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| 2MASS J23375921+4308509 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:29:37 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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. | |||||
|
2006AJ....132..663B |
48 | 104 | A survey for spectroscopic binaries among very low mass stars. | BASRI G. and REINERS A. | |||||
|
2008NewA...13..133A |
15 | D | 459 | 29 | Spatial distribution and galactic model parameters of cataclysmic variables. | AK T., BILIR S., AK S., et al. | |||
|
2009ApJS..184..138H |
15 | D | 1 | 20623 | 68 | XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. | HAAKONSEN C.B. and RUTLEDGE R.E. | ||
|
2010A&A...524A..64C |
15 | D | 1 | 1294 | 157 | The Palermo Swift-BAT hard X-ray catalogue. III. Results after 54 months of sky survey. | CUSUMANO G., LA PAROLA V., SEGRETO A., et al. | ||
| 2017A&A...602A.124R | 100 | 9 | The nature of 50 Palermo Swift-BAT hard X-ray objects through optical spectroscopy. | ROJAS A.F., MASETTI N., MINNITI D., et al. | |||||
|
2018AJ....156..231W |
1445 | T A | D | S X C | 34 | 6 | ~ |
An optical study of two VY Sculptoris-type cataclysmic binary stars: V704 And and RX J2338+431. |
WEIL K.E., THORSTENSEN J.R. and HABERL F. |
|
2019A&A...621A..38G |
16 | D | 1 | 39805 | 85 | The population of hot subdwarf stars studied with Gaia. II. The Gaia DR2 catalogue of hot subluminous stars. | GEIER S., RADDI R., GENTILE FUSILLO N.P., et al. | ||
|
2020MNRAS.492L..40A |
16 | D | 1 | 1220 | 31 | Disentangling cataclysmic variables in Gaia's HR diagram. | ABRIL J., SCHMIDTOBREICK L., EDEROCLITE A., et al. | ||
|
2021ApJS..256...28L |
17 | D | 1 | 2206 | 16 | Hot subdwarf atmospheric parameters, kinematics, and origins based on 1587 hot subdwarf stars observed in Gaia DR2 and LAMOST DR7. | LUO Y., NEMETH P., WANG K., et al. | ||
|
2021ApJS..257...65S |
17 | D | 1 | 328 | 5 | A catalog of 323 cataclysmic variables from LAMOST DR6. | SUN Y., CHENG Z., YE S., et al. | ||
|
2022ApJ...928...20B |
17 | D | 2 | 1219 | 10 | New Variable Hot Subdwarf Stars Identified from Anomalous Gaia Flux Errors, Observed by TESS, and Classified via Fourier Diagnostics. | BARLOW B.N., CORCORAN K.A., PARKER I.M., et al. | ||
|
2022A&A...662A..40C |
17 | D | 1 | 62976 | 9 | The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3. | CULPAN R., GEIER S., REINDL N., et al. | ||
|
2023ApJS..264...17Z |
17 | D | 1 | 31380 | 1 | Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. | ZHANG L.-Y., SU T., MISRA P., et al. | ||
|
2023AJ....165..148H |
17 | D | 2 | 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. | ||
| 2023A&A...679L...3Z | 17 | D | 1 | 30 | ~ | A trio of month-long flares in the nova-like variable V704 And. | ZSIDI G., NIXON C.J., NAYLOR T., et al. | ||
| 2024MNRAS.535.3035D | 779 | D | S X C F | 15 | 28 | ~ | Characterizing high and low accretion states in VY Scl CVs using ZTF and TESS data. | DUFFY C., WU K., RAMSAY G., et al. | |
|
2025A&A...693A.268R |
19 | D | 1 | 581 | ~ | Variability in hot sub-luminous stars and binaries: Machine-learning analysis of Gaia DR3 multi-epoch photometry. | RANAIVOMANANA P., UZUNDAG M., JOHNSTON C., et al. | ||
| 2025ApJ...984....9Z | 19 | D | 1 | 108 | ~ | Searching for Accreting Compact Binary Systems from Spectroscopy and Photometry: Application to LAMOST Spectra. | ZHAO X., WANG S. and LIU J. |