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This is a public page, open to people external to the LAT Collaboration.

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

Received, OK

Optical/NIR

B, R, J

SMARTS/Yale

E. W. Bonning, C. Bailyn, M.Buxton, P.Coppi, J. Isler, A.Kaptur, M. Urry, L. Maraschi, G. Fossati

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

W. Max-Moerbeck, V. Pavlidou, T. J. Pearson, A. C. S. Readhead, J. L. Richards, M. Stevenson

Received, OK

Radio

cm/mm, Polarization

Effelsberg

L. Fuhrmann, J. A. Zensus, I. Nestoras, E. Angelakis, T. P. Krichbaum, N. Marchili

Received, OK

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.

Not received (yet?)

Swift schedule:

It appears that we can benefit of some more snapshots:

Contact: Luigi Foschini (luigi.foschini@brera.inaf.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

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