S. A. Stanford

The CatWISE2020 Catalog

Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey

Euclid Preparation. XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3

Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT

Galaxy populations in the most distant SPT-SZ clusters

The growth of brightest cluster galaxies and intracluster light over the past 10 billion years

Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at 1.4 ≲ z ≲ 1.7

Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters to<i>z</i> = 1.3

Galaxy Populations in Massive Galaxy Clusters to $z$ = 1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction

STAR-FORMING BRIGHTEST CLUSTER GALAXIES AT 0.25 &lt; z &lt; 1.25: A TRANSITIONING FUEL SUPPLY

COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY

STAR FORMATION AND AGN ACTIVITY IN GALAXY CLUSTERS FROM z = 1–2: A MULTI-WAVELENGTH ANALYSIS FEATURING HERSCHEL/PACS

SPT-GMOS: A GEMINI/GMOS-SOUTH SPECTROSCOPIC SURVEY OF GALAXY CLUSTERS IN THE SPT-SZ SURVEY

GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY

The XXL Survey

MASS CALIBRATION AND COSMOLOGICAL ANALYSIS OF THE SPT-SZ GALAXY CLUSTER SAMPLE USING VELOCITY DISPERSION σ_<i>v</i>AND X-RAY<i>Y</i>_XMEASUREMENTS

A MEASUREMENT OF GRAVITATIONAL LENSING OF THE COSMIC MICROWAVE BACKGROUND BY GALAXY CLUSTERS USING DATA FROM THE SOUTH POLE TELESCOPE

Baryon content of massive galaxy clusters at 0.57 &lt; <i>z</i> &lt; 1.33

OPTICAL SPECTROSCOPY AND VELOCITY DISPERSIONS OF GALAXY CLUSTERS FROM THE SPT-SZ SURVEY

SPT-CL J2040–4451: AN SZ-SELECTED GALAXY CLUSTER AT<i>z</i>= 1.478 WITH SIGNIFICANT ONGOING STAR FORMATION

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

THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 &lt;<i>z</i>&lt; 1.2 SELECTED FROM THE SPT-SZ SURVEY

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 NEW POPULATION OF HIGH-<i>z</i>, DUSTY Lyα EMITTERS AND BLOBS DISCOVERED BY<i>WISE</i>: FEEDBACK CAUGHT IN THE ACT?

SPT-CL J0205–5829: A<i>z</i>= 1.32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV-ZEL'DOVICH EFFECT SURVEY

THE <i>SPITZER</i> SOUTH POLE TELESCOPE DEEP FIELD: SURVEY DESIGN AND INFRARED ARRAY CAMERA CATALOGS

THE<i>HUBBLE SPACE TELESCOPE</i>CLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVE<i>z</i>&gt; 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE

Epigenetic control of steroid hormone signaling in axon pruning