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| ASAS J114028-6201.6 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST02:18:02 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2006AJ....132..866R 
|
15 | D | 1076 | 188 | Identification of new M dwarfs in the solar neighborhood. | RIAZ B., GIZIS J.E. and HARVIN J. | |||
|
2009ApJS..184..138H
|
15 | D | 2 | 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. | ||
| 2010OEJV..128....1B | 25 | 2 | Chromospherically active stars in the ASAS-3 database: Paper 2. | BERNHARD K. and BERNHARD C. | |||||
| 2010BAVSM.211....1B | 151 | X C | 3 | 25 | 0 | Chromospherically active stars in the ASAS-3 database: Paper 2. 25 new variables. | BERNHARD K. and BERNHARD C. | ||
|
2012AcA....62...67K
|
15 | D | 1 | 2326 | 121 | ASAS photometry of ROSAT sources. I. Periodic variable stars coincident with bright sources from the ROSAT All Sky Survey. | KIRAGA M. | ||
|
2016MNRAS.461..794P
|
16 | D | 1 | 802 | 260 | The star formation history and accretion-disc fraction among the K-type members of the Scorpius-Centaurus OB association. | PECAUT M.J. and MAMAJEK E.E. | ||
|
2018ApJ...868...32G
|
16 | D | 1 | 1859 | 7 | A large moving group within the Lower Centaurus Crux association. | GOLDMAN B., ROSER S., SCHILBACH E., et al. | ||
|
2018A&A...620A.172Z
|
16 | D | 1 | 127610 | 99 | 3D mapping of young stars in the solar neighbourhood with Gaia DR2. | ZARI E., HASHEMI H., BROWN A.G.A., et al. | ||
|
2023A&A...677A..59R
|
17 | D | 1 | 13197 | ~ | Significance mode analysis (SigMA) for hierarchical structures An application to the Sco-Cen OB association. | RATZENBOCK S., GROSSSCHEDL J.E., MOLLER T., et al. | ||
|
2024AJ....167..210V
|
18 | D | 1 | 7289 | ~ | The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. | VACH S., ZHOU G., HUANG C.X., et al. |
