12 May 2015 ISS-Lobster: a low-cost wide-field x-ray transient detector on the ISS
Author Affiliations +
Abstract
ISS-Lobster is a wide-field X-ray transient detector proposed to be deployed on the International Space Station. Through its unique imaging X-ray optics that allow a 30 deg by 30 deg FoV, a 1 arc min position resolution and a 1.6x10-11 erg/(sec cm2) sensitivity in 2000 sec, ISS-Lobster will observe numerous events per year of X-ray transients related to compact objects, including: tidal disruptions of stars by supermassive black holes, supernova shock breakouts, neutron star bursts and superbursts, high redshift Gamma-Ray Bursts, and perhaps most exciting, X-ray counterparts of gravitational wave detections involving stellar mass and possibly supermassive black holes. The mission includes a 3-axis gimbal system that allows fast Target of Opportunity pointing, and a small gamma-ray burst monitor. In this article we focus on ISS-Lobster measurements of X-ray counterparts of detections by the world-wide ground-based gravitational wave network.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jordan Camp, Jordan Camp, Scott Barthelmy, Scott Barthelmy, Rob Petre, Rob Petre, Neil Gehrels, Neil Gehrels, Francis Marshall, Francis Marshall, Andy Ptak, Andy Ptak, Judith Racusin, Judith Racusin, } "ISS-Lobster: a low-cost wide-field x-ray transient detector on the ISS", Proc. SPIE 9510, EUV and X-ray Optics: Synergy between Laboratory and Space IV, 951007 (12 May 2015); doi: 10.1117/12.2176745; https://doi.org/10.1117/12.2176745
PROCEEDINGS
7 PAGES


SHARE
RELATED CONTENT

Terrestrial gamma-ray flashes monitor demonstrator on CubeSat
Proceedings of SPIE (September 19 2016)
X RED a satellite mission concept to detect early...
Proceedings of SPIE (August 18 2005)
Swift gamma-ray burst MIDEX
Proceedings of SPIE (December 13 2000)
The swift x-ray telescope: status and performance
Proceedings of SPIE (September 13 2007)

Back to Top