General information

Table creation/update:  Sat Jul 18 20:27:52 2009 (D.Paneque, dpaneque@slac.stanford.edu)

Start of campaign:  2008/09/20

End of campaign:  2008/11/5

Instruments involved:  Effelsberg, Fermi, GASP, KANATA, MAGIC, MITsuME, RATAN-600, RXTE, Swift, Suzaku, VLBA, VERITAS, Whipple

Home Web addresses of the instruments involved in the campaign

Effelsberg:  http://www.mpifr-bonn.mpg.de/div/effelsberg/index_e.html

Fermi:  http://www-glast.stanford.edu/index.html

GASP:  http://www.to.astro.it/blazars/webt/

Kanata:  http://hasc.hiroshima-u.ac.jp/instruments/summary.html

MAGIC:  http://wwwmagic.mppmu.mpg.de/

MITsuME:  http://www.hp.phys.titech.ac.jp/mitsume/index.html

Medicina:  http://www.med.ira.inaf.it/index_EN.htm

RATAN-600:  http://www.sao.ru/ratan/

RXTE:  http://heasarc.gsfc.nasa.gov/docs/xte/rxte.html

SWIFT:  http://heasarc.gsfc.nasa.gov/docs/swift/swiftsc.html

Suzaku:  http://www.astro.isas.ac.jp/suzaku/

VLBA:  http://www.vlba.nrao.edu/

VERITAS:  http://veritas.sao.arizona.edu/

Whipple:  http://veritas.sao.arizona.edu/content/blogsection/6/40/

REMARKS

General:  The fluxes on this table are preliminary and cannot be used in publications. The purpose of making this information available is to provide an overall (quick) status of the activity of the source during the campaign. A more reliable and optimized analysis will be peformed at the end of the campaign.

Fermi fluxes:  The fluxes displayed correspond to groups of 5-6 MJD days centered at the RXTE observations. Fluxes with TS<16 are not displayed. During MJD [54559-54561] Fermi detected a flux increase by a factor ~3 at E>1 GeV (with respect to the typical fluxes during the MW. This flux increase is not that visible in this plot, where the flaring days are included in the (twice larger) bin [54959.5-54966]

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