Swift/XRT follow-up observation of IGR J12131+0700 (not NGC 4180)

Details Swift/XRT follow-up observation of IGR J12131+0700 (not NGC 4180) Swift/XRT follow-up observation of IGR J12131+0700 (not NGC 4180)

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1310....1l&link_type=abstract

The Astronomer's Telegram, #1310

Astronomy and Astrophysics

Astronomy

1

X-Ray, Gamma Ray, Agn

Scientific paper

IGR J12131+0700 (not NGC 4180) The third IBIS survey contains a source at RA(J2000) = 183.291 and Dec(J2000) = +7.009, initially associated to the galaxy NGC 4180, which has been recently classified as a possible Seyfert 2 galaxy (Masetti et al. 2007, Atel 1033). Swift/XRT has now observed this sky region for 4.6 ksec and detected within the IBIS uncertainty (5.1 arcmin), two sources at: 1) RA(J2000) = 12h 12m 49.62s, Dec(J2000) = +06d 59s 44.6s (5.1 arcsec uncertainty, 5.3 sigma) 2) RA(J2000) = 12h 12m 56.60s, Dec(J2000) = +07d 03s 06.7s (6 arcsec uncertainty, 3.6 sigma) Object N.1 coincides with the QSO SDSS J121249.84+065945.4 (also NVSS J121249+065950) at z = 0.2095 and has a 2-10 keV flux of 1.5 x 10-13 erg cm-2 s-1 (Gamma = 1.8).

Affiliated with

Also associated with

No associations

Rating

Swift/XRT follow-up observation of IGR J12131+0700 (not NGC 4180) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Swift/XRT follow-up observation of IGR J12131+0700 (not NGC 4180), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Swift/XRT follow-up observation of IGR J12131+0700 (not NGC 4180) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-737220