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| V* NX Cam , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST12:12:50 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2006PZP.....6...16K | 57 | 0 | New short periodic eclipsing binaries. | KHRUSLOV A.V. | |||||
2011IBVS.5969....1K 
|
15 | D | 1 | 2041 | 27 | The 80th name-list of variable stars. Part I - RA 0h to 6h. | KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al. | ||
| 2015IBVS.6152....1H | 507 | 40 | BAV-Results of observations - Photoelectric Minima of Selected Eclipsing Binaries and Maxima of Pulsating Stars. | HUBSCHER J. | |||||
|
2020RAA....20..163Q
|
16 | D | 1 | 8835 | 46 | Contact binaries at different evolutionary stages. | QIAN S.-B., ZHU L.-Y., LIU L., et al. | ||
|
2022ApJS..258...16P
|
17 | D | 1 | 4582 | 43 | TESS Eclipsing Binary stars. I. Short-cadence observations of 4584 eclipsing binaries in sectors 1-26. | PRSA A., KOCHOSKA A., CONROY K.E., et al. | ||
| 2022MNRAS.510.5315P | 17 | D | 2 | 125 | 10 | Investigation of the orbital period and mass relations for W UMa-type contact systems. | PORO A., SARABI S., ZAMANPOUR S., et al. | ||
|
2022PASP..134k4202G
|
17 | D | 1 | 77 | ~ | Photometric and Spectroscopic Studies of the Long-Period Low-Mass-Ratio Deep-Contact Binary KN Per. | GAO X.-Y., LI K., CAI Y.-W., et al. | ||
|
2023A&A...674A..16M
|
17 | D | 1 | 2184478 | 19 | Gaia Data Release 3 The first Gaia catalogue of eclipsing-binary candidates. | MOWLAVI N., HOLL B., LECOEUR-TAIBI I., et al. | ||
| 2024RAA....24a5002P | 18 | D | 1 | 141 | ~ | Two-dimensional Parameter Relationships for W UMa-type Systems Revisited. | PORO A., PAKI E., ALIZADEHSABEGH A., et al. | ||
|
2024AJ....167..192D
|
18 | D | 1 | 1374 | ~ | Detection of Contact Binary Candidates Observed By TESS Using the Autoencoder Neural Network. | DING X., SONG Z., WANG C., et al. | ||
| 2025ApJ...988...80D | 19 | D | 5 | 146 | ~ | Fundamental Parameters for Totally Eclipsing Contact Binaries Observed by TESS. | DING X., JI K., SONG Z., et al. |
