Outburst from SS 433 observed with BOOTES-2/COLORES
ATel #6385; M. D. Caballero-Garcia (CTU-FEL, Prague, CZ), A. Castro-Tirado (IAA-CSIC, Spain), M. Jelinek (IAA-CSIC, Spain), on behalf of a larger collaboration.
on 12 Aug 2014; 09:59 UT
Credential Certification: Maria D. Caballero-Garcia (mcaballe@brera.inaf.it)
Subjects: Optical, X-ray, Binary, Black Hole
In light of the recent extreme outburst of SS 433 (ATELs #6347, #6355) and
follow-up by SWIFT (ATEL #6364) the 0.6m TELMA robotic telescope at the
BOOTES-2 (+COLORES) astronomical station in Malaga (Spain), obtained optical
4000-9000 A spectra starting at 2014-08-01 and ending at 2014-08-07.
The most prominent feature of the spectra is the variable H alpha line.
There is also a variable emission line at 7100 A that might be a 300 A
shifted H alpha Pfund line (7460 A), previously reported in the literature
(Fuchs, Miramon & Abraham, 2006).
Photometric daily measurements from BOOTES-2 (in SDSS r and i filters) are
given in the following:
r filter :
1406931041. 1.185651 12.36425 0.008
1407017454. 1.182885 11.8165 0.006
1407098707. 1.323325 12.306 0.008
1407372395. 1.41157 12.43675 0.012
i filter:
1406931063. 1.185651 11.0045 0.006
1407017476. 1.182885 10.356 0.007
1407098729. 1.320411 10.807 0.006
1407372417. 1.41157 10.97925 0.007
where the format is Obs. time (seconds since 1970/01/01), airmass, r/i
magnitude and error in r/i magnitude. These measurements indicate that
the source is returning to quiescence (this source has a quiescent level
of 12.65, 11.27 magnitudes in the Johnson R and I filters, respectively).
This is in agreement with results from UVOT/SWIFT (ATEL #6364).
Continuous monitoring of this source with BOOTES-2 is ongoing.