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
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.
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 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 |
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.
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)