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| 1RXS J053114.3-092237 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST13:02:52 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2003A&A...405..149F | 48 | 75 | Further identification of ROSAT all-sky survey sources in Orion. | FRASCA A., ALCALA J.M., COVINO E., 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. | ||
|
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. | ||
|
2017AJ....153..257O
|
16 | D | 1 | 10625 | 142 | Comoving stars in Gaia DR1: an abundance of very wide separation comoving pairs. | OH S., PRICE-WHELAN A.M., HOGG D.W., et al. | ||
|
2018A&A...609A.116R
|
16 | D | 1 | 143018 | 65 | Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. | RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al. | ||
|
2018AJ....155..149B
|
16 | D | 1 | 9764 | 5 | Fundamental properties of co-moving stars observed by Gaia. | BOCHANSKI J.J., FAHERTY J.K., GAGNE J., et al. | ||
|
2019AJ....158..122K
|
16 | D | 1 | 290057 | 150 | Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. | KOUNKEL M. and COVEY K. | ||
|
2020ApJ...890...46T
|
16 | D | 1 | 403 | 45 | Superflares on solar-type stars from the first year observation of TESS. | TU Z.-L., YANG M., ZHANG Z.J., et al. | ||
|
2022AJ....164..213G
|
17 | D | 1 | 124 | 2 | Correcting Stellar Flare Frequency Distributions Detected by TESS and Kepler. | GAO D.-Y., LIU H.-G., YANG M., et al. |
