Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Photometry (optics).
Silicate precursor silane detected in cold low-metallicity brown dwarf
Euclid Quick Data Release (Q1): Hunting for luminous z > 6 galaxies in the Euclid Deep Fields -- forecasts and first bright detections
The Initial Mass Function Based on the Full-sky 20 pc Census of ∼3600 Stars and Brown Dwarfs
Methane emission from a cool brown dwarf
The Near-Earth Object Surveyor Mission
An Improved Near-infrared Spectrum of the Archetype Y Dwarf WISEP J182831.08+265037.8
The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries*
The multiple merger assembly of a hyperluminous obscured quasar at redshift 4.6
Eddington-limited Accretion in z ∼ 2 WISE-selected Hot, Dust-obscured Galaxies
Heavy X-ray obscuration in the most luminous galaxies discovered by WISE
<i>Planck</i>2015 results
STAR FORMATION AND AGN ACTIVITY IN GALAXY CLUSTERS FROM z = 1–2: A MULTI-WAVELENGTH ANALYSIS FEATURING HERSCHEL/PACS
QUASAR VARIABILITY IN THE MID-INFRARED
<i>Planck</i>2015 results
HALF OF THE MOST LUMINOUS QUASARS MAY BE OBSCURED: INVESTIGATING THE NATURE OF<i>WISE</i>-SELECTED HOT DUST-OBSCURED GALAXIES
<i>HUBBLE SPACE TELESCOPE</i>SPECTROSCOPY OF BROWN DWARFS DISCOVERED WITH THE WIDE-FIELD INFRARED SURVEY EXPLORER
INITIAL PERFORMANCE OF THE<i>NEOWISE</i>REACTIVATION MISSION
<i>Planck</i>2013 results. XXIX. The<i>Planck</i>catalogue of Sunyaev-Zeldovich sources
<i>NuSTAR</i>AND<i>XMM-NEWTON</i>OBSERVATIONS OF LUMINOUS, HEAVILY OBSCURED,<i>WISE</i>-SELECTED QUASARS AT<i>Z</i>∼ 2
Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxies
MID-INFRARED SELECTION OF ACTIVE GALACTIC NUCLEI WITH THE<i>WIDE-FIELD INFRARED SURVEY EXPLORER</i>. II. PROPERTIES OF<i>WISE</i>-SELECTED ACTIVE GALACTIC NUCLEI IN THE NDWFS BOÖTES FIELD
THE ERA OF STAR FORMATION IN GALAXY CLUSTERS
CHARACTERIZING THE MID-INFRARED EXTRAGALACTIC SKY WITH<i>WISE</i>AND SDSS
THE CLUSTER AND FIELD GALAXY ACTIVE GALACTIC NUCLEUS FRACTION AT<i>z</i>= 1-1.5: EVIDENCE FOR A REVERSAL OF THE LOCAL ANTICORRELATION BETWEEN ENVIRONMENT AND AGN FRACTION
The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years★
A STUDY OF THE DIVERSE T DWARF POPULATION REVEALED BY WISE
2013cited by 101position: middle
A NEW POPULATION OF HIGH-<i>z</i>, DUSTY Lyα EMITTERS AND BLOBS DISCOVERED BY<i>WISE</i>: FEEDBACK CAUGHT IN THE ACT?
THE EXEMPLAR T8 SUBDWARF COMPANION OF WOLF 1130
THE <i>SPITZER</i> SOUTH POLE TELESCOPE DEEP FIELD: SURVEY DESIGN AND INFRARED ARRAY CAMERA CATALOGS