Search Publications

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
Current Sheets, Plasmoids and Flux Ropes in the Heliosphere. Part I. 2-D or not 2-D? General and Observational Aspects
DOI: 10.1007/s11214-021-00814-x Bibcode: 2021SSRv..217...38K

Li, Gang; Bruno, R.; Malandraki, O. +13 more

Recent accumulation of a critical mass of observational material from different spacecraft complete with the enhanced abilities of numerical methods have led to a boom of studies revealing the high complexity of processes occurring in the heliosphere. Views on the solar wind filling the interplanetary medium have dramatically developed from the be…

2021 Space Science Reviews
Ulysses 40
The Galactic center chimneys: the base of the multiphase outflow of the Milky Way
DOI: 10.1051/0004-6361/202039636 Bibcode: 2021A&A...646A..66P

Churazov, E.; Ponti, G.; Heywood, I. +2 more

Context. Outflows and feedback are key ingredients of galaxy evolution. Evidence for an outflow arising from the Galactic center (GC) - the so-called GC chimneys - has recently been discovered at radio, infrared, and X-ray bands.
Aims: We undertake a detailed examination of the spatial relationships between the emission in the different bands…

2021 Astronomy and Astrophysics
Herschel XMM-Newton 40
Birth of the ELMs: a ZTF survey for evolved cataclysmic variables turning into extremely low-mass white dwarfs
DOI: 10.1093/mnras/stab2583 Bibcode: 2021MNRAS.508.4106E

Rix, Hans-Walter; El-Badry, Kareem; Kupfer, Thomas +2 more

We present a systematic survey for mass-transferring and recently detached cataclysmic variables (CVs) with evolved secondaries, which are progenitors of extremely low mass white dwarfs (ELM WDs), AM CVn systems, and detached ultracompact binaries. We select targets below the main sequence in the Gaia colour-magnitude diagram with ZTF light curves…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 40
Iron in X-COP: Tracing enrichment in cluster outskirts with high accuracy abundance profiles
DOI: 10.1051/0004-6361/202038501 Bibcode: 2021A&A...646A..92G

Gastaldello, Fabio; Ettori, Stefano; Bartalucci, Iacopo +11 more

We present the first metal abundance profiles for a representative sample of massive clusters. Our measurements extend to R500 and are corrected for a systematic error plaguing previous outskirt estimates. Our profiles flatten out at large radii, admittedly not a new result, however the radial range and representative nature of our samp…

2021 Astronomy and Astrophysics
XMM-Newton 40