Journal: Monthly Notices of the Royal Astronomical Society
Publication
Void BAO measurements on quasars from eBOSS
We present the clustering of voids based on the quasar (QSO) sample of the extended Baryon Oscillation Spectroscopic Survey Data Release 16 in configuration...
VVV WIN 1733-3349: a low extinction window to probe the far side of the Milky Way bulge
Windows of low extinction in the Milky Way (MW) have been used along the past decades for the study of the Galactic structure and the stellar population across...
WALLABY pilot survey: H I gas disc truncation and star formation of galaxies falling into the Hydra I cluster
We present results from our analysis of the Hydra I cluster observed in neutral atomic hydrogen (H I) as part of the Widefield ASKAP L-band Legacy All-sky Blind...
WALLABY pre-pilot survey: two dark clouds in the vicinity of NGC 1395
We present the Australian Square Kilometre Array Pathfinder (ASKAP) WALLABY pre-pilot observations of two 'dark' H I sources (with H I masses of a few times 10...
WASP-14 b: transit timing analysis of 19 light curves
Although WASP-14 b is one of the most massive and densest exoplanets on a tight and eccentric orbit, it has never been a target of photometric follow-up...
WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up...
WD 1145+017 photometric observations during eight months of high activity
WD 1145+017 was observed from 2015 November to 2016 July for the purpose of characterizing transit behavior of the white dwarf by dust clouds thought to be...
WD1032 + 011, an inflated brown dwarf in an old eclipsing binary with a white dwarf
We present the discovery of only the third brown dwarf known to eclipse a non-accreting white dwarf. Gaia parallax information and multicolour photometry...
Weak lensing combined with the kinetic Sunyaev-Zel'dovich effect: a study of baryonic feedback
Extracting precise cosmology from weak lensing surveys requires modelling the non-linear matter power spectrum, which is suppressed at small scales due to...