SDSS J115207.00+404947.9 , the SIMBAD biblio

SDSS J115207.00+404947.9 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST15:07:16


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Title First 3 Authors
2007AJ....134..185S viz 16       D               27 71 Cataclysmic variables from Sloan Digital Sky Survey. VI. The sixth year (2005). SZKODY P., HENDEN A., MANNIKKO L., et al.
2009MNRAS.397.2170G 15       D               1 154 238 SDSS unveils a population of intrinsically faint cataclysmic variables at the minimum orbital period. GANSICKE B.T., DILLON M., SOUTHWORTH J., et al.
2010A&A...510A.100S viz 725     A D     X C       19 11 12 Orbital periods of cataclysmic variables identified by the SDSS. VII. Four new eclipsing systems. SOUTHWORTH J., COPPERWHEAT C.M., GAENSICKE B.T., et al.
2011MNRAS.415.2025S 846     A D S   X C F     20 17 65 Cataclysmic variables below the period gap: mass determinations of 14 eclipsing systems. SAVOURY C.D.J., LITTLEFAIR S.P., DHILLON V.S., et al.
2011A&A...536A..42Z 16       D               1 97 224 Post common envelope binaries from SDSS. XI. The white dwarf mass distributions of CVs and pre-CVs. ZOROTOVIC M., SCHREIBER M.R. and GAENSICKE B.T.
2012PASJ...64...63K viz 15       D               1 322 10 Characterization of dwarf novae using SDSS colors. KATO T., MAEHARA H. and UEMURA M.
2012AJ....144...81T viz 15       D               1 337 25 Spectroscopy and photometry of cataclysmic variable candidates from the Catalina Real Time Survey. THORSTENSEN J.R. and SKINNER J.N.
2013A&A...554A..25M viz 78           X         2 9 3 Photometry of the eclipsing cataclysmic variable SDSS J152419.33+220920.0. MICHEL R., ECHEVARRIA J. and HERNANDEZ SANTISTEBAN J.V.
2013PASJ...65..115K 39           X         1 53 44 New method of estimating binary's mass ratios by using superhumps. KATO T. and OSAKI Y.
2015ApJ...812...40G viz 16       D               1 38 64 Adiabatic mass loss in binary stars. II. From zero-age main sequence to the base of the giant branch. GE H., WEBBINK R.F., CHEN X., et al.
2016MNRAS.460.2526O viz 16       D               1 638 28 Statistical analysis of properties of dwarf novae outbursts. OTULAKOWSKA-HYPKA M., OLECH A. and PATTERSON J.
2017MNRAS.464.1353M 41           X         1 9 8 Using Gaussian processes to model light curves in the presence of flickering: the eclipsing cataclysmic variable ASASSN-14ag. McALLISTER M.J., LITTLEFAIR S.P., DHILLON V.S., et al.
2017MNRAS.465.4968H viz 57       D     X         2 79 12 Hunting for eclipses: high-speed observations of cataclysmic variables. HARDY L.K., McALLISTER M.J., DHILLON V.S., et al.
2017PASJ...69...75K viz 97       D S             2 98 34 Survey of period variations of superhumps in SU UMa-type dwarf novae. IX. The ninth year (2016-2017). KATO T., ISOGAI K., HAMBSCH F.-J., et al.
2019A&A...622A..60C viz 17       D               1 150347 194 Gaia Data Release 2. Specific characterisation and validation of all-sky Cepheids and RR Lyrae stars. CLEMENTINI G., RIPEPI V., MOLINARO R., et al.
2019MNRAS.486.2169K viz 17       D               1 25030 80 White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 14. KEPLER S.O., PELISOLI I., KOESTER D., et al.
2019MNRAS.486.5535M viz 351       D     X         9 54 41 The evolutionary status of Cataclysmic Variables: eclipse modelling of 15 systems. McALLISTER M., LITTLEFAIR S.P., PARSONS S.G., et al.
2020MNRAS.491.5717B viz 17       D               1 202 34 Evidence for reduced magnetic braking in polars from binary population models. BELLONI D., SCHREIBER M.R., PALA A.F., et al.
2020MNRAS.492L..40A viz 17       D               1 1220 31 Disentangling cataclysmic variables in Gaia's HR diagram. ABRIL J., SCHMIDTOBREICK L., EDEROCLITE A., et al.
2021ApJ...914....5S viz 104       D       C       2 206 8 Nova-produced common envelope: source of the nonsolar abundances and an additional frictional angular momentum loss in cataclysmic variables. SPARKS W.M. and SION E.M.
2021MNRAS.508.3877G viz 17       D               2 451937 102 A catalogue of white dwarfs in Gaia EDR3. GENTILE FUSILLO N.P., TREMBLAY P.-E., CUKANOVAITE E., et al.

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