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astro-ph.GA20241 cited

The Low-Redshift Lyman Continuum Survey: The Roles of Stellar Feedback and ISM Geometry in LyC Escape

Sophia R. Flury, Anne E. Jaskot, Alberto Saldana-Lopez +30

One of the fundamental questions of cosmology is the origin and mechanism(s) responsible for the reionization of the Universe beyond . To address this question, many studie…

astro-ph.GA20241 cited

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Broad-line AGN at revealed by JWST/NIRCam WFSS

Xiaojing Lin, Feige Wang, Xiaohui Fan +33

Low-luminosity AGNs with low-mass black holes (BHs) in the early universe are fundamental to understanding the BH growth and their co-evolution with the host galaxies. Utilizing JW…

astro-ph.GA202441 cited

Ubiquitous broad-line emission and the relation between ionized gas outflows and Lyman continuum escape in Green Pea galaxies

R. O. Amorín, M. Rodríguez-Henríquez, V. Fernández +29

We report observational evidence of highly turbulent ionized gas kinematics in a sample of 20 Lyman continuum (LyC) emitters (LCEs) at low redshift (). Detailed Gaussian…

astro-ph.GA2024

Polarimetry of the Ly-alpha envelope of the radio-quiet quasar SDSS J124020.91+145535.6

P. North, M. Hayes, M. Millon +5

The radio-quiet quasar SDSS J1240+1455 lies at a redshift of z=3.11, is surrounded by a Ly-alpha blob (LAB), and is absorbed by a proximate damped Ly-alpha system. In order to bett…

astro-ph.GA20245 cited

A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields

Vasily Kokorev, Karina I. Caputi, Jenny E. Greene +9

Observations with the James Webb Space Telescope (JWST) have uncovered numerous faint active galactic nuclei (AGN) at and beyond. These objects are key to our understandin…

astro-ph.GA20235 cited

MAGNIF: A Tentative Lensed Rotating Disk at detected by JWST NIRCam WFSS with Dynamical Forward Modeling

Zihao Li, Zheng Cai, Fengwu Sun +39

We report galaxy MACS0416-Y3 behind the lensing cluster MACSJ0416.1--2403 as a tentative rotating disk at detected through its [OIII] emission in JWST NIRCam…