next up previous contents
Next: Instrument Description Up: Instrument Definition Previous: Instrument Definition

Scientific Performances Summary

IBIS is a gamma-ray coded-mask telescope observing celestial objects of all classes ranging from the most compact galactic systems to extragalactic objects, with powerful diagnostic capabilities of fine imaging, source identification and spectral sensitivity in both continuum and lines. It is able to localize weak sources at low energy to better than a few arcminutes accuracy, covering the entire energy range from a few tens of keV to several MeV. Table [*] gives an overview of the scientific capabilities of IBIS. The effective area curves are given in Fig. [*].


Table: Scientific Parameters of IBIS. Mathematical symbols are not rendered here. Please refer to the PDF version of the document.
Operating energy range 15 keV - 10 MeV
Energy resolution (FWHM) 7% @ 100 keV
  9% @ 1 MeV
Effective Area ISGRI: 960 cm at 50 keV
  PICsIT: 870 cm at 300 keV (single events)
  PICsIT: 275 cm at 1 MeV (multiple events)
Field of view 8.3 8.0 (fully coded)
  19 19 (partially coded, 50%)
Angular resolution (FWHM) 12
Point source location accuracy 30 @100 keV
(90% error radius) 5 @1 MeV
Continuum sensitivity, @100 keV
photons cm s keV 1 - 2 @ 1 MeV
(3 detection, , 10 s integration)  
Narrow line sensitivity, @100 keV
photons cm s @ 1 MeV
(3 , 10 s integration)  
Absolute timing accuracy (3 ) ISGRI: 61 s
  PICsIT: 0.976 - 500ms (selected from ground)

Figure: IBIS effective area
Image ibis_area


next up previous contents
Next: Instrument Description Up: Instrument Definition Previous: Instrument Definition

2020-09-18