Search Publications

Old and young stellar populations in DustPedia galaxies and their role in dust heating
DOI: 10.1051/0004-6361/201935118 Bibcode: 2019A&A...624A..80N

Bianchi, S.; Fritz, J.; Madden, S. C. +19 more


Aims: Within the framework of the DustPedia project we investigate the properties of cosmic dust and its interaction with stellar radiation (originating from different stellar populations) for 814 galaxies in the nearby Universe, all observed by the Herschel Space Observatory.
Methods: We take advantage of the widely used fitting code CI…

2019 Astronomy and Astrophysics
Herschel 108
The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars
DOI: 10.3847/1538-4357/ab3c1a Bibcode: 2019ApJ...883...76R

Green, Paul J.; Anderson, Scott F.; Eracleous, Michael +5 more

Despite their factor of ∼108 difference in black hole mass, several lines of evidence suggest possible similarities between black hole accretion flows in active galactic nuclei (AGN) and Galactic X-ray binaries. However, it is still unclear whether the geometry of the disk-corona system in X-ray binaries directly scales up to AGN and wh…

2019 The Astrophysical Journal
XMM-Newton 108
Reclassification of Cepheids in the Gaia Data Release 2. Period-luminosity and period-Wesenheit relations in the Gaia passbands
DOI: 10.1051/0004-6361/201834506 Bibcode: 2019A&A...625A..14R

Ripepi, V.; Molinaro, R.; Eyer, L. +3 more

Context. Classical Cepheids are the most important primary indicators for the extragalactic distance scale. Establishing the precise zero points of their period-luminosity and period-Wesenheit (PL/PW) relations has profound consequences on the estimate of H0. Type II Cepheids are also important distance indicators and tracers of old ste…

2019 Astronomy and Astrophysics
Gaia INTEGRAL 108
Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the “Planetary” Mass Regime
DOI: 10.3847/1538-4365/aaf6af Bibcode: 2019ApJS..240...19K

Cushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R. +16 more

We present preliminary trigonometric parallaxes of 184 late-T and Y dwarfs using observations from Spitzer (143), the U.S. Naval Observatory (18), the New Technology Telescope (14), and the United Kingdom Infrared Telescope (9). To complete the 20 pc census of ≥T6 dwarfs, we combine these measurements with previously published trigonometric parall…

2019 The Astrophysical Journal Supplement Series
Gaia 107
An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: source catalogue and properties
DOI: 10.1093/mnras/stz1536 Bibcode: 2019MNRAS.487.4648S

Thomson, A. P.; Ivison, R. J.; Kocevski, Dale D. +26 more

We present the catalogue and basic properties of sources in AS2UDS, an 870-µm continuum survey with the Atacama Large Millimetre/sub-millimetre Array (ALMA) of 716 single-dish sub-millimetre sources detected in the UKIDSS/UDS field by the SCUBA-2 Cosmology Legacy Survey. In our sensitive ALMA follow-up observations, we detect 708 sub-millime…

2019 Monthly Notices of the Royal Astronomical Society
Herschel eHST 107
Machine Learning for the Zwicky Transient Facility
DOI: 10.1088/1538-3873/aaf3fa Bibcode: 2019PASP..131c8002M

Duev, Dmitry A.; Riddle, Reed; Saunders, Nicholas +47 more

The Zwicky Transient Facility is a large optical survey in multiple filters producing hundreds of thousands of transient alerts per night. We describe here various machine learning (ML) implementations and plans to make the maximal use of the large data set by taking advantage of the temporal nature of the data, and further combining it with other…

2019 Publications of the Astronomical Society of the Pacific
Gaia 107
The Nucleus of comet 67P/Churyumov-Gerasimenko - Part I: The global view - nucleus mass, mass-loss, porosity, and implications
DOI: 10.1093/mnras/sty3171 Bibcode: 2019MNRAS.483.2337P

Tellmann, Silvia; Pätzold, Martin; Häusler, Bernd +7 more

The radio science experiment RSI on-board Rosetta determined the mass of the nucleus of comet 67P/Churyumov-Gerasimenko at the start of the prime mission from 2014 August to November (GM = 666.2 ± 0.2 m3 s-2 or 9982 ± 3 × 1012 kg) and shortly before the end of the mission from 2016 July to September (GM …

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 107
Resolving the Metallicity Distribution of the Stellar Halo with the H3 Survey
DOI: 10.3847/1538-4357/ab5710 Bibcode: 2019ApJ...887..237C

Conroy, Charlie; Johnson, Benjamin D.; Caldwell, Nelson +4 more

The Galactic stellar halo is predicted to have formed at least partially from the tidal disruption of accreted dwarf galaxies. This assembly history should be detectable in the orbital and chemical properties of stars. The H3 Survey is obtaining spectra for 200,000 stars and, when combined with Gaia data, is providing detailed orbital and chemical…

2019 The Astrophysical Journal
Gaia 107
The Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field
DOI: 10.3847/1538-4357/ab3792 Bibcode: 2019ApJ...883...99S

Franx, Marijn; Illingworth, Garth D.; Muzzin, Adam +12 more

We present 16 new ultrabright H AB ≲ 25 galaxy candidates at z ∼ 8 identified over the COSMOS/UltraVISTA field. The new search takes advantage of the deepest-available ground-based optical and near-infrared observations, including the DR3 release of UltraVISTA and full-depth Spitzer/IRAC observations from the SMUVS and SPLASH programs…

2019 The Astrophysical Journal
eHST 107
Low-mass halo perturbations in strong gravitational lenses at redshift z ∼ 0.5 are consistent with CDM
DOI: 10.1093/mnras/stz464 Bibcode: 2019MNRAS.485.2179R

Vegetti, S.; McKean, J. P.; Auger, M. W. +3 more

We use a sample of 17 strong gravitational lens systems from the BELLS GALLERY survey to quantify the amount of low-mass dark matter haloes within the lensing galaxies and along their lines of sight, and to constrain the properties of dark matter. Based on a detection criterion of 10σ, we report no significant detection in any of the lenses. Using…

2019 Monthly Notices of the Royal Astronomical Society
eHST 107