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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 - 200
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ksec deep observation
- 2009-01-19 23:19 - 2009-01-22 22:32
- 2009-01-23 21:00 - 2009-01-25 03:00
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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
- From 2009-01-21T1621 16:48:01 (Rev. 1670- 2009.01.22. 00:38:01 (~28.2 ksec)
INTEGRAL
- 2009-01-21 20:34:11 - 2009-01-21 21:27:31 (3.2ks2 ksec)
- 2009-01-21 21:56:02 - 2009-01-22 12:40:59 (51.2ks2 ksec)
- 2009-01-22 13:30:00 - 2009-01-22 20:51:14 (25.6ks6 ksec)
- 2009-01-22 21:58:00 - 2009-01-23 04:23:27 (22.4ks4 ksec)
- 2009-01-26 14:14:32 - 2009-01-27 06:48:57 (57.6 ksksec)
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").
Infra-red band:
Spitzter
- ~ 1 hour observation each day
- MIPS: Feburay 15-20
- IRS : March 3-4
Radio band:
- Observations at the 32m Noto radio telescope (Italy) underway since January 20, roughly every 4 days until mid-February. Data are taken at 8 and 22 GHz.
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