Search Publications

On the UV compactness and morphologies of typical Lyman α emitters from z ∼ 2 to z ∼ 6
DOI: 10.1093/mnras/sty281 Bibcode: 2018MNRAS.476.5479P

Sobral, David; Matthee, Jorryt; Paulino-Afonso, Ana +8 more

We investigate the rest-frame UV morphologies of a large sample of Lyman α emitters (LAEs) from z ∼ 2 to z ∼ 6, selected in a uniform way with 16 different narrow and medium bands over the full COSMOS field. We use 3045 LAEs with Hubble Space Telescope coverage in a stacking analysis and find that they have MUV ∼ -20, below M_UV^\ast at…

2018 Monthly Notices of the Royal Astronomical Society
eHST 54
Gaia reveals evidence for merged white dwarfs
DOI: 10.1093/mnrasl/sly110 Bibcode: 2018MNRAS.479L.113K

Hambly, N. C.; Rowell, N.; Genest-Beaulieu, C. +2 more

We use Gaia Data Release 2 to identify 13 928 white dwarfs (WDs) within 100 pc of the Sun. The exquisite astrometry from Gaia reveals for the first time a bifurcation in the observed WD sequence in both Gaia and the Sloan Digital Sky Survey (SDSS) passbands. The latter is easily explained by a helium atmosphere WD fraction of 36 per cent. However,…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 54
The dusty progenitor star of the Type II supernova 2017eaw
DOI: 10.1093/mnras/sty2435 Bibcode: 2018MNRAS.481.2536K

Kilpatrick, Charles D.; Foley, Ryan J.

We present pre-explosion photometry of the likely progenitor star of the Type II supernova (SN II) 2017eaw in NGC 6946. We use a Hubble Space Telescope (HST) image of SN 2017eaw to perform relative astrometry with HST and Spitzer Space Telescope (Spitzer) imaging, finding a single point source consistent with its position. We detect the progenitor…

2018 Monthly Notices of the Royal Astronomical Society
eHST 54
Venus Interior Structure and Dynamics
DOI: 10.1007/s11214-018-0518-1 Bibcode: 2018SSRv..214...88S

Sotin, Christophe; Smrekar, Suzanne E.; Davaille, Anne

No two rocky bodies offer a better laboratory for exploring the conditions controlling interior dynamics than Venus and Earth. Their similarities in size, density, distance from the sun, and young surfaces would suggest comparable interior dynamics. Although the two planets exhibit some of the same processes, Venus lacks Earth's dominant process f…

2018 Space Science Reviews
VenusExpress 54
The XUV environments of exoplanets from Jupiter-size to super-Earth
DOI: 10.1093/mnras/sty1110 Bibcode: 2018MNRAS.478.1193K

Kirk, James; Wheatley, Peter J.; Louden, Tom +8 more

Planets that reside close-in to their host star are subject to intense high-energy irradiation. Extreme-ultraviolet (EUV) and X-ray radiation (together, XUV) is thought to drive mass-loss from planets with volatile envelopes. We present XMM-Newton observations of six nearby stars hosting transiting planets in tight orbits (with orbital period, P

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 54
StarGO: A New Method to Identify the Galactic Origins of Halo Stars
DOI: 10.3847/1538-4357/aacd0d Bibcode: 2018ApJ...863...26Y

Kang, Xi; Chang, Jiang; Han, Jiaxin +3 more

We develop a new method, Stars’ Galactic Origin (StarGO), to identify the galactic origins of halo stars using their kinematics. Our method is based on a self-organizing map (SOM), which is one of the most popular unsupervised learning algorithms. STARGO combines SOM with a novel adaptive group identification algorithm with essentially no free par…

2018 The Astrophysical Journal
Gaia 54
Analysis of the SFR-M plane at z < 3: single fitting versus multi-Gaussian decomposition
DOI: 10.1051/0004-6361/201731399 Bibcode: 2018A&A...609A..82B

Koekemoer, A.; Caputi, K. I.; Bisigello, L. +1 more

The analysis of galaxies on the star formation rate-stellar mass (SFR-M) plane is a powerful diagnostic for galaxy evolution at different cosmic times. We consider a sample of 24 463 galaxies from the CANDELS/GOODS-S survey to conduct a detailed analysis of the SFR-M relation at redshifts re than three dex in stellar mass. …

2018 Astronomy and Astrophysics
Herschel eHST 53
Bending waves in the Milky Way's disc from halo substructure
DOI: 10.1093/mnras/sty2114 Bibcode: 2018MNRAS.480.4244C

Widrow, Lawrence M.; Chequers, Matthew H.; Darling, Keir

We use N-body simulations to investigate the excitation of bending waves in a Milky Way-like disc-bulge-halo system. The dark matter halo consists of a smooth component and a population of subhaloes, while the disc is composed of thin and thick components. Also, considered is a control simulation where all of the halo mass is smoothly distributed.…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 53
Galaxy and Quasar Fueling Caught in the Act from the Intragroup to the Interstellar Medium
DOI: 10.3847/2041-8213/aaf1cf Bibcode: 2018ApJ...869L...1J

Bouché, Nicolas; Marino, Raffaella A.; Maseda, Michael V. +11 more

We report the discovery of six spatially extended (10-100 kpc) line-emitting nebulae in the z ≈ 0.57 galaxy group hosting PKS 0405-123, one of the most luminous quasars at z < 1. The discovery is enabled by the Multi Unit Spectroscopic Explorer and provides tantalizing evidence connecting large-scale gas streams with nuclear activity on scales …

2018 The Astrophysical Journal
eHST 53
A Gaia DR2 Mock Stellar Catalog
DOI: 10.1088/1538-3873/aabd70 Bibcode: 2018PASP..130g4101R

Rix, Hans-Walter; Fouesneau, Morgan; Andrae, René +3 more

We present a mock catalog of Milky Way stars, matching in volume and depth the content of the Gaia data release 2 (GDR2). We generated our catalog using Galaxia, a tool to sample stars from a Besançon Galactic model, together with a realistic 3D dust extinction map. The catalog mimics the complete GDR2 data model and contains most of the entries i…

2018 Publications of the Astronomical Society of the Pacific
Gaia 53