Searching for optical transients in real-time : the RAPTOR experiment /.
- W. Thomas
- Konstantin N.
- Donald E.
- Mark C.
- Katherine E.
- Simon J.
- William C.
- Dan L.
- Robert A.
- James
A rich, but relatively unexplored, region in optical astronomy is the study of transients with durations of less than a day. We describe a wide-field optical monitoring system, RAPTOR, which is designed to identify and make follow-up observations of optical transients in real-time. The system is composed of an array of telescopes that continuously monitor about 1500 square degrees of the sky for transients down to about 12' magnitude in 60 seconds and a central fovea telescope that can reach 16{approx}m' agnitude in 60 seconds. Coupled to the telescope array is a real-time data analysis pipeline that is designed to identify transients on timescales of seconds. In a manner analogous to human vision, the entire array is mounted on a rapidly slewing robotic mount so that the fovea of the array can be rapidly directed at transients identified by the wide-field system. The goal of the project is to develop a ground-based optical system that can reliably identify transients in real-time and ultimately generate alerts with source locations to enable follow-up observations wilh other, larger, telescopes.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- USDOE
- OSTI ID:
- 975969
- Report Number(s):
- LA-UR-02-0369; LA-UR-02-369; TRN: US201018%%1054
- Resource Relation:
- Journal Volume: 662; Conference: Submitted to: Woods Hole Gamma-Ray Burst Meeting
- Country of Publication:
- United States
- Language:
- English
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