Published data for cataclysmic variables


 

The data available here have been presented in my papers on cataclysmic variables. The photometric observations are presented as text files containing HJD (sometimes minus 2400000) and differential magnitude (warning: some light curves are not given in HJD but in JD with the heliocentric correction given in the second column). The spectroscopy is presented in the native format of the spectral reduction, analysis and storage package I use, molly, written by Tom Marsh. Please contact me if you would like spectra in other formats (ascii, FITS).

VLT spectroscopy of CVs discovered by the SDSS
The intermediate polar SDSS J233325.92+152222.1
Spectra of the quasar KUV 23182+1229 and white dwarf KUV 23061+1007
Orbital periods of CVs identified by the SDSS. II. Six objects
Orbital periods of CVs identified by the SDSS. IV. SDSS J220553.98+115553.7

 


 

VLT spectroscopy of cataclysmic variables discovered by the Sloan Digital Sky Survey

These data are described in Southworth et al. (2006, MNRAS, 373, 687).

Type of data Files Number of observations
SDSS J023322.61+005059.5 spectra VLT Hβ, WHT/ISIS blue arm, WHT/ISIS red arm, SDSS spectrum 38 (VLT), 34 (blue), 31 (red)
SDSS J023322.61+005059.5 photometry INT (g filter), LT (g filter), SDSS spectrum 299 (INT), 193 (LT)
SDSS J091127.36+084140.7 spectra VLT Hα, SDSS spectrum 42 (VLT)
SDSS J093238.21+010902.5 spectra VLT Hα, SDSS spectrum 9 (VLT)
SDSS J101037.05+024914.9 spectra VLT Hα, SDSS spectrum 5 (VLT)
SDSS J103533.02+055158.3 spectra VLT Hα, SDSS spectrum 58 (VLT)
SDSS J121607.03+052013.9 spectra VLT Hα, SDSS spectrum 41 (VLT)

The INT, WHT and LT (Liverpool Telescope) data were taken by various members of the University of Warwick astrophysics group as part of the 2004 International Time Project at La Palma.

 


 

SDSS J233325.92+152222.1 and the evolution of intermediate polars

These data are described in Southworth et al. (2007, MNRAS, 378, 635).

Type of data Files Number of observations
SDSS J233325.92+152222.1 spectra WHT/ISIS blue arm, WHT/ISIS red arm, SDSS spectrum 38 (WHT/ISIS blue and red arms)
SDSS J233325.92+152222.1 photometry Calar Alto (unfiltered) 293

These data were taken as part of a collaborative effort by various members of the University of Warwick astrophysics group.

 


 

KUV 23182+1229 and KUV 23061+1007

KUV 23182+1229 was investigated as a possible ultra-compact binary due to apparent helium II emission at 4686 Å in an old classification spectrum. KUV 23061+1007 was also observed because the authors of the original paper managed to get completely confused between the two objects.

It turns out that KUV 23182+1229 is a quasar at a redshift of 0.665, and the emission near 4680 Å is actually due to the magnesium 2800 Å quasar feature. As expected, KUV 23061+1007 is a bog-standard white dwarf of type DA. These results were published in Southworth et al. (2007, IBVS, 5775).

Type of data Files Number of observations
KUV 23182+1229 spectra molly file 2
KUV 23182+1229 combined spectrum data file 1
KUV 23061+1007 spectrum molly file   and   data file 1

 


 

Orbital periods of cataclysmic variables identified by the SDSS. II. Measurements for six objects, including two eclipsing systems

These data are described in Southworth et al. (2007, MNRAS, 382, 1145).

Type of data Files Number of observations
SDSS J005050.88+000912.6 photometry WHT (g filter), SDSS spectrum 355 datapoints
SDSS J013132.39-090122.2 spectra WHT/ISIS blue arm, WHT/ISIS red arm, SDSS spectrum 38 spectra
SDSS J075443.01+500729.2 photometry NOT (unfiltered), SDSS spectrum 1127 datapoints
SDSS J155531.99-001055.0 photometry INT (unfiltered), SDSS spectrum 233 datapoints
SDSS J165658.12+212139.3 photometry INT (unfiltered), SDSS spectrum 171 datapoints
SDSS J205914.87-061220.4 spectra WHT/ISIS blue arm, WHT/ISIS red arm, SDSS spectrum 38 spectra
SDSS J210449.94+010545.8 photometry WHT (g filter), SDSS spectrum 375 datapoints

The INT, WHT and NOT data were taken by various members of the University of Warwick astrophysics group as part of the 2004 International Time Project at La Palma.

 


 

Orbital periods of cataclysmic variables identified by the SDSS. IV. SDSS J220553.98+115553.7 has stopped pulsating

These data are described in Southworth, Townsley & Gänsicke (2008, MNRAS, 388, 709).

Type of data Files Number of observations
SDSS J220553.98+115553.7 VLT spectroscopy VLT/FORS2 spectra 37 spectra
SDSS J220553.98+115553.7 SDSS spectrum SDSS spectrum 1 spectrum
SDSS J220553.98+115553.7 NTT photometry NTT/SUSI2 (unfiltered) 852 datapoints

 


 

 


 

 


Last modified: 2014/11/11           John Southworth   (Keele University, UK)