Orbital periods of cataclysmic variables identified by the SDSS - VII. Four new eclipsing systems

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Volume 510 (February 2010)

A&A, 510 (2010) A100

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Table 1:

Full names, references and SDSS *ugriz* apparent magnitudes of our targets.
SDSS name	Short name	Reference	u	g	r	i	z	$g_{\rm spec}$
SDSS J031051.66-075500.2	SDSS J0310	Szkody et al. (2003)	15.76	15.49	15.74	15.89	16.10	22.03
SDSS J074355.55+183834.8	SDSS J0743	Szkody et al. (2006)	20.11	20.07	19.29	18.78	18.61	21.66
SDSS J074640.61+173412.7	SDSS J0746	Szkody et al. (2006)	18.21	18.16	18.37	18.52	18.55	21.20
SDSS J075059.97+141150.1	SDSS J0750	Szkody et al. (2007)	19.20	19.09	18.98	18.79	18.58	18.83
SDSS J075808.81+104345.5	SDSS J0758	Szkody et al. (2009)	17.06	16.92	17.07	17.17	17.25	17.06
SDSS J090628.24+052656.9	SDSS J0906	Szkody et al. (2005)	18.82	18.76	18.46	18.10	17.82	19.32
SDSS J092444.48+080150.9	SDSS J0924	Szkody et al. (2005)	19.49	19.25	19.26	18.70	17.88	19.36
SDSS J115207.00+404947.8	SDSS J1152	Szkody et al. (2007)	19.22	19.26	19.15	19.13	19.00	19.56
SDSS J152419.33+220920.1	SDSS J1524	Szkody et al. (2009)	19.04	19.04	18.90	18.80	18.50	19.52

Notes. $g_{\rm spec}$ is an apparent magnitude calculated by convolving the SDSS flux-calibrated spectra with the g passband function. These represent a different epoch to the SDSS ugriz magnitudes, but may be affected by ``slit losses'' due to any errors in astrometry or positioning of the fibre entrance.

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