-
1
-
-
78751672618
-
-
Sensitivity curves are produced on data obtained either from the official web sites or conference presentations on the instrument or from the instrument headquarter. Atmospheric Cherenkov Telescopes traditionally use sensitivity for flux above E. The differential sensitivity curves given here has been calculated assuming a Crab-like spectrum. Note most curves are read out by eye of plots given below and can be off by 20-30%. • AstroE2-HXD (SiPIN+GSO)
-
Sensitivity curves are produced on data obtained either from the official web sites or conference presentations on the instrument or from the instrument headquarter. Atmospheric Cherenkov Telescopes traditionally use sensitivity for flux above E. The differential sensitivity curves given here has been calculated assuming a Crab-like spectrum. Note most curves are read out by eye of plots given below and can be off by 20-30%. • AstroE2-HXD (SiPIN+GSO): H. Soojing http://eaya2003.asiaa.sinica.edu.tw/pdf/hong-sj.pdf,
-
-
-
Soojing, H.1
-
2
-
-
78751679027
-
Integral Overview
-
Integral IBIS (ISGRI+PICsIT)
-
Integral IBIS (ISGRI+PICsIT): R. Diehl, "Integral Overview" Magic Physics 2002 Workshop,
-
Magic Physics 2002 Workshop
-
-
Diehl, R.1
-
3
-
-
78751678580
-
-
GLAST-LAT: http://www-glast.slac.stanford.edu/software/IS/glast-lat- performance.htm
-
-
-
-
4
-
-
78751668196
-
-
AGILE: http://agile.mi.iasf.cnr.it/Homepage/performances.shtml
-
-
-
-
5
-
-
78751676199
-
-
EGRET: Since there is no official sensitivity curve available, the author calculated based on the Crab observation (see the text). So admittedly not official and may lack accuracy
-
EGRET: Since there is no official sensitivity curve available, the author calculated based on the Crab observation (see the text). So admittedly not official and may lack accuracy.
-
-
-
-
6
-
-
78751658828
-
-
Magic: http://hegral.mppmu.mpg.de/MAGICWeb
-
Magic
-
-
-
7
-
-
84884638845
-
-
(in Japanese)
-
Cangaroo: http://icrhp9.icrr.u-tokyo.ac.jp/paper/C3.pdf (in Japanese)
-
Cangaroo
-
-
-
8
-
-
78751667884
-
-
HESS: http://www.mpi-hd.mpg.de/hfin/HESS/HESS.html
-
HESS
-
-
-
9
-
-
78751668929
-
-
The spectra of popular sources have been interpolated if experimental data are sparse or missing in a large portion of spectrum. Hence they are to be taken as crude references
-
Veritas: http://veritas.sao.arizona.edu/ The spectra of popular sources have been interpolated if experimental data are sparse or missing in a large portion of spectrum. Hence they are to be taken as crude references.
-
-
-
-
10
-
-
0035499959
-
-
Crab Nebula and Pulsar: [2]
-
• Crab Nebula and Pulsar: de Jager [2]; Kuiper, L., et al., 2001, A&A 378, 918;
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(2001)
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De Jager1
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Extragalactic Background (EXB)
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official website
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GLAST-LAT official website, http://www-glast.stanford.edu/
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Reviews in
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Reviews in http://www.physics.hku.hk/~2003conf/participants.html
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and astro-ph/0409104
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78751666860
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in preparation
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Kamae, T., et al., in preparation
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Astro E2 XRS Team, http://phonon.gsfc.nasa.gov/xrscal/SHI2004/index.html
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may provide such a possibility
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MAXI may provide such a possibility: http://www-maxi.tksc.nasda.go.jp/ indexe.html
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50
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0000659645
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See for example
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(southern sky pulsars) and astro-ph/0407546 (a milli-second pulsar)
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(southern sky pulsars) and Cognard, I., and Backer, D. C, astro-ph/0407546 (a milli-second pulsar)
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Cognard, I.1
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See also a cosmological analysis on them in
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See also a cosmological analysis on them in: Cooray, A. R., 1999, A&A 342, 353
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Cooray, A.R.1
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