activity
19942026
most citedOptical and Radio Observations of the Afterglow from GRB990510: Evidence for a Jet

283 citations · 1.2k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2026★ 14 cited

The Vera C. Rubin Observatory Data Preview 1

Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325

We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…

astro-ph.IM2026

Attaining Spectral Energy Distributions With Sub-Percent Uncertainties: All-Sky DA White Dwarf Spectrophotometric Standard Stars For Large Telescopes And Surveys

Abhijit Saha, Edward W. Olszewski, Benjamin M. Boyd +14

We present a synopsis of the project to establish thirty-two new faint () DA white dwarfs as spectrophotometric standards distributed over the whole sky. O…

astro-ph2002★ 101 cited

The Planetary Nebulae Spectrograph: the green light for Galaxy Kinematics

N. G. Douglas, M. Arnaboldi, K. C. Freeman +10

Planetary nebulae are now well established as probes of galaxy dynamics and as standard candles in distance determinations. Motivated by the need to improve the efficiency of plane…

astro-ph2002★ 90 cited

Discovery of GRB 020405 and its Late Red Bump

P. A. Price, S. R. Kulkarni, E. Berger +41

We present the discovery of GRB 020405 made with the Inter-Planetary Network (IPN). With a duration of 60 s, the burst appears to be a typical long duration event. We observed the…

astro-ph2002★ 30 cited

GRB 010921: Strong Limits on an Underlying Supernova from HST

P. A. Price, S. R. Kulkarni, B. P. Schmidt +24

GRB 010921 was the first HETE-2 GRB to be localized via its afterglow emission. The low-redshift of the host galaxy, z=0.451, prompted us to undertake intensive multi-color observa…

astro-ph2002★ 105 cited

GRB 011121: A Massive Star Progenitor

P. A. Price, E. Berger, D. E. Reichart +29

Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z=0.36. More importantly, the multi-color excess in the afterglow detected in the Hubble Space Telescope (…