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Proceedings Paper

GLUV: a balloon-borne high-cadence ultraviolet monitoring telescope for supernova shock breakouts and exoplanet atmospheres
Author(s): Rob Sharp; B. Tucker; R. Ridden-Harper; G. Bloxham; M. Petkovic
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Paper Abstract

Routine photometric monitoring at near-ultraviolet wavelengths (< 400 nm) is compromised from the ground due to highly variable atmospheric transmission and cloud cover. The GLUV project will mount a modest sized telescope (200 mm primary) on a series of long-duration high-altitude balloon flights. The wide field camera (~7 deg2) will perform high cadence (10-300 second rolling integrations) each night for campaign durations of three to six months. The principle science mission is the early-time detection of supernova shock-breakout at near-ultraviolet wavelengths. Additionally, early design analysis has shown the system is also able to probe the atmospheric composition of exoplanet atmospheres through the combination of UV transit measurements with ground-based measurements at longer wavelengths. In this presentation we consider the specifications for a long-duration balloon platform for such a mission, focusing on the necessary mission requirements (sensitivity, sky coverage, cadence etc.) and the available platform suitability. Particular attention is paid to platform flight altitude and atmospheric transmission.

Paper Details

Date Published: 3 August 2016
PDF: 11 pages
Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99080V (3 August 2016); doi: 10.1117/12.2231555
Show Author Affiliations
Rob Sharp, The Australian National Univ. (Australia)
B. Tucker, The Australian National Univ. (Australia)
R. Ridden-Harper, The Australian National Univ. (Australia)
G. Bloxham, The Australian National Univ. (Australia)
M. Petkovic, The Australian National Univ. (Australia)


Published in SPIE Proceedings Vol. 9908:
Ground-based and Airborne Instrumentation for Astronomy VI
Christopher J. Evans; Luc Simard; Hideki Takami, Editor(s)

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