Journal: Monthly Notices of the Royal Astronomical Society
Publication
Hα flares from V404 Cyg in quiescence
We present a spectrophotometric study of short-term optical variability in the quiescent black hole X-ray transient V404 Cyg. This includes two nights of high...
Hα kinematics of 11 starburst galaxies selected from the Sloan Digital Sky Survey
We present analysis of Fabry-Perot interferometric observations for a sample of 11 starburst galaxies with redshift z ≲ 0.03 selected from the Sloan Digital Sky...
We present a study of the kinematics of the isolated spiral galaxy NGC 864, using Hα Fabry-Perot data obtained with the Galaxy Hα Fabry-Perot System (GHαFaS)...
Hα kinematics of S4G spiral galaxies - II. Data description and non-circular motions
We present a kinematical study of 29 spiral galaxies included in the Spitzer Survey of Stellar Structure in Galaxies, using Hα Fabry-Perot (FP) data obtained...
Hα kinematics of S4G spiral galaxies - III. Inner rotation curves
We present a detailed study of the shape of the innermost part of the rotation curves of a sample of 29 nearby spiral galaxies, based on high angular and...
Hα kinematics of the Spitzer Infrared Nearby Galaxies Survey - II
This is the second part of an Hα kinematics follow-up survey of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample. The aim of this paper is to shed new...
Hα star formation rates in massive galaxies at z˜ 1
We present a near-infrared spectroscopic study of a stellar mass selected sample of galaxies at z˜ 1 utilizing the Long-slit Intermediate Resolution Infrared...
IC 2602: a lithium depletion boundary age and new candidate low-mass stellar members
We report the results from a photometric and spectroscopic survey of ˜1.4 deg2 of the young open cluster IC 2602. Fourteen objects have been identified as...
Identification of tidal features in deep optical galaxy images with convolutional neural networks
Interactions between galaxies leave distinguishable imprints in the form of tidal features, which hold important clues about their mass assembly. Unfortunately...