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The Fermi/LAT team is organizing a multi-wavelength campaign on the blazar (FSRQ) 3C279 starting at the end of January and finishing at the middle of March.
We encourage observation , including variaous satelistes (IR to gamma-ray). We encourage multi-wavelength observations in any energy bands from radio to TeV to cover obtain the broad band SED throughout the period.
Observation Schedule
X-ray observations
Suzaku : 200 ks deep observation
- 19 January 23:19 - 22 January 22:32
- 23 January 21:00 - 25 January 03:00
RXTE : monitring observaition
- ~2ks per obs every other days since 26 December 2008 (thoughr March)
XMM :
- From 2009-01-21T16:48:01 (Rev. 1670)
INTEGRAL :
- 2009-01-21 20:34:11.0 (3.2ks)
- 2009-01-21 21:56:02.0 (51.2ks)
- 2009-01-22 13:30:00.0 (25.6ks)
- 2009-01-22 21:58:00.0 (22.4ks)
Optical band
Wiki Markup current optical status : [recent 30 days|http://users.utu.fi/kani/1m/3C_279_l.png] (by KVA \[La Palma\] and the Tuorla telescope \[Finland\] under "the Tuorla Blazar monitoring program").
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- Fermi/LAT Automated Science Processing public data: HEASARC Browse
- ATEL (#1864)
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| Wiki Markup |
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\[ internal page\|https://confluence.slac.stanford.edu/display/SCIGRPS/PIC+MWL+observations+(Jan-Mar+2009)\] |
Source Informaion
- (RA, Dec: J2000) = (12h56m11.1s -05d47m22s), z=0.53620
- Multi-wavelength SED
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