Journal: Monthly Notices of the Royal Astronomical Society
Publication
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...
Identifying blue large amplitude pulsators from Gaia DR2 and ZTF DR3
Blue large amplitude pulsators (BLAPs) are hot, subluminous stars undergoing rapid variability with periods of under 60 min. They have been linked with the...
Identifying nearby field T dwarfs in the UKIDSS Galactic Clusters Survey
We present the discovery of two new late-T dwarfs identified in the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Clusters Survey (GCS) Data Release 2 (DR2)...
IMF and [Na/Fe] abundance ratios from optical and NIR spectral features in early-type galaxies
We present a joint analysis of the four most prominent sodium-sensitive features (Na D, Na I λ8190Å, Na I λ1.14 μm, and Na I λ2.21 μm), in the optical and near...
IMF radial gradients in most massive early-type galaxies
Using new long-slit spectroscopy obtained with X-Shooter at ESO-VLT, we study, for the first time, radial gradients of optical and near-infrared initial mass...
IMF shape constraints from stellar populations and dynamics from CALIFA
In this Paper, we describe how we use stellar dynamics information to constrain the shape of the stellar initial mass function (IMF) in a sample of 27 early...
Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles
The back-reaction of baryons on the dark matter halo density profile is of great interest, not least because it is an important systematic uncertainty when...