Northern Sky Variability Survey: Public Data Release

Autor: S. L. Marshall, Katherine E. McGowan, Timothy A. McKay, S. Fletcher, R. Balsano, W. T. Vestrand, Robert Kehoe, Brian C. Lee, Jeffrey J. Bloch, P. R. Wozniak, Galen Gisler, Karen Kinemuchi, John J. Szymanski, E. S. Rykoff, D. A. Smith, Donald E. Casperson, Carl W. Akerlof, Jim Wren
Rok vydání: 2004
Předmět:
Zdroj: The Astronomical Journal. 127:2436-2449
ISSN: 1538-3881
0004-6256
DOI: 10.1086/382719
Popis: The Northern Sky Variability Survey (NSVS) is a temporal record of the sky over the optical magnitude range from 8 to 15.5. It was conducted in the course of the first generation Robotic Optical Transient Search Experiment (ROTSE-I) using a robotic system of four co-mounted unfiltered telephoto lenses equipped with CCD cameras. The survey was conducted from Los Alamos, NM, and primarily covers the entire northern sky. Some data in southern fields between declinations 0 and -38 deg is also available, although with fewer epochs and noticeably lesser quality. The NSVS contains light curves for approximately 14 million objects. With a one year baseline and typically 100-500 measurements per object, the NSVS is the most extensive record of stellar variability across the bright sky available today. In a median field, bright unsaturated stars attain a point to point photometric scatter of ~0.02 mag and position errors within 2 arcsec. At Galactic latitudes |b| < 20 deg the data quality is limited by severe blending due to ~14 arcsec pixel size. We present basic characteristics of the data set and describe data collection, analysis, and distribution. All NSVS photometric measurements are available for on-line public access from the Sky Database for Objects in Time-Domain (SkyDOT; http://skydot.lanl.gov) at LANL. Copies of the full survey photometry may also be requested on tape.
accepted for publication in Astronomical Journal
Databáze: OpenAIRE