Period: January 19th to March 17th in 2009
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
...
- 200
...
ksec 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
...
- monitring observaition
...
- \~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 2009-01-21T16:48:01 (Rev. 1670)
...
- per obs every other day since 26 December 2008 (thourgh March) [observation schedule (weekly)]
XMM
- 2009-01-21 16:48:01 - 2009.01.22. 00:38:01 (~28.2 ksec)
INTEGRAL
- 2009-01-21 20:34:11 .0 - 2009-01-21 21:27:31 (3.2ks2 ksec)
- 2009-01-21 21:56:02 .0 - 2009-01-22 12:40:59 (51.2ks2 ksec)
- 2009-01-22 13:30:00 .0 - 2009-01-22 20:51:14 (25.6ks6 ksec)
- 2009-01-22 21:58:00 .0 (22.4ks)
Optical band
- - 2009-01-23 04:23:27 (22.4 ksec)
- 2009-01-26 14:14:32 - 2009-01-27 06:48:57 (57.6 ksec)
Optical band:
- current optical status : recent 30 days (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.
Wiki Markup
LAT news
- Fermi/LAT Automated Science Processing public data: HEASARC Browse
...