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| V* HK Leo , the SIMBAD biblio (35 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:14:14 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
1986ApJS...61..305G |
1882 | 923 | The Palomar-Green catalog of ultraviolet-excess stellar objects. | GREEN R.F., SCHMIDT M. and LIEBERT J. | |||||
|
1991A&A...250..370B |
121 | 44 | A high galactic latitude survey of far-ultraviolet excess objects. | BIXLER J.V., BOWYER S. and LAGET M. | |||||
|
1993PASP..105..127D |
819 | 152 | A catalog and atlas of cataclysmic variables. | DOWNES R.A. and SHARA M.M. | |||||
| 1994A&AS..104...79B | 179 | 112 | A catalogue of UBV colours of cataclysmic variables. | BRUCH A. and ENGEL A. | |||||
| 1994A&AS..107..503Z | 59 | 36 | CCD spectrophotometry of CVs. I. 4600-9000A low resolution atlas for 31 faint systems. | ZWITTER T. and MUNARI U. | |||||
| 1995AJ....109.1757M | 1 | 12 | 55 | Time-resolved photometry of a sample of Palomar-Green cataclysmic variable candidates. | MISSELT K.A. and SHAFTER A.W. | ||||
|
1997PASP..109..345D |
1017 | 137 | A catalog and atlas of cataclysmic variables-second edition. | DOWNES R., WEBBINK R.F. and SHARA M.M. | |||||
|
1997PASP..109..441H |
2379 | 53 | Secondary photometric standards for northern cataclysmic variables and related objects. | HENDEN A.A. and HONEYCUTT R.K. | |||||
|
1997KFNT...13e..70R |
49738 | 3 | GPM - compiled catalogue of absolute proper motions of stars in selected areas of sky with galaxies. | RYBKA S.P. and YATSENKO A.I. | |||||
| 1999AcASn..40....1L | 20 | 5 | Spectroscopic identification for 20 cataclysmic variables or relative objects. | LI Z.-Y., LIU W. and HU J.-Y. | |||||
| 2000AJ....120.1113H | 108 | T K | 42 | 23 |
Post-common-envelope binary stars and the precataclysmic binary PG 1114+187. |
HILLWIG T.C., HONEYCUTT R.K. and ROBERTSON J.W. | |||
|
2001PASP..113..764D |
1714 | 277 | A catalog and atlas of cataclysmic variables: the living edition. | DOWNES R.A., WEBBINK R.F., SHARA M.M., et al. | |||||
| 2002AJ....124.2853K | 10 | 25 | Optical observations and orbital parameters of the close DA plus dMe binaries BPM 71214, EUVE J0720-31.7, BPM 6502, and EC 13471-1258. | KAWKA A., VENNES S., KOCH R., et al. | |||||
| 2002PASP..114..756H | 4 | 3 | The classification and orbital period of WD 2154+408: a new short-period Post-Common-Envelope binary. | HILLWIG T.C., GALE A.A., HONEYCUTT R.K., et al. | |||||
|
2004A&A...418..357K |
15 | D | 1 | 57785 | 7 | The Pul-3 catalogue of 58483 stars in the Tycho-2 system. | KHRUTSKAYA E.V., KHOVRITCHEV M.Y. and BRONNIKOVA N.M. | ||
|
2006IBVS.5721....1K |
1754 | 36 | The 78th name-list of variable stars. | KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al. | |||||
| 2006BSAO...59...34V | 50 | 1 | Precatalysmic binary systems. | VOICHANSKAYA N.F. | |||||
| 2011MNRAS.410.2095V | 53 | D | X | 2 | 173 | 54 | A selection of hot subluminous stars in the GALEX survey – I. Correlation with the guide star catalog. | VENNES S., KAWKA A. and NEMETH P. | |
| 2011AJ....142...62H | 38 | X | 1 | 13 | 13 | The Kepler light curve of the unique DA white dwarf BOKS 53856. | HOLBERG J.B. and HOWELL S.B. | ||
|
2011AJ....142..181S |
39 | A | D | X F | 1 | 36 | 83 | Cataclysmic variables from the Sloan Digital Sky Survey. VIII. The final year (2007-2008). | SZKODY P., ANDERSON S.F., BROOKS K., et al. |
|
2012AJ....144...81T |
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. | ||
|
2014ApJS..213....9D |
15 | D | 1 | 46794 | 385 | The Catalina surveys periodic variable star catalog. | DRAKE A.J., GRAHAM M.J., DJORGOVSKI S.G., et al. | ||
|
2015MNRAS.448.2260G |
16 | D | 1 | 32939 | 53 | A photometric selection of white dwarf candidates in Sloan Digital Sky Survey Data Release 10. | GENTILE FUSILLO N.P., GANSICKE B.T. and GREISS S. | ||
|
2016MNRAS.457.3396P |
16 | D | 1 | 437 | 3 | A search for new hot subdwarf stars by means of virtual observatory tools II. | PEREZ-FERNANDEZ E., ULLA A., SOLANO E., et al. | ||
|
2016yCat....1.2035M |
16 | D | 14271 | ~ | A Catalogue of Spectroscopically Identified White Dwarfs | MCCOOK G.P. and SION E.M. | |||
|
2017MNRAS.472.4173R |
16 | D | 1 | 2245 | 21 | Multiband photometry and spectroscopy of an all-sky sample of bright white dwarfs. | RADDI R., GENTILE FUSILLO N.P., PALA A.F., et al. | ||
|
2019MNRAS.482.4570G |
16 | D | 1 | 486646 | 296 | A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS. | GENTILE FUSILLO N.P., TREMBLAY P.-E., GANSICKE B.T., et al. | ||
|
2020AJ....159...43H |
16 | D | 2 | 182 | 17 | Spectroscopically identified cataclysmic variables from the LAMOST survey. I. The sample. | HOU W., LUO A.-L., LI Y.-B., et al. | ||
|
2021MNRAS.508.3877G |
17 | D | 1 | 451937 | 102 | A catalogue of white dwarfs in Gaia EDR3. | GENTILE FUSILLO N.P., TREMBLAY P.-E., CUKANOVAITE E., et al. | ||
|
2021ApJS..257...65S |
17 | D | 2 | 328 | 5 | A catalog of 323 cataclysmic variables from LAMOST DR6. | SUN Y., CHENG Z., YE S., et al. | ||
|
2022MNRAS.509.2674G |
17 | D | 2 | 3067 | 5 | White dwarfs identified in LAMOST Data Release 5. | GUO J., ZHAO J., ZHANG H., et al. | ||
|
2023AJ....165..148H |
409 | D | X C | 9 | 220 | 1 | Spectroscopically Identified Cataclysmic Variables from the LAMOST Survey. II. Period Estimates. | HOU W., LUO A.-L., DONG Y.-Q., et al. | |
|
2023AJ....165..163C |
17 | D | 1 | 1619 | ~ | Galactic Model Parameters and Spatial Density of Cataclysmic Variables in the Gaia Era: New Constraints on Population Models. | CANBAY R., BILIR S., OZDONMEZ A., et al. | ||
|
2023MNRAS.524.4867I |
17 | D | 1 | 545 | ~ | A catalogue of cataclysmic variables from 20 yr of the Sloan Digital Sky Survey with new classifications, periods, trends, and oddities. | INIGHT K., GANSICKE B.T., BREEDT E., et al. | ||
| 2024MNRAS.533..324L | 45 | X | 1 | 56 | ~ | Short-period post-common envelope binaries with Balmer emission from SDSS and LAMOST based on ZTF photometric data. | LI L. and ZHANG F. |