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Crab intensity from JEM-X onboard INTEGRAL and a source of ”deadtime” Niels J. Westergaard C. Budtz-Jørgensen S. Brandt C. A. Oxborrow Evolution in time connecting to particle background rate.

Crab intensity from JEM-X onboard INTEGRAL and a source …web.mit.edu/iachec/meetings/2011/Presentations/Westergaard_JEMX.pdf · Crab intensity from JEM-X onboard INTEGRAL ... 4

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Crab intensity from JEM-X onboard INTEGRAL

and a source of ”deadtime” Niels J. Westergaard C. Budtz-Jørgensen

S. Brandt C. A. Oxborrow

Evolution in time connecting to particle background rate.

2011-04-11 IACHEC Meeting #6 2 DTU Space, Technical University of Denmark

JEM-X HARDWARE

Mask : 535 mm

Mask hex holes: 3 mm

Detector diam : 250 mm

Mask-Detector: 3401 mm

2011-04-11 IACHEC Meeting #6 3 DTU Space, Technical University of Denmark

JEM-X Detector

2011-04-11 IACHEC Meeting #6 4 DTU Space, Technical University of Denmark

The 10 micron anode strips are destroyed by heavy cosmic ray particles by ionization and subsequent spark.

Hence the Crab has been used ’actively’ for the calibration assuming stability.

INTEGRAL spends two times 3 days per year observing the Crab.

The standard analysis software (OSA, issued by ISDC) for JEM-X analysis has a correction for Crab intensity variations.

So where are we now?

2011-04-11 IACHEC Meeting #6 5 DTU Space, Technical University of Denmark

JMX1 shadowgram revolutions 311 – 497, 12 – 25 keV Progression of anode deterioration

2011-04-11 IACHEC Meeting #6 6 DTU Space, Technical University of Denmark

JEM-X1 “Good” Regions

2011-04-11 IACHEC Meeting #6 7 DTU Space, Technical University of Denmark

JEM-X1 Spectrum

2011-04-11 IACHEC Meeting #6 8 DTU Space, Technical University of Denmark

2011-04-11 IACHEC Meeting #6 9 DTU Space, Technical University of Denmark

2011-04-11 IACHEC Meeting #6 10 DTU Space, Technical University of Denmark

An unexpected feature has become visible – some counts seem to

be lost, not only to dead-time effects

Schematic of snapshot in time Zoomed version

Particles

X rays

2011-04-11 IACHEC Meeting #6 11 DTU Space, Technical University of Denmark

Particle count rate as function of INTEGRAL orbit number

Slope: as function of orbit number as function of background rate

2011-04-11 IACHEC Meeting #6 12 DTU Space, Technical University of Denmark

2011-04-11 IACHEC Meeting #6 13 DTU Space, Technical University of Denmark

2011-04-11 IACHEC Meeting #6 14 DTU Space, Technical University of Denmark

2011-04-11 IACHEC Meeting #6 15 DTU Space, Technical University of Denmark

2011-04-11 IACHEC Meeting #6 16 DTU Space, Technical University of Denmark

Conclusion:

An unexpected ”deadtime” has been discovered.

Further analysis of the phenomenon will be initiated

Better calibration source count rate determination (runs for a long time)