Search Publications

Design and Operation of the ATLAS Transient Science Server
DOI: 10.1088/1538-3873/ab936e Bibcode: 2020PASP..132h5002S

Rest, A.; Smartt, S. J.; Stalder, B. +19 more

The Asteroid Terrestrial impact Last Alert System (ATLAS) system consists of two 0.5 m Schmidt telescopes with cameras covering 29 square degrees at plate scale of 1.86 arcsec per pixel. Working in tandem, the telescopes routinely survey the whole sky visible from Hawaii (above $\delta \gt -50^\circ $ ) every two nights, exposing four times per ni…

2020 Publications of the Astronomical Society of the Pacific
Gaia 275
Universal bolometric corrections for active galactic nuclei over seven luminosity decades
DOI: 10.1051/0004-6361/201936817 Bibcode: 2020A&A...636A..73D

Maiolino, R.; Fiore, F.; Bianchi, S. +12 more

Context. The AGN bolometric correction is a key element for understanding black hole (BH) demographics and computing accurate BH accretion histories from AGN luminosities. However, current estimates still differ from each other by up to a factor of two to three, and rely on extrapolations at the lowest and highest luminosities.
Aims: Here we …

2020 Astronomy and Astrophysics
ISO 264
The biggest splash
DOI: 10.1093/mnras/staa876 Bibcode: 2020MNRAS.494.3880B

Grand, Robert J. J.; Fattahi, Azadeh; Belokurov, Vasily +4 more

Using a large sample of bright nearby stars with accurate Gaia Data Release 2 astrometry and auxiliary spectroscopy we map out the properties of the principle Galactic components such as the 'thin' and 'thick' discs and the halo. We confirm previous claims that in the Solar neighbourhood, there exists a large population of metal-rich ([Fe/H] > …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 260
On the Spectral Evolution of Hot White Dwarf Stars. I. A Detailed Model Atmosphere Analysis of Hot White Dwarfs from SDSS DR12
DOI: 10.3847/1538-4357/abafbe Bibcode: 2020ApJ...901...93B

Fontaine, G.; Bergeron, P.; Bédard, A. +1 more

As they evolve, white dwarfs undergo major changes in surface composition, a phenomenon known as spectral evolution. In particular, some stars enter the cooling sequence with helium atmospheres (type DO) but eventually develop hydrogen atmospheres (type DA), most likely through the upward diffusion of residual hydrogen. Our empirical knowledge of …

2020 The Astrophysical Journal
Gaia 256
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