Search Publications

The Fourth Fermi-GBM Gamma-Ray Burst Catalog: A Decade of Data
DOI: 10.3847/1538-4357/ab7a18 Bibcode: 2020ApJ...893...46V

Meegan, C. A.; von Kienlin, A.; Kocevski, D. +18 more

We present the fourth in a series of catalogs of gamma-ray bursts (GRBs) observed with Fermi's Gamma-ray Burst Monitor (Fermi-GBM). It extends the six year catalog by four more years, now covering the 10 year time period from trigger enabling on 2008 July 12 to 2018 July 11. During this time period GBM triggered almost twice a day on transient eve…

2020 The Astrophysical Journal
INTEGRAL 255
The lifecycle of molecular clouds in nearby star-forming disc galaxies
DOI: 10.1093/mnras/stz3525 Bibcode: 2020MNRAS.493.2872C

Henshaw, Jonathan D.; Kruijssen, J. M. Diederik; Longmore, Steven N. +29 more

It remains a major challenge to derive a theory of cloud-scale (≲100 pc) star formation and feedback, describing how galaxies convert gas into stars as a function of the galactic environment. Progress has been hampered by a lack of robust empirical constraints on the giant molecular cloud (GMC) lifecycle. We address this problem by systematically …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 254
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. II. A Statistical Characterization of Class 0 and Class I Protostellar Disks
DOI: 10.3847/1538-4357/ab6f64 Bibcode: 2020ApJ...890..130T

Kounkel, Marina; Kratter, Kaitlin; Dunham, Michael M. +33 more

We have conducted a survey of 328 protostars in the Orion molecular clouds with the Atacama Large Millimeter/submillimeter Array at 0.87 mm at a resolution of ∼0"1 (40 au), including observations with the Very Large Array at 9 mm toward 148 protostars at a resolution of ∼0"08 (32 au). This is the largest multiwavelength survey of protostars at thi…

2020 The Astrophysical Journal
Gaia 248
Nightside condensation of iron in an ultrahot giant exoplanet
DOI: 10.1038/s41586-020-2107-1 Bibcode: 2020Natur.580..597E

Martins, C. J. A. P.; Lendl, Monika; Udry, Stéphane +94 more

Ultrahot giant exoplanets receive thousands of times Earth's insolation1,2. Their high-temperature atmospheres (greater than 2,000 kelvin) are ideal laboratories for studying extreme planetary climates and chemistry3-5. Daysides are predicted to be cloud-free, dominated by atomic species6 and much hotter than night…

2020 Nature
Gaia 245
Clusters and mirages: cataloguing stellar aggregates in the Milky Way
DOI: 10.1051/0004-6361/201936691 Bibcode: 2020A&A...633A..99C

Anders, F.; Cantat-Gaudin, T.

Context. Many of the open clusters listed in modern catalogues were initially reported by visual astronomers as apparent overdensities of bright stars. As observational techniques and analysis methods continue to improve, some of them have been shown to be chance alignments of stars and not true clusters. Recent publications making use of Gaia DR2…

2020 Astronomy and Astrophysics
Gaia 243
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies
DOI: 10.1093/mnras/staa769 Bibcode: 2020MNRAS.494.3828D

Thomson, A. P.; Ivison, R. J.; Scott, D. +27 more

We analyse the physical properties of a large, homogeneously selected sample of ALMA-located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across the ∼1 deg2 field, including ∼17 per cent, which are undetected at K ≳ 25.7 mag. We interpret their ultraviolet-to-radio data using magphys and determine a median re…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 232
The Gaia-Kepler Stellar Properties Catalog. I. Homogeneous Fundamental Properties for 186,301 Kepler Stars
DOI: 10.3847/1538-3881/159/6/280 Bibcode: 2020AJ....159..280B

van Saders, Jennifer L.; Huber, Daniel; Berger, Travis A. +3 more

An accurate and precise Kepler Stellar Properties Catalog is essential for the interpretation of the Kepler exoplanet survey results. Previous Kepler Stellar Properties Catalogs have focused on reporting the best-available parameters for each star, but this has required combining data from a variety of heterogeneous sources. We present the Gaia-Ke…

2020 The Astronomical Journal
Gaia 232
Kraken reveals itself - the merger history of the Milky Way reconstructed with the E-MOSAICS simulations
DOI: 10.1093/mnras/staa2452 Bibcode: 2020MNRAS.498.2472K

Kruijssen, J. M. Diederik; Chevance, Mélanie; Bonaca, Ana +6 more

Globular clusters (GCs) formed when the Milky Way experienced a phase of rapid assembly. We use the wealth of information contained in the Galactic GC population to quantify the properties of the satellite galaxies from which the Milky Way assembled. To achieve this, we train an artificial neural network on the E-MOSAICS cosmological simulations o…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 228
The Zwicky Transient Facility Catalog of Periodic Variable Stars
DOI: 10.3847/1538-4365/ab9cae Bibcode: 2020ApJS..249...18C

Tian, Hao; Yang, Ming; Wang, Shu +3 more

The number of known periodic variables has grown rapidly in recent years. Thanks to its large field of view and faint limiting magnitude, the Zwicky Transient Facility (ZTF) offers a unique opportunity to detect variable stars in the northern sky. Here, we exploit ZTF Data Release 2 (DR2) to search for and classify variables down to r ∼ 20.6 mag. …

2020 The Astrophysical Journal Supplement Series
Gaia 228
A new set of atmosphere and evolution models for cool T-Y brown dwarfs and giant exoplanets
DOI: 10.1051/0004-6361/201937381 Bibcode: 2020A&A...637A..38P

Tremblin, P.; Allard, N. F.; Baraffe, I. +6 more

We present a new set of solar metallicity atmosphere and evolutionary models for very cool brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere models are generated with our state-of-the-art 1D radiative-convective equilibrium code ATMO, and are used as surface boundary conditions to calculate the interior structure…

2020 Astronomy and Astrophysics
eHST 228