Tipo de publicación: Con árbitro

  • Publicación
    Identifying Anomalous DESI Galaxy Spectra with a Variational Autoencoder
    The tens of millions of spectra being captured by the Dark Energy Spectroscopic Instrument (DESI) provide tremendous discovery potential. In this work we show...
  • Publicación
    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...
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    Identifying Close-in Jupiters that Arrived via Disk Migration: Evidence of Primordial Alignment, Preference of Nearby Companions and Hint of Runaway Migration
    Two leading hypotheses for hot Jupiter migration are disk migration and high-eccentricity migration (HEM). Stellar obliquity is commonly used to distinguish...
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    Identifying Missing Quasars from the DESI Bright Galaxy Survey
    The Dark Energy Spectroscopic Instrument (DESI) cosmology survey includes a Bright Galaxy Survey (BGS), which will yield spectra for over 10 million bright...
  • Publicación
    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)...
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    Identifying New High-confidence Polluted White Dwarf Candidates Using Gaia XP Spectra and Self-organizing Maps
    The identification of new white dwarfs (WDs) polluted with heavy elements is important since they provide a valuable tool for inferring the chemical properties...
  • Publicación
    Identifying RR Lyrae Variable Stars in Six Years of the Dark Energy Survey
    We present a search for RR Lyrae stars using the full six-year data set from the Dark Energy Survey covering ∼5000 deg 2 of the southern sky. Using a multistage...
  • Publicación
    Identifying Sagittarius Stream Stars by Their APOGEE Chemical Abundance Signatures
    The SDSS-IV Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey provides precise chemical abundances of 18 chemical elements for ∼176,000 red...
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    Identifying the best iron-peak and α-capture elements for chemical tagging: The impact of the number of lines on measured scatter
    Aims: The main goal of this work is to explore which elements carry the most information about the birth origin of stars and, as such, which are best suited for...