Search Publications

Morphological and Spectral Diversity of the Clay-Bearing Unit at the ExoMars Landing Site Oxia Planum
DOI: 10.1089/ast.2020.2292 Bibcode: 2021AsBio..21..464M

Pan, Lu; Quantin-Nataf, Cathy; Cremonese, Gabriele +10 more

The European Space Agency and Roscosmos' ExoMars rover mission, which is planned to land in the Oxia Planum region, will be dedicated to exobiology studies at the surface and subsurface of Mars. Oxia Planum is a clay-bearing site that has preserved evidence of long-term interaction with water during the Noachian era. Fe/Mg-rich phyllosilicates hav…

2021 Astrobiology
ExoMars-16 MEx 40
The Low-redshift Lyman-continuum Survey: [S II] Deficiency and the Leakage of Ionizing Radiation
DOI: 10.3847/1538-4357/ac0434 Bibcode: 2021ApJ...916....3W

Giavalisco, Mauro; Grazian, Andrea; Henry, Alaina +19 more

The relationship between galaxy characteristics and the reionization of the universe remains elusive, mainly due to the observational difficulty in accessing the Lyman continuum (LyC) at these redshifts. It is thus important to identify low-redshift LyC-leaking galaxies that can be used as laboratories to investigate the physical processes that al…

2021 The Astrophysical Journal
eHST 40
The MOSDEF survey: a comprehensive analysis of the rest-optical emission-line properties of z ∼ 2.3 star-forming galaxies
DOI: 10.1093/mnras/stab119 Bibcode: 2021MNRAS.502.2600R

Barro, Guillermo; Siana, Brian; Shapley, Alice E. +16 more

We analyse the rest-optical emission-line spectra of z ~ 2.3 star-forming galaxies in the complete MOSFIRE Deep Evolution Field (MOSDEF) survey. In investigating the origin of the well-known offset between the sequences of high-redshift and local galaxies in the [O III]λ5008/Hβ versus [N II]λ6585/Hα ('[N II] BPT') diagram, we define two population…

2021 Monthly Notices of the Royal Astronomical Society
eHST 40
The 12CO/13CO isotopologue ratio of a young, isolated brown dwarf. Possibly distinct formation pathways of super-Jupiters and brown dwarfs
DOI: 10.1051/0004-6361/202141502 Bibcode: 2021A&A...656A..76Z

Zhang, Yapeng; Mollière, Paul; Snellen, Ignas A. G.

Context. Linking atmospheric characteristics of planets to their formation pathways is a central theme in the study of extrasolar planets. Although the 12C/13C isotope ratio shows little variation in the Solar System, the atmosphere of a super-Jupiter was recently shown to be rich in 13CO, possibly as a result of d…

2021 Astronomy and Astrophysics
Gaia 40
Haze evolution in temperate exoplanet atmospheres through surface energy measurements
DOI: 10.1038/s41550-021-01375-3 Bibcode: 2021NatAs...5..822Y

Fortney, Jonathan J.; Moran, Sarah E.; Valenti, Jeff A. +13 more

Photochemical hazes are important opacity sources in temperate exoplanet atmospheres, hindering current observations from characterizing exoplanet atmospheric compositions. The haziness of an atmosphere is determined by the balance between haze production and removal. However, the material-dependent removal physics of the haze particles are curren…

2021 Nature Astronomy
eHST 40
Stellar Surface Inhomogeneities as a Potential Source of the Atmospheric Signal Detected in the K2-18b Transmission Spectrum
DOI: 10.3847/1538-3881/ac2824 Bibcode: 2021AJ....162..300B

Kostov, Veselin B.; Barclay, Thomas; Schlieder, Joshua E. +5 more

Transmission spectroscopy of transiting exoplanets is a proven technique that can yield information on the composition and structure of a planet's atmosphere. However, transmission spectra may be compromised by inhomogeneities in the stellar photosphere. The sub-Neptune-sized habitable zone planet K2-18b has water absorption detected in its atmosp…

2021 The Astronomical Journal
eHST 40
Comprehensive Gas Characterization of a z = 2.5 Protocluster: A Cluster Core Caught in the Beginning of Virialization?
DOI: 10.3847/1538-4357/abf4e6 Bibcode: 2021ApJ...913..110C

Casey, Caitlin M.; Long, Arianna S.; Zavala, Jorge A. +6 more

In order to connect galaxy clusters to their progenitor protoclusters, we must constrain the star formation histories within their member galaxies and the timescale of virial collapse. In this paper we characterize the complex star-forming properties of a z = 2.5 protocluster in the COSMOS field using ALMA dust continuum and new Very Large Array C…

2021 The Astrophysical Journal
Herschel eHST 40
TESS survey of rotational and pulsational variability of mercury-manganese stars
DOI: 10.1093/mnras/stab2107 Bibcode: 2021MNRAS.506.5328K

Neiner, C.; Paunzen, E.; Kochukhov, O. +4 more

Mercury-manganese (HgMn) stars are late-B upper main sequence chemically peculiar stars distinguished by large overabundances of heavy elements, slow rotation, and frequent membership in close binary systems. These stars lack strong magnetic fields typical of magnetic Bp stars but occasionally exhibit non-uniform surface distributions of chemical …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 40
Detection of Galactic and Extragalactic Millimeter-wavelength Transient Sources with SPT-3G
DOI: 10.3847/1538-4357/ac06a3 Bibcode: 2021ApJ...916...98G

Ade, P. A. R.; Benabed, K.; Bouchet, F. R. +119 more

High angular resolution cosmic microwave background experiments provide a unique opportunity to conduct a survey of time-variable sources at millimeter wavelengths, a population that has primarily been understood through follow-up measurements of detections in other bands. Here we report the first results of an astronomical transient survey with t…

2021 The Astrophysical Journal
Gaia 40
The GOGREEN and GCLASS surveys: first data release
DOI: 10.1093/mnras/staa3008 Bibcode: 2021MNRAS.500..358B

Cooper, M. C.; Matharu, Jasleen; Muzzin, Adam +43 more

We present the first public data release of the GOGREEN (Gemini Observations of Galaxies in Rich Early Environments) and GCLASS (Gemini CLuster Astrophysics Spectroscopic Survey) surveys of galaxies in dense environments, spanning a redshift range 0.8 < z < 1.5. The surveys consist of deep, multiwavelength photometry and extensive Gemini GMO…

2021 Monthly Notices of the Royal Astronomical Society
eHST 40