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The Volume-complete Sample of M Dwarfs with Masses 0.1 ≤ M/M ≤ 0.3 within 15 Parsecs
DOI: 10.3847/1538-3881/abcc74 Bibcode: 2021AJ....161...63W

Henry, Todd J.; Winters, Jennifer G.; Irwin, Jonathan M. +4 more

M dwarfs with masses 0.1 ≤ M/M ≤ 0.3 are under increasing scrutiny because these fully convective stars pose interesting astrophysical questions regarding their magnetic activity and angular momentum history. They also afford the most accessible near future opportunity to study the atmospheres of terrestrial planets. Because they are i…

2021 The Astronomical Journal
Gaia 37
Chromospheric Heating by Magnetohydrodynamic Waves and Instabilities
DOI: 10.1029/2020JA029097 Bibcode: 2021JGRA..12629097S

Srivastava, A. K.; Murawski, K.; Cally, P. S. +7 more

The importance of the chromosphere in the mass and energy transport within the solar atmosphere is now widely recognized. This review discusses the physics of magnetohydrodynamic waves and instabilities in large-scale chromospheric structures as well as in magnetic flux tubes. We highlight a number of key observational aspects that have helped our…

2021 Journal of Geophysical Research (Space Physics)
IRIS 37
Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field
DOI: 10.1051/0004-6361/202140612 Bibcode: 2021A&A...654A.121P

Dole, H.; Lagache, G.; Montier, L. +10 more

The Planck satellite has identified more than 2000 protocluster candidates with extreme star formation rates (SFRs). Here, we present the spectroscopic identification of a Planck-selected protocluster located in the Cosmos field, PHz G237.01+42.50. PHz G237.01+42.50 contains a galaxy overdensity of 31 spectroscopically identified galaxies at z ≃ 2…

2021 Astronomy and Astrophysics
Herschel XMM-Newton eHST 37
Evidence for disequilibrium chemistry from vertical mixing in hot Jupiter atmospheres. A comprehensive survey of transiting close-in gas giant exoplanets with warm-Spitzer/IRAC
DOI: 10.1051/0004-6361/202039708 Bibcode: 2021A&A...648A.127B

Deming, Drake; Burrows, Adam; Fortney, Jonathan J. +10 more


Aims: We present a large atmospheric study of 49 gas giant exoplanets using infrared transmission photometry with Spitzer/IRAC at 3.6 and 4.5 µm.
Methods: We uniformly analyze 70 photometric light curves of 33 transiting planets using our custom pipeline, which implements pixel level decorrelation. Augmenting our sample with 16 pre…

2021 Astronomy and Astrophysics
Gaia IUE 37
Gyro-kinematic Ages for around 30,000 Kepler Stars
DOI: 10.3847/1538-3881/abe4d6 Bibcode: 2021AJ....161..189L

Angus, Ruth; Kiman, Rocio; Curtis, Jason L. +2 more

Estimating stellar ages is important for advancing our understanding of stellar and exoplanet evolution and investigating the history of the Milky Way. However, ages for low-mass stars are hard to infer as they evolve slowly on the main sequence. In addition, empirical dating methods are difficult to calibrate for low-mass stars as they are faint.…

2021 The Astronomical Journal
Gaia 37
Fitting spectral energy distributions of FMOS-COSMOS emission-line galaxies at z ∼ 1.6: Star formation rates, dust attenuation, and [OIII]λ5007 emission-line luminosities
DOI: 10.1051/0004-6361/202140890 Bibcode: 2021A&A...654A.153V

Buat, V.; Boquien, M.; Burgarella, D. +2 more

We perform a spectral energy distribution fitting analysis on a COSMOS photometric sample covering the ultra-violet up to the far-infrared wavelengths and including emission lines from the Fiber Multi-Object Spectrograph survey. The sample consists of 182 objects with Hα and [OIII]λ5007 emission line measurements lying in a redshift range of 1.40 …

2021 Astronomy and Astrophysics
Herschel 37
Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster?
DOI: 10.1051/0004-6361/202039650 Bibcode: 2021A&A...646A..63V

Mamon, Gary A.; Vitral, Eduardo

We analyze proper motions from the Hubble Space Telescope (HST) and the second Gaia data release along with line-of-sight velocities from the MUSE spectrograph to detect imprints of an intermediate-mass black hole (IMBH) in the center of the nearby, core-collapsed, globular cluster NGC 6397. For this, we use the new MAMPOSST-PM Bayesian mass-model…

2021 Astronomy and Astrophysics
Gaia eHST 37
Direct imaging of sub-Jupiter mass exoplanets with James Webb Space Telescope coronagraphy
DOI: 10.1093/mnras/staa3579 Bibcode: 2021MNRAS.501.1999C

Carter, Aarynn L.; Hinkley, Sasha; Pueyo, Laurent +7 more

The James Webb Space Telescope (JWST), currently scheduled to launch in 2021, will dramatically advance our understanding of exoplanetary systems with its ability to directly image and characterize planetary-mass companions at wide separations through coronagraphy. Using state-of-the-art simulations of JWST performance, in combination with the lat…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 37
Populating the brown dwarf and stellar boundary: Five stars with transiting companions near the hydrogen-burning mass limit
DOI: 10.1051/0004-6361/202141145 Bibcode: 2021A&A...652A.127G

Henning, Thomas; Triaud, Amaury H. M. J.; Latham, David W. +53 more

We report the discovery of five transiting companions near the hydrogen-burning mass limit in close orbits around main sequence stars originally identified by the Transiting Exoplanet Survey Satellite (TESS) as TESS objects of interest (TOIs): TOI-148, TOI-587, TOI-681, TOI-746, and TOI-1213. Using TESS and ground-based photometry as well as radia…

2021 Astronomy and Astrophysics
Gaia 37
The ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field
DOI: 10.1051/0004-6361/202140310 Bibcode: 2021A&A...649A..22M

Elbaz, D.; Castellano, M.; Pentericci, L. +17 more

Context. We present ASTRODEEP-GS43, a new multi-wavelength photometric catalogue of the GOODS-South field, which builds and improves upon the previously released CANDELS catalogue.
Aims: We provide photometric fluxes and corresponding uncertainties in 43 optical and infrared bands (25 wide and 18 medium filters), as well as the photometric re…

2021 Astronomy and Astrophysics
eHST 37