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A Robotic Wide-Angle Hα Survey of the Southern Sky

Published online by Cambridge University Press:  12 April 2016

John E. Gaustad
Affiliation:
Dept. of Phys. & Astr., Swarthmore Coll., Swarthmore PA 19081, USA
Wayne Rosing
Affiliation:
Las Cumbres Obs., 1500 Miramar Beach, Montecito CA 93108, USA
Peter McCullough
Affiliation:
Dept. of Astronomy, Univ. of Illinois, Urbana IL 51801, USA
Dave Van Buren
Affiliation:
Extrasolar Research Corporation, Niskayuna NY 12309, USA

Abstract

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We are conducting a robotic wide-angle imaging survey of the southern sky at 656.3 nm wavelength, the Hα emission line of hydrogen. Each image of the survey covers an area of the sky 13° square at an angular resolution of approximately one arcminute, and reaches a sensitivity level of 0.5 Rayleigh (3 × 10−18erg cm−2s−1arcsec−2), corresponding to an emission measure of 1 cm−6pc, and to a brightness temperature for microwave free-free emission of 3 µK at 30 GHz.

Type
II. Monitoring and Surveys
Copyright
Copyright © Astronomical Society of the Pacific 2001