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| 1SWASP J015100.23-100524.2 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST08:07:20 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013A&A...549A..86L |
15 | D | 1 | 154 | 69 | Period and period change measurements for 143 SuperWASP eclipsing binary candidates near the short-period limit and discovery of a doubly eclipsing quadruple system. | LOHR M.E., NORTON A.J., KOLB U.C., et al. | ||
|
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. | ||
| 2015AJ....150..117Q | 1404 | T K A | D | X C | 35 | 9 | 4 |
SuperWASP J015100.23-100524.2: a spotted shallow-contact binary below the period limit. |
QIAN S.B., ZHANG B., SOONTHORNTHUM B., et al. |
|
2017MNRAS.465.4678M |
16 | D | 1 | 9381 | 6 | Characterization of 9380 contact binaries from the CRTS Variable Sources Catalogue. | MARSH F.M., PRINCE T.A., MAHABAL A.A., et al. | ||
| 2017NewA...54...52B | 40 | X | 1 | 11 | 1 | 1SWASP J200503.05-343726.5: A high mass ratio eclipsing binary near the period limit. | BIN Z., SHENGBANG Q., ZEJDA M., et al. | ||
|
2018AJ....156..241H |
16 | D | 1 | 311106 | 199 | A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). | HEINZE A.N., TONRY J.L., DENNEAU L., et al. | ||
| 2019PASP..131c4201Z | 41 | X | 1 | 15 | 5 | A detached eclipsing binary with a period shorter than 0.2 days in a triple system. | ZHANG B., QIAN S.-B., ZHI Q.-J., et al. | ||
| 2018RAA....18...30Z | 80 | X | 2 | 15 | 7 | First photometric study of ultrashort-period contact binary 1SWASP J140533.33+114639.1. | ZHANG B., QIAN S.-B., MICHEL R., et al. | ||
| 2019MNRAS.485.4588L | 16 | D | 1 | 57 | 39 | Contact binaries at the short period cut-off - I. Statistics and the first photometric investigations of 10 totally eclipsing systems. | LI K., XIA Q.-Q., MICHEL R., et al. | ||
| 2019PASJ...71...21K | 122 | X C | 2 | 138 | 16 | Starspots in contact and semi-detached binary systems. | KOUZUMA S. | ||
|
2020ApJS..249...18C |
16 | D | 1 | 781605 | 122 | The Zwicky Transient Facility catalog of periodic variable stars. | CHEN X., WANG S., DENG L., et al. | ||
| 2020MNRAS.497.3493Z | 16 | D | 1 | 360 | 25 | Orbital period cut-off of W UMa-type contact binaries. | ZHANG X.-D. and QIAN S.-B. | ||
|
2021ApJS..254...10L |
17 | D | 1 | 694 | 37 | Statistics of 700 individually studied W UMa stars. | LATKOVIC O., CEKI A. and LAZAREVIC S. | ||
| 2021PASJ...73.1470S | 17 | D | 1 | 59 | ~ | BM UMa: A middle shallow contact binary at pre-transition stage of evolution from W-type to A-type. | SAROTSAKULCHAI T., SOONTHORNTHUM B., POSHYACHINDA S., et al. | ||
| 2022PASJ...74..326X | 43 | X | 1 | 11 | 1 | Red dwarf contact binary V0627 Hydrae. | XU H.-S., ZHU L.-Y., THAWICHARAT S., et al. | ||
| 2022RAA....22b5011Z | 43 | X | 1 | 10 | 1 | CSS J075415.6+191052 and NW Leo: Two Contact Binaries at Different Evolutionary Stages. | ZHANG X.-D., QIAN S.-B., ZHAO E.-G., et al. | ||
| 2022RAA....22c5024X | 43 | X | 1 | 9 | 2 | V0644 Ser: An Active Ultrashort Period Contact Binary Star. | XU H.-S., ZHU L.-Y., THAWICHARAT S., et al. | ||
|
2022ApJ...932..118C |
17 | D | 2 | 730182 | 4 | Searching for Anomalies in the ZTF Catalog of Periodic Variable Stars. | CHAN H.-S., VILLAR V.A., CHEUNG S.-H., 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. | ||
|
2024ApJS..273...31W |
18 | D | 1 | 5142 | ~ | A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey. | WANG J., DING X., LI J., et al. | ||
| 2025PASP..137f4201Z | 19 | D | 1 | 360 | ~ | The Photometric, Spectroscopic and Orbital Period Investigations of Ten Short Period Contact Binaries. | ZHANG B., GAO Y.-D., ZHAO G., et al. |