Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Cluster (spacecraft).
Galaxy mergers in the epoch of reionization – I. A JWST study of pair fractions, merger rates, and stellar mass accretion rates at <i>z</i> = 4.5–11.5
EPOCHS. I. The Discovery and Star-forming Properties of Galaxies in the Epoch of Reionization at 6.5 < <i>z</i> < 18 with PEARLS and Public JWST Data
Globular Clusters in the Galaxy Cluster MACS0416 at <i>z</i> = 0.397
EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin<sup>2</sup> of Deep, Blank Fields from the PEARLS Survey and Public JWST Data
The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
JWST Photometric Time-delay and Magnification Measurements for the Triply Imaged Type Ia “SN H0pe” at z = 1.78
JWST’s PEARLS: Resolved study of the stellar and dust components in starburst galaxies at cosmic noon
JWST’s PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at <i>z</i> = 0.4
PEARLS: A Potentially Isolated Quiescent Dwarf Galaxy with a Tip of the Red Giant Branch Distance of 30 Mpc
JWST NIRCam Photometry: A Study of Globular Clusters Surrounding Bright Elliptical Galaxy VV 191a at z = 0.0513
An improved <i>Magellan</i> weak lensing analysis of the galaxy cluster Abell 2744
The FENIKS Survey: Multiwavelength Photometric Catalog in the UDS Field, and Catalogs of Photometric Redshifts and Stellar Population Properties
Early Results from GLASS-JWST. XIV. A Spectroscopically Confirmed Protocluster 650 Million Years after the Big Bang
Early Results from GLASS-JWST. XIX. A High Density of Bright Galaxies at z ≈ 10 in the A2744 Region
JWST/NIRCam Probes Young Star Clusters in the Reionization EraSunrise Arc
A magnified compact galaxy at redshift 9.51 with strong nebular emission lines
Early Results from GLASS-JWST. XI. Stellar Masses and Mass-to-light Ratio of z > 7 Galaxies
The GLASS-JWST Early Release Science Program. III. Strong-lensing Model of Abell 2744 and Its Infalling Regions
Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST
EPOCHS VII: discovery of high-redshift (6.5 &lt; <i>z</i> &lt; 12) AGN candidates in JWST ERO and PEARLS data
JWST Reveals a Possible z ∼ 11 GalaxyMerger in Triply Lensed MACS0647–JD
JWST’s PEARLS: Mothra, a new kaiju star at <i>z</i> = 2.091 extremely magnified by MACS0416, and implications for dark matter models
JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
The GLASS-JWST Early Release Science Program. II. Stage I Release of NIRCam Imaging and Catalogs in the Abell 2744 Region
Early Results from GLASS-JWST. XIII. A Faint, Distant, and Cold Brown Dwarf*
JWST’s PEARLS: TN J1338–1942 – I. Extreme jet-triggered star formation in a <i>z</i> = 4.11 luminous radio galaxy
CLASH-VLT: The Inner Slope of the MACS J1206.2-0847 Dark Matter Density Profile
Are JWST/NIRCam Color Gradients in the Lensed z = 2.3 Dusty Star-forming Galaxy El Anzuelo Due to Central Dust Attenuation or Inside-out Galaxy Growth?
Spectroscopy of the supernova H0pe host galaxy at redshift 1.78
EPOCHS IX. When cosmic dawn breaks: evidence for evolved stellar populations in 7 &lt; <i>z</i> &lt; 12 galaxies from PEARLS GTO and public NIRCam imaging