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3D morphology of open clusters with Gaia EDR3. II.
We identify members of 65 open clusters in the solar neighborhood using the machine-learning algorithm StarGO based on Gaia EDR3 data. After adding members of 20 clusters from... -
CANDELS & KINGFISH disk-dominated galaxies
We examine and quantify how hybrid (e.g., UV+IR) star formation rate (SFR) estimators and the A_FUV_-{beta} relation depend on inclination for disk-dominated galaxies using... -
Subaru/HSC imaging of SQuIGGLE z~0.7 galaxies
We present structural measurements of 145 spectroscopically selected intermediate-redshift (z~0.7), massive (M_*~10^11^M{sun}_) post-starburst galaxies from the SQuIGG->LE... -
Catalog of FR-II radio galaxies
We present an independent catalog (FRIIRGcat) of 45241 Fanaroff-Riley Type II (FR-II) radio galaxies compiled from the Very Large Array Faint Images of the Radio Sky at... -
ALMA-QUARKS Survey. I.
This paper presents an overview of the QUARKS survey, which stands for "Querying Underlying mechanisms of massive star formation with ALMA-Resolved gas Kinematics and... -
TEMPO. Fragmentation and emission properties
The role of massive (>=8M_{sun}) stars in defining the energy budget and chemical enrichment of the interstellar medium in their host galaxy is significant. In this first... -
JWST galaxy morphologies
The James Webb Space Telescope's (JWST's) unprecedented combination of sensitivity, spatial resolution, and infrared coverage has enabled a new era of galaxy morphology... -
Galaxy Zoo: Clump Scout: clumpy SDSS gal. at z~<0.2
Massive, star-forming clumps are a common feature of high-redshift star-forming galaxies. How they formed, and why they are so rare at low redshift, remains unclear. In this... -
Dwarf morphology types and parameters
We use a complete, unbiased sample of 257 dwarf (10^8^M_{sun}<Mstar<10^9.5^M{sun}_) galaxies at z<0.08, in the COSMOS field, to study the morphological mix of the dwarf... -
Galaxies bulge & disk data from SHARDS & HST
We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface... -
DESI Peculiar Velocity survey
We describe the target selection and characteristics of the DESI Peculiar Velocity Survey, the largest survey of peculiar velocities (PVs) using both the fundamental plane (FP)... -
Opt. morphologies of FIR & submm host gal. in COSMOS
We present a host morphological study of 1266 far-infrared galaxies (FIRGs) and submillimeter galaxies (SMGs) in the Cosmic Evolution Survey field using the F160W and F814W...
