View Source

Domain	Energy band/Filter/Frequency	Facility	Analyzer(s)	Status
Gamma-rays	0.1-10 GeV	Fermi/LAT	L. Foschini	OK
Hard X-rays	20-100 keV	Swift/BAT	L. Foschini	OK
X-rays	0.2-10 keV	Swift/XRT	L. Foschini	OK
Optical/UV	V,B,U,UVW1,UVM2,UVW2	Swift/UVOT	P. Roming, M. Stark, L. Foschini	OK
Optical	B,R	ATOM	S. Wagner, M. Hauser	Received, OK
NIR	J,H,Ks	INAOEP	L. Carrasco, E. Recillas, A. Carraminana	Received, OK
NIR	J, K	WIRO	J. Norris	Received, OK
Radio	15 GHz	OVRO	T. Readhead et al.	Waiting...
Radio	cm/mm, Polarization	Effelsberg	L. Fuhrmann & E. Angelakis	Waiting... Seen some preview
Radio	1-22 GHz	RATAN-600	Y.Y. Kovalev, Yu.A. Kovalev	Received, OK
Radio	15 GHz, Polarization	MOJAVE	Y.Y. Kovalev, M.L. Lister, A.B. Pushkarev	Received, OK
Radio	1.66, 22.2 GHz	e-VLBI	M. Giroletti, Z. Paragi, H. Bignall, C. Phillips, P. Edwards, J. Blanchard, A. Doi, M. Kino, H. Nagai, M. Sekido, H. J. van Langevelde, T. Tzioumis, A. Szomoru, X. Hong, F. Colomer, M. Kadler	Received, OK
Radio	37 GHz	Metsahovi	Lahteenmaki et al.	Waiting...

It appears that we can benefit of some more snapshots:

Data format:

Time: MJD
Frequency: Hz
Energy: eV or multiples (keV, MeV, GeV)
Fluxes (nuFnu): erg/cm2/s (or Jy*Hz, if easier)
Fluxes should be already corrected and dereddened (ground based observatories should correct also for the extinction due to the airmass). Use as reference AV=0.277 and the extinction laws of Cardelli et al. (1989).
Include also the observed magnitudes (for NIR/optical/UV data).
Inclued also some short text explaining the data analysis performed.
Include also the list of people (and their affiliations) to be included in the authors list.

Deadline to send data: 31 July 2009