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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

OK

Optical/NIR

B, R, J

SMARTS/Yale

C. Bailyn, E.W. Bonning, M.Buxton, J. Isler, C. M. Urry

Received, OK

NIR

J, H, Ks

INAOEP

L. Carrasco, E. Recillas, A. Carraminana

Received, OK

NIR

J, K

WIRO

J. Bonnell, R. Canterna, A. Kutyrev, D. Macomb, J. Norris

Received, OK

Radio

15 GHz

OVRO

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

OK

Radio

cm/mm, Polarization

Effelsberg

L. Fuhrmann & , J. A. Zensus, I. Nestoras, E. Angelakis
Waiting, T. P. . Seen some preview Krichbaum, N. Marchili

OK

Radio

1-22 GHz

RATAN-600

Kovalev et al.

Waiting...

Y.Y. Kovalev, Yu.A. Kovalev

OK

Radio

15 GHz, Polarization

MOJAVE

Y.Y. Kovalev, M.L. Lister, A.B. Pushkarev

OK Received, checking

Radio

1.66, 22.2 GHz

e-VLBI

Giroletti et al.

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 Waiting... Seen some preview

Radio

37 GHz

Metsahovi

Lahteenmaki et al.

A. Lahteenmaki, M. Tornikoski, J. Tammi

OK Waiting...

Swift schedule:

...

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)