activity
20022018
most citedA gravitational-wave standard siren measurement of the Hubble constant

1.2k citations · 2.2k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2018★ 134 cited

Discovery of two neighboring satellites in the Carina constellation with MagLiteS

G. Torrealba, V. Belokurov, S. E. Koposov +23

We report the discovery of two ultra-faint satellites in the vicinity of the Large Magellanic Cloud (LMC) in data from the Magellanic Satellites Survey (MagLiteS). Situated 18$^{\c…

astro-ph.SR2018★ 56 cited

The First Post-Kepler Brightness Dips of KIC 8462852

Tabetha S. Boyajian, Roi Alonso, Alex Ammerman +203

We present a photometric detection of the first brightness dips of the unique variable star KIC 8462852 since the end of the Kepler space mission in 2013 May. Our regular photometr…

astro-ph.CO2017★ 1.2k cited

A gravitational-wave standard siren measurement of the Hubble constant

B. P. Abbott, R. Abbott, T. D. Abbott +1308

The detection of GW170817 in both gravitational waves and electromagnetic waves heralds the age of gravitational-wave multi-messenger astronomy. On 17 August 2017 the Advanced LIGO…

astro-ph2008★ 318 cited

Uncovering Extremely Metal-Poor Stars in the Milky Way's Ultra-Faint Dwarf Spheroidal Satellite Galaxies

Evan N. Kirby, Joshua D. Simon, Marla Geha +2

We present new metallicity measurements for 298 individual red giant branch stars in eight of the least luminous dwarf spheroidal galaxies (dSphs) in the Milky Way (MW) system. Our…

astro-ph2007★ 31 cited

Constraints on Circumstellar Material Around the Type Ia Supernova 2007af

Joshua D. Simon, Avishay Gal-Yam, Bryan E. Penprase +9

Patat et al. recently inferred the existence of circumstellar material around a normal Type Ia supernova (SN) for the first time, finding time-variable Na I D absorption lines in t…

astro-ph2007★ 28 cited

Self-consistent massive disks in triaxial dark matter halos

Jeremy Bailin, Josh D. Simon, Alberto D. Bolatto +2

Galactic disks in triaxial dark matter halos become deformed by the elliptical potential in the plane of the disk in such a way as to counteract the halo ellipticity. We develop a…