Search Publications

Distances and parallax bias in Gaia DR2
DOI: 10.1093/mnras/stz1451 Bibcode: 2019MNRAS.487.3568S

Schönrich, Ralph; Eyer, Laurent; McMillan, Paul

We derive Bayesian distances for all stars in the radial velocity sample of Gaia DR2, and use the statistical method of Schönrich, Binney & Asplund to validate the distances and test the Gaia parallaxes. In contrast to other methods, which rely on special sources, our method directly tests the distances to all stars in our sample. We find clea…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 140
The discovery of weak coherent pulsations in the ultraluminous X-ray source NGC 1313 X-2
DOI: 10.1093/mnrasl/slz086 Bibcode: 2019MNRAS.488L..35S

Fabian, A. C.; Pinto, C.; Bachetti, M. +8 more

We report the detection of weak pulsations from the archetypal ultraluminous X-ray source (ULX) NGC 1313 X-2. Acceleration searches reveal sinusoidal pulsations in segments of two out of six new deep observations of this object, with a period of ∼1.5 s and a pulsed fraction of ∼ 5 per cent. We use Monte Carlo simulations to demonstrate that the in…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 135
Evolution of the galaxy stellar mass functions and UV luminosity functions at z = 6-9 in the Hubble Frontier Fields
DOI: 10.1093/mnras/stz866 Bibcode: 2019MNRAS.486.3805B

Conselice, Christopher J.; Bhatawdekar, Rachana; Duncan, Kenneth +1 more

We present new measurements of the evolution of the galaxy stellar mass functions (GSMFs) and ultraviolet luminosity functions (UV LFs) for galaxies from z = 6-9 within the Frontier Field cluster MACSJ0416.1-2403 and its parallel field. To obtain these results, we derive the stellar masses of our sample by fitting synthetic stellar population mode…

2019 Monthly Notices of the Royal Astronomical Society
eHST 135
A distance of 13 Mpc resolves the claimed anomalies of the galaxy lacking dark matter
DOI: 10.1093/mnras/stz771 Bibcode: 2019MNRAS.486.1192T

Beasley, Michael A.; Borlaff, Alejandro; Vazdekis, Alexandre +10 more

The claimed detection of a diffuse galaxy lacking dark matter represents a possible challenge to our understanding of the properties of these galaxies and galaxy formation in general. The galaxy, already identified in photographic plates taken in the summer of 1976 at the UK 48-in Schmidt telescope, presents normal distance-independent properties …

2019 Monthly Notices of the Royal Astronomical Society
eHST 134
On the dust temperatures of high-redshift galaxies
DOI: 10.1093/mnras/stz2134 Bibcode: 2019MNRAS.489.1397L

Faucher-Giguère, Claude-André; Hayward, Christopher C.; Hopkins, Philip F. +7 more

Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is required when converting (sub)millimetre broad-band flux to total infrared luminosity (LIR), and hence star formation rate, in high-redshift galaxies. However, different definitions of dust temperatures have been used in the literature, leading…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 130
Is the dark-matter halo spin a predictor of galaxy spin and size?
DOI: 10.1093/mnras/stz1952 Bibcode: 2019MNRAS.488.4801J

Somerville, Rachel S.; Genel, Shy; Dekel, Avishai +8 more

The similarity between the distributions of spins for galaxies (λgal) and for dark-matter haloes (λhalo), indicated both by simulations and observations, is naively interpreted as a one-to-one correlation between the spins of a galaxy and its host halo. This is used to predict galaxy sizes in semi-analytic models via Re<…

2019 Monthly Notices of the Royal Astronomical Society
eHST 130
Evidence for rapid disc formation and reprocessing in the X-ray bright tidal disruption event candidate AT 2018fyk
DOI: 10.1093/mnras/stz1976 Bibcode: 2019MNRAS.488.4816W

Gromadzki, M.; Hodgkin, S. T.; Kostrzewa-Rutkowska, Z. +15 more

We present optical spectroscopic and Swift UVOT/XRT observations of the X-ray and UV/optical bright tidal disruption event (TDE) candidate AT 2018fyk/ASASSN-18ul discovered by ASAS-SN. The Swift light curve is atypical for a TDE, entering a plateau after ∼40 d of decline from peak. After 80 d the UV/optical light curve breaks again to decline furt…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 128
NIHAO XV: the environmental impact of the host galaxy on galactic satellite and field dwarf galaxies
DOI: 10.1093/mnras/sty2913 Bibcode: 2019MNRAS.483.1314B

Buck, Tobias; Dutton, Aaron A.; Macciò, Andrea V. +2 more

We study the impact of the host on dwarf galaxy properties using four new Milky Way (MW)-like, ultra-high-resolution simulations (Npart > 107) from the NIHAO project. We split our sample into satellite (R < R200), nearby (1 < R/R200 < 2.5), and field (R > 2.5R200) galaxies. Simu…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 126
The total stellar halo mass of the Milky Way
DOI: 10.1093/mnras/stz2793 Bibcode: 2019MNRAS.490.3426D

Belokurov, Vasily; Sanders, Jason L.; Deason, Alis J.

We measure the total stellar halo luminosity using red giant branch (RGB) stars selected from Gaia data release 2. Using slices in magnitude, colour, and location on the sky, we decompose RGB stars belonging to the disc and halo by fitting two-dimensional Gaussians to the Galactic proper motion distributions. The number counts of RGB stars are con…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 125
Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients
DOI: 10.1093/mnras/stz438 Bibcode: 2019MNRAS.485.2642G

Maccarone, Thomas J.; Gandhi, Poshak; Rao, Anjali +2 more

We report on a first census of Galactic black hole X-ray binary (BHXRB) properties with the second data release (DR2) of Gaia, focusing on dynamically confirmed and strong candidate BH transients. Gaia DR2 provides five-parameter astrometric solutions including position, parallax and proper motion for 11 out of a sample of 24 systems. Distance est…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 124