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19932026
most citedA very energetic supernova associated with the gamma-ray burst of 29 March 2003

1.5k citations · 16k across the 213 of their papers we have counts for

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Showing 2021 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2021

New spectroscopic confirmations of Lyman- emitters at z 7 from the LAGER survey

Santosh Harish, Isak G. B. Wold, Sangeeta Malhotra +14

We report spectroscopic confirmations of 15 Lyman-alpha galaxies at , implying a spectroscopic confirmation rate of 80% on candidates selected from LAGER (Lyman-Alpha…

astro-ph.GA2021★ 30 cited

Conditions for detecting lensed Population III galaxies in blind surveys with the James Webb Space Telescope, the Roman Space Telescope and Euclid

Anton Vikaeus, Erik Zackrisson, Daniel Schaerer +5

Dark matter halos that reach the HI-cooling mass without prior star formation or external metal pollution represent potential sites for the formation of small - extremely faint - P…

astro-ph.GA2021★ 1 cited

Evidence for Black Holes in Green Peas from WISE colors and variability

Santosh Harish, Sangeeta Malhotra, James E. Rhoads +3

We explore the presence of active galactic nuclei (AGN)/black holes (BH) in Green Pea galaxies (GPs), motivated by the presence of high ionization emission lines such as HeII and […

astro-ph.GA2021★ 70 cited

LAGER Ly Luminosity Function at , Implications for Reionization

Isak G. B. Wold, Sangeeta Malhotra, James Rhoads +17

We present a new measurement of the Ly luminosity function at redshift , finding moderate evolution from that is consistent with a fully or largely ionized $z\sim…

astro-ph.GA2021★ 28 cited

The Compact UV Size of Green Pea Galaxies As Local Analogs of High-redshift Ly-Emitters

Keunho J. Kim, Sangeeta Malhotra, James E. Rhoads +1

We study the dependence of Ly escape from galaxies on UV continuum size and luminosity using a sample of 40 Green Pea (GP) galaxies, which are the best local analogs of high-red…

astro-ph.GA2021★ 14 cited

Correlations between H Equivalent Width and Galaxy Properties at : Physical or Selection-driven?

Ali Ahmad Khostovan, Sangeeta Malhotra, James E. Rhoads +13

The H equivalent width (EW) is an observational proxy for specific star formation rate (sSFR) and a tracer of episodic star-formation activity. Previous assessments show that EW…