Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Astronomy, Panchromatic film, Galaxy, and Star cluster.
The JWST Resolved Stellar Populations Early Release Science Program. V. DOLPHOT Stellar Photometry for NIRCam and NIRISS
The JWST Resolved Stellar Populations Early Release Science Program. IV. The Star Formation History of the Local Group Galaxy WLM
The JWST Resolved Stellar Populations Early Release Science Program. II. Survey Overview
Advancing Space Science Requires NASA Support for Coordination Between the Science Mission Directorate Communities
The JWST Resolved Stellar Populations Early Release Science Program. I. NIRCam Flux Calibration
Advancing Space Science Requires NASA Support for Coordination Between the Science Mission Directorate Communities
Scientific discovery with the James Webb Space Telescope
The field white dwarf mass distribution
THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. XV. THE BEAST: BAYESIAN EXTINCTION AND STELLAR TOOL*
THE HIGH-MASS STELLAR INITIAL MASS FUNCTION IN M31 CLUSTERS
PANCHROMATIC HUBBLE ANDROMEDA TREASURY. XII. MAPPING STELLAR METALLICITY DISTRIBUTIONS IN M31
THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. V. AGES AND MASSES OF THE YEAR 1 STELLAR CLUSTERS
An age difference of two billion years between a metal-rich and a metal-poor globular cluster
ULTRA-DEEP<i>HUBBLE SPACE TELESCOPE</i>IMAGING OF THE SMALL MAGELLANIC CLOUD: THE INITIAL MASS FUNCTION OF STARS WITH<i>M</i>≲ 1<i>M</i><sub>☉</sub>
An extended main-sequence turn-off in the Small Magellanic Cloud star cluster NGC 411★
THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY
THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. I. BRIGHT UV STARS IN THE BULGE OF M31
THE SPLASH SURVEY: KINEMATICS OF ANDROMEDA's INNER SPHEROID
THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. IV. A PROBABILISTIC APPROACH TO INFERRING THE HIGH-MASS STELLAR INITIAL MASS FUNCTION AND OTHER POWER-LAW FUNCTIONS
THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. III. MEASURING AGES AND MASSES OF PARTIALLY RESOLVED STELLAR CLUSTERS