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The Fermi/LAT Collaboration organized a multiwavelength campaign to monitor the radio-loud narrow-line Seyfert 1 quasar PMN J0948+0022, already detected at gamma-rays by LAT (Bright Source List; Bright AGN List; plus a dedicated LAT paper published on ApJ).
The observing campaign is now closed
The reference period is 26 March - 5 July 2009
Present coverage and status of the data analysis.
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 |
OK |
Optical/NIR |
B, R, J |
SMARTS/Yale |
C. Bailyn, E.W. Bonning, M.Buxton, J. Isler, C. M. Urry |
OK |
NIR |
J, H, Ks |
INAOEP |
L. Carrasco, E. Recillas, A. Carraminana |
OK |
NIR |
J, K |
WIRO |
J. Bonnell, R. Canterna, A. Kutyrev, D. Macomb, J. Norris |
OK |
Radio |
15 GHz |
OVRO |
W. Max-Moerbeck, V. Pavlidou, T. J. Pearson, A. C. S. Readhead, J. L. Richards, M. Stevenson |
OK |
Radio |
cm/mm, Polarization |
Effelsberg |
L. Fuhrmann, J. A. Zensus, I. Nestoras, E. Angelakis, T. P. Krichbaum, N. Marchili |
OK |
Radio |
1-22 GHz |
RATAN-600 |
Y.Y. Kovalev, Yu.A. Kovalev |
OK |
Radio |
15 GHz, Polarization |
MOJAVE |
Y.Y. Kovalev, M.L. Lister, A.B. Pushkarev |
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 |
OK |
Radio |
37 GHz |
Metsahovi |
A. Lahteenmaki, M. Tornikoski, J. Tammi |
OK |
Swift schedule:
- 1st: 26 March 2009
- 2nd: 15 April 2009
- 3rd: 5 May 2009
- 4th: 10 May 2009
- 5th:15 May 2009
- 6th: 25 May 2009
- 7th: 4 June 2009
- 8th:14 June 2009
- 9th: 23 June 2009
It appears that we can benefit of some more snapshots:
- 10th: 24 June 2009
- 11th: 3 July 2009
Contact: Luigi Foschini (luigi.foschini@brera.inaf.itor foschini@merate.mi.astro.it)
Data format and deadline to participate to the paper in preparation:
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 (expired)