activity
19952025
most citedLSST Science Book, Version 2.0

924 citations · 1.2k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2025★ 8 cited

NSF-DOE Vera C. Rubin Observatory Observations of Interstellar Comet 3I/ATLAS (C/2025 N1)

Colin Orion Chandler, Pedro H. Bernardinelli, Mario Jurić +305

We report on the observation and measurement of astrometry, photometry, morphology, and activityof the interstellar object 3I/ATLAS, also designated C/2025 N1 (ATLAS) with the NSF-…

astro-ph.CO2012★ 119 cited

Redshifts, Sample Purity, and BCG Positions for the Galaxy Cluster Catalog from the first 720 Square Degrees of the South Pole Telescope Survey

J. Song, A. Zenteno, B. Stalder +74

We present the results of the ground- and space-based optical and near-infrared (NIR) follow-up of 224 galaxy cluster candidates detected with the Sunyaev-Zel'dovich (SZ) effect in…

astro-ph.IM2009★ 924 cited

LSST Science Book, Version 2.0

LSST Science Collaboration, Paul A. Abell, Julius Allison +245

A survey that can cover the sky in optical bands over wide fields to faint magnitudes with a fast cadence will enable many of the exciting science opportunities of the next decade.…

astro-ph2002★ 1 cited

LIFTS: an Imaging Fourier Transform Spectrograph for Astronomy

Ron Wurtz, Edward Wishnow, Sébastien Blais-Ouellette +5

We present the first astronomical observations of the Livermore Imaging Fourier Transform Spectrograph for visible-band astronomy using the 3.5-meter Apache Point Observatory.

astro-ph1999★ 119 cited

Binary Microlensing Events from the MACHO Project

MACHO, GMAN collaborations, : +1

We present the lightcurves of 21 gravitational microlensing events from the first six years of the MACHO Project gravitational microlensing survey which are likely examples of lens…

astro-ph1997★ 4 cited

Optical identification of the LMC supersoft source RXJ0527.8-6954 from MACHO Project photometry

C. Alcock et al

We identify the likely optical counterpart to the LMC supersoft X-ray source RXJ0527.8-6954, and hence recover HV2554. This identification is based on an analysis of approximately…