Published September 9, 2019 | Version public
Book Section - Chapter

2018 flight of the faint intergalactic medium redshifted emission balloon (FIREBall-2) (Conference Presentation)

Abstract

In this talk, I will describe briefly the telescope, instrument, and flight of the Faint Intergalactic medium Redshifted Emission Balloon (FIREBall-2). FIREBall-2 is a UV multi-object spectrograph fed by a 1 meter parabola mirror. The instrument was designed to observe 4 pre-selected fields and uses a UV optimized delta-doped EMCCD. The telescope flew on September 22, 2018 from Fort Sumner, NM, as part of the fall CSBF balloon campaign. The telescope collected data for several night hours before being cut down. I will describe the testing, flight, and hardware performance with an emphasis on the in flight performance of the instrument, including resolution, throughput, and the overall operation of the UV optimized EMCCD. Additional talks will be presented on other aspects of the flight and data.

Additional Information

© 2019 Society of Photo-Optical Instrumentation Engineers (SPIE).

Additional details

Identifiers

Eprint ID
98601
Resolver ID
CaltechAUTHORS:20190912-090006441

Dates

Created
2019-09-12
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Space Radiation Laboratory
Series Name
Proceedings of SPIE
Series Volume or Issue Number
11118