PhysRevD.103.123501 Bibcode: 2021PhRvD.103l3501S

Seto, Osamu; Toda, Yo

A shorter sound horizon scale at the recombination epoch, arising from introducing extra energy components such as extra radiation or early dark energy (EDE), is a simple approach to resolving the so-called Hubble tension. We compare EDE models, an extra radiation model, and a model in which EDE and extra radiation coexist, paying attention to the…

2021 Physical Review D
eHST 77
The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview
DOI: 10.1051/0004-6361/202039632 Bibcode: 2021A&A...650A.104C

Okabe, N.; Aussel, H.; Arnaud, M. +66 more

The Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) is a three-mega-second Multi-Year Heritage Programme to obtain X-ray observations of a minimally-biased, signal-to-noise-limited sample of 118 galaxy clusters detected by Planck through the Sunyaev-Zeldovich effect. Th…

2021 Astronomy and Astrophysics
XMM-Newton 77
Dark Energy Survey year 3 results: point spread function modelling
DOI: 10.1093/mnras/staa3679 Bibcode: 2021MNRAS.501.1282J

Bechtol, K.; Smith, M.; Abbott, T. M. C. +79 more

We introduce a new software package for modelling the point spread function (PSF) of astronomical images, called PIFF (PSFs In the Full FOV), which we apply to the first three years (known as Y3) of the Dark Energy Survey (DES) data. We describe the relevant details about the algorithms used by PIFF to model the PSF, including how the PSF model va…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 76
Characterizing Extreme Emission-line Galaxies. I. A Four-zone Ionization Model for Very High-ionization Emission
DOI: 10.3847/1538-4357/ac141b Bibcode: 2021ApJ...922..170B

Skillman, Evan D.; Chisholm, John; Erb, Dawn K. +3 more

Stellar population models produce radiation fields that ionize oxygen up to O+2, defining the limit of standard H II region models (<54.9 eV). Yet, some extreme emission-line galaxies, or EELGs, have surprisingly strong emission originating from much higher ionization potentials. We present UV HST/COS and optical LBT/MODS spectra of …

2021 The Astrophysical Journal
eHST 76
Dissecting the Local Environment of FRB 190608 in the Spiral Arm of its Host Galaxy
DOI: 10.3847/1538-4357/ac2818 Bibcode: 2021ApJ...922..173C

Chittidi, Jay S.; Simha, Sunil; Mannings, Alexandra +15 more

We present a high-resolution analysis of the host galaxy of fast radio burst (FRB) 190608, an SB(r)c galaxy at z = 0.11778 (hereafter HG 190608), to dissect its local environment and its contributions to the FRB properties. Our Hubble Space Telescope Wide Field Camera 3 ultraviolet and visible light image reveals that the subarcsecond localization…

2021 The Astrophysical Journal
Gaia eHST 76
Transit detection of the long-period volatile-rich super-Earth ν2 Lupi d with CHEOPS
DOI: 10.1038/s41550-021-01381-5 Bibcode: 2021NatAs...5..775D

Charnoz, Sébastien; Guedel, Manuel; Gandolfi, Davide +75 more

Exoplanets transiting bright nearby stars are key objects for advancing our knowledge of planetary formation and evolution. The wealth of photons from the host star gives detailed access to the atmospheric, interior and orbital properties of the planetary companions. ν2 Lupi (HD 136352) is a naked-eye (V = 5.78) Sun-like star that was d…

2021 Nature Astronomy
CHEOPS 76