Abstract
The payload of the Faint Intergalactic Redshifted Emission Balloon (FIREBall-2), the second generation of the FIREBall instrument (PI: C. Martin, Caltech), has been calibrated and launched from the NASA Columbia Scientific Balloon Facility in Fort Sumner, New Mexico. FIREBall-2 was launched for the first time on the September 22, 2018, and the payload performed the very first multi-object acquisition from space using a multi-object spectrograph. Our performance-oriented paper presents the calibration and last ground adjustments of FIREBall-2, the in-flight performance assessed based on the flight data, and the predicted instrument's ultimate sensitivity. This analysis predicts that future flights of FIREBall-2 should be able to detect the HI Ly? resonance line in galaxies at z ? 0.67, but will find it challenging to spatially resolve the circumgalactic medium.
| Original language | English (US) |
|---|---|
| Article number | 044004 |
| Journal | Journal of Astronomical Telescopes, Instruments, and Systems |
| Volume | 6 |
| Issue number | 4 |
| DOIs | |
| State | Published - Oct 1 2020 |
Keywords
- balloon borne instrument
- calibration
- electron multiplying CCD
- multi-object spectrograph
- space mission
- ultraviolet
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Control and Systems Engineering
- Instrumentation
- Astronomy and Astrophysics
- Mechanical Engineering
- Space and Planetary Science
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