Search Publications

Fast spectrophotometry of WD 1145+017
DOI: 10.1093/mnras/sty2315 Bibcode: 2018MNRAS.481..703I

Villaver, Eva; Raddi, Roberto; Gänsicke, Boris T. +16 more

WD 1145+017 is currently the only white dwarf known to exhibit periodic transits of planetary debris as well as absorption lines from circumstellar gas. We present the first simultaneous fast optical spectrophotometry and broad-band photometry of the system, obtained with the Gran Telescopio Canarias (GTC) and the Liverpool Telescope, respectively…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 32
SHARDS: constraints on the dust attenuation law of star-forming galaxies at z ∼ 2
DOI: 10.1093/mnras/stx3334 Bibcode: 2018MNRAS.475.2363T

Barro, Guillermo; Pérez-González, Pablo G.; Cava, Antonio +11 more

We make use of the Survey of High-z Absorption Red and Dead Sources, an ultradeep (<26.5AB) galaxy survey that provides optical photospectra at resolution R ∼ 50, via medium-band filters (FWHM ∼ 150 Å). This data set is combined with ancillary optical and NIR fluxes to constrain the dust attenuation law in the rest-frame NUV region of star-form…

2018 Monthly Notices of the Royal Astronomical Society
eHST 32
ALMA observation of the disruption of molecular gas in M87
DOI: 10.1093/mnras/sty047 Bibcode: 2018MNRAS.475.3004S

Simionescu, A.; Allen, S. W.; Werner, N. +3 more

We present the results from Atacama Large Millimeter Array (ALMA) observations centred 40 arcsec (3 kpc in projection) south-east of the nucleus of M87. We report the detection of extended CO (2-1) line emission with a total flux of (5.5 ± 0.6) × 10-18 erg s-1 cm-2 and corresponding molecular gas mass M_{H_2}=(4.7 …

2018 Monthly Notices of the Royal Astronomical Society
eHST 31
The radius of the quiescent neutron star in the globular cluster M13
DOI: 10.1093/mnras/sty582 Bibcode: 2018MNRAS.476.4713S

Campana, S.; Heinke, C. O.; Cohn, H. N. +5 more

X-ray spectra of quiescent low-mass X-ray binaries containing neutron stars can be fit with atmosphere models to constrain the mass and the radius. Mass-radius constraints can be used to place limits on the equation of state of dense matter. We perform fits to the X-ray spectrum of a quiescent neutron star in the globular cluster M13, utilizing da…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 31
The GALAH survey: accurate radial velocities and library of observed stellar template spectra
DOI: 10.1093/mnras/sty2293 Bibcode: 2018MNRAS.481..645Z

Ting, Yuan-Sen; Casey, Andrew R.; Buder, Sven +34 more

GALAH is a large-scale magnitude-limited southern stellar spectroscopic survey. Its second data release (GALAH DR2) provides values of stellar parameters and abundances of 23 elements for 342 682 stars (Buder et al.). Here we add a description of the public release of radial velocities with a typical accuracy of 0.1 km s-1 for 336 215 o…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 31
The very faint X-ray binary IGR J17062-6143: a truncated disc, no pulsations, and a possible outflow
DOI: 10.1093/mnras/stx3224 Bibcode: 2018MNRAS.475.2027V

Altamirano, D.; Degenaar, N.; Wijnands, R. +10 more

We present a comprehensive X-ray study of the neutron star low-mass X-ray binary IGR J17062-6143, which has been accreting at low luminosities since its discovery in 2006. Analysing NuSTAR, XMM-Newton, and Swift observations, we investigate the very faint nature of this source through three approaches: modelling the relativistic reflection spectru…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 31
Multiwavelength observations of V407 Lupi (ASASSN-16kt) - a very fast nova erupting in an intermediate polar
DOI: 10.1093/mnras/sty1759 Bibcode: 2018MNRAS.480..572A

Ness, J. -U.; Henze, M.; Kniazev, A. +19 more

We present a detailed study of the 2016 eruption of nova V407 Lupi (ASASSN-16kt), including optical, near-infrared, X-ray, and ultraviolet data from SALT, SMARTS, SOAR, Chandra, Swift, and XMM-Newton. Timing analysis of the multiwavelength light curves shows that, from 168 d post-eruption and for the duration of the X-ray supersoft source phase, t…

2018 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 31
High-precision multiwavelength eclipse photometry of the ultra-hot gas giant exoplanet WASP-103 b
DOI: 10.1093/mnras/stx2896 Bibcode: 2018MNRAS.474.2334D

Bouchy, F.; Magain, P.; Queloz, D. +14 more

We present 16 occultation and three transit light curves for the ultra-short period hot Jupiter WASP-103b, in addition to five new radial velocity measurements. We combine these observations with archival data and perform a global analysis of the resulting extensive data set, accounting for the contamination from a nearby star. We detect the therm…

2018 Monthly Notices of the Royal Astronomical Society
eHST 31
SEAGLE - I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
DOI: 10.1093/mnras/sty1741 Bibcode: 2018MNRAS.479.4108M

Crain, Robert A.; Schaye, Joop; Theuns, Tom +8 more

In this paper we introduce the SEAGLE (i.e. Simulating EAGLE LEnses) programme, which approaches the study of galaxy formation through strong gravitational lensing, using a suite of high-resolution hydrodynamic simulations, Evolution and Assembly of GaLaxies and their Environments (EAGLE) project. We introduce the simulation and analysis pipeline …

2018 Monthly Notices of the Royal Astronomical Society
eHST 30
Prevalence of neutral gas in centres of merging galaxies
DOI: 10.1093/mnras/sty1872 Bibcode: 2018MNRAS.480..947D

Srianand, R.; Gupta, N.; Dutta, R.

We present Giant Metrewave Radio Telescope and Very Large Array observations of H I 21-cm absorption in 10 z ≤ 0.2 galaxy mergers that host strong radio sources. Seven of these mergers show strong absorption [with N({H I}) ∼ 1021 - 22 cm-2, for spin temperature of 100 K and unit covering factor]. Including literature sources,…

2018 Monthly Notices of the Royal Astronomical Society
eHST 30