Microcalorimeter array development for X-ray astronomy

Details Microcalorimeter array development for X-ray astronomy Microcalorimeter array development for X-ray astronomy

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nimpa.504..339p&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 504, Issue 1-3, p. 339-342.

Physics

1

Scientific paper

A development of X-ray sensitive microcalorimeter arrays is presently being undertaken to provide a spectroimager of high-energy resolution which could fit the focal plane of the X-ray astronomy spatial missions of the new generation (ESLAB 1999/093/SA).
The infrared-sensitive arrays which have been realized at LETI in collaboration with the SAp, for the PACS experiment on board the Herschel satellite (Proceedings of the SPIE Conference of Orlando, 5-9 April 1999, 3698-38), are taken as the basis of this development which will rely conservatively on standard technology.

Affiliated with

Also associated with

No associations

Rating

Microcalorimeter array development for X-ray astronomy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Microcalorimeter array development for X-ray astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Microcalorimeter array development for X-ray astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1470535