Spectroscopic follow-up of flaring blazars from CRTS
ATel #1952; A. A. Mahabal, S. G. Djorgovski, A. J. Drake, M. Graham, R. Williams, W. Max-Moerbeck, J. Richards (Caltech), A. Myers (UIUC), G. Pooley (Cavendish Lab, Cambridge), V. Mohan, A. N. Ramaprakash, A. Kembhavi, G. Devangan (IUCAA), E. Beshore, S. M. Larson, A. Boattini (UA/LPL), E. Christiansen (Gemin Obs.)
on 6 Mar 2009; 07:55 UT
Credential Certification: Ashish Mahabal (aam@astro.caltech.edu)
Subjects: Radio, Optical, AGN, Quasar, Transient, Variables
We report spectroscopic observations using the Double Beam Spectrograph at the
Palomar 200-inch telescope of three transients from Catalina Sky Survey.
The observations were carried out on 25 Feb 2009 UT.
As reported in ATEL #1890, CSS090102:112403+233646 is a known radio source. We
will separately report the radio monitoring of it. The redshift was determined
using Ly-alpha and C IV lines.
CSS090120:085010-121335 is known to have gone through phases of optical
flaring before (1997IAUC.6639B...1H)
We also have additional radio epochs for CSS090214:101052-020020. Those data
will be updated at the links given below.
The discovery data, CSS lightcurve and finding charts for these sources are
posted at the following VOEventNet webpages:
http://voeventnet.caltech.edu/feeds/ATEL/CRTS/901021230574116817.atel.html
http://voeventnet.caltech.edu/feeds/ATEL/CSS/902140010554111683.atel.html
http://voeventnet.caltech.edu/feeds/ATEL/CSS/901200120474150650.atel.html