ISOPHOT - CAPABILITIES AND PERFORMANCE

Citation
D. Lemke et al., ISOPHOT - CAPABILITIES AND PERFORMANCE, Astronomy and astrophysics, 315(2), 1996, pp. 64-70
Citations number
22
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00046361
Volume
315
Issue
2
Year of publication
1996
Pages
64 - 70
Database
ISI
SICI code
0004-6361(1996)315:2<64:I-CAP>2.0.ZU;2-9
Abstract
ISOPHOT covers the largest wavelength range on ISO from 2.5 to 240 mu m. Its scientific capabilities include multi filter and multi-aperture photometry, polarimetry, imaging and spectrophotometry. All modes can optionally include a focal plane chopper. The backbone of the photome tric calibration are internal standard sources checked against celesti al primary standards. The instrument is in excellent condition with al l components functioning properly. There is increased detector noise d ue to the ionizing cosmic radiation affecting the detectability of the faintest sources. All lessons learnt from operating the instrument in space are continuously being implemented in the standard data reducti on software packages available to every observer. Particular strengths of the instrument include tile detectability of very cold sources, hi gh resolution mapping and fast spectrophotometry. The far infrared ser endipity sky survey performed during slews of the satellite has succes sfully started.