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  The Fermi/LAT team is organizing a multi-wavelength campaign on the blazar (FSRQ) 3C279 (z=0.536) starting at the end of January and finishing at the middle of March, including various satellites (IR to gamma-ray) and ground-based Chrenkov telescopes for VHE gamma-ray.

We stronglly encourage any multi-wavelength observations from radio to TeV to obtain the broad band SED throughout the period.

 Observation Schedule

X-ray observations:

Suzaku

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- 200 ks deep observation

  • 2009-01-19 January 23:19 - 2009-01-22 January 22:32
  • 2009-01-23 January 21:00 - 2009-01-25 January 03:00

RXTE

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- monitring observaition

  • Wiki Markup
    \~2ks per obs  every other day since 26 December 2008 (thourgh March) \[[observation schedule (weekly)|http://heasarc.gsfc.nasa.gov/docs/xte/SOF/Schedules/index.phphttp://heasarc.gsfc.nasa.gov/docs/xte/SOF/Schedules/index.php]\]

XMM

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  • From 2009-01-21T16:48:01 (Rev. 1670)

INTEGRAL

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  • 2009-01-21 20:34:11 .0  - 2009-01-21 21:27:31 (3.2ks) 
  • 2009-01-21 21:56:02 .0  - 2009-01-22 12:40:59 (51.2ks) 
  • 2009-01-22 13:30:00 .0  - 2009-01-22 20:51:14 (25.6ks)
  • 2009-01-22 21:58:00 .0  - 2009-01-23 04:23:27 (22.4ks) 
  • 2009-01-26 14:14:32 - 2009-01-27 06:48:57 (57.6 ks)

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"). 

LAT news

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