output
19962026
most citedBeaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir

1.2k citations

Showing 2021Show all

29 papers · 1 filter

astro-ph.EP2021★ 3 cited

An Imaging Search for Post-Main-Sequence Planets of Sirius B

Miles Lucas, Michael Bottom, Garreth Ruane +1

We present deep imaging of Sirius B, the closest and brightest white dwarf, to constrain post-main-sequence planetary evolution in the Sirius system. We use Keck/NIRC2 in L'-band (…

astro-ph.GA2021★ 30 cited

KODIAQ-Z: Metals and Baryons in the Cool Intergalactic and Circumgalactic Gas at 2.2<z<3.6

Nicolas Lehner, Claire Kopenhafer, John O'Meara +8

We present the KODIAQ-Z survey aimed to characterize the cool, photoionized gas at 2.2<z<3.6 in 202 HI-selected absorbers with 14.6<log N(HI)<20, i.e., the gaseous interface betwee…

astro-ph.GA2021★ 96 cited

Spectroscopic Confirmation of a Protocluster at with a High Fraction of Quiescent Galaxies

Ian McConachie, Gillian Wilson, Ben Forrest +10

We report the discovery of MAGAZ3NE J095924+022537, a spectroscopically-confirmed protocluster at around a spectroscopically-confirmed -quiesc…

astro-ph.IM2021★ 5 cited

Developing Adaptive Secondary Mirror Concepts for the APF and W.M. Keck Observatory Based on HVR Technology

Philip M. Hinz, Rachel Bowens-Rubin, Christoph Baranec +16

An Adaptive secondary mirror (ASM) allows for the integration of adaptive optics (AO) into the telescope itself. Adaptive secondary mirrors, based on hybrid variable reluctance (HV…

astro-ph.GA2021★ 38 cited

The CGM Survey: Circumgalactic O VI from dwarf to massive star-forming galaxies

K. Tchernyshyov, J. K. Werk, M. C. Wilde +9

We combine 126 new galaxy-O VI absorber pairs from the CGM survey with 123 pairs drawn from the literature to examine the simultaneous dependence of the column density of O VI…

astro-ph.GA2021★ 21 cited

Lyman Continuum Galaxy Candidates in COSMOS

Laura J. Prichard, Marc Rafelski, Jeff Cooke +11

Star-forming galaxies are the sources likely to have reionized the universe. As we cannot observe them directly due to the opacity of the intergalactic medium at , we st…