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| LSPM J1954+4720 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST05:04:02 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2005AJ....129.1483L 
|
63380 | 364 | A catalog of northern stars with annual proper motions larger than 0.15" (LSPM-NORTH catalog). | LEPINE S. and SHARA M.M. | |||||
|
2011ApJ...736...19B
|
15 | D | 1 | 1507 | 867 | Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. | BORUCKI W.J., KOCH D.G., BASRI G., et al. | ||
|
2011AJ....142..160S
|
15 | D | 1 | 2325 | 365 | Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. | SLAWSON R.W., PRSA A., WELSH W.F., et al. | ||
|
2014ApJS..210...19B
|
16 | D | 1 | 5860 | 211 | Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). | BURKE C.J., BRYSON S.T., MULLALLY F., et al. | ||
|
2014AJ....147..119C
|
16 | D | 1 | 8010 | 91 | Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. | COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al. | ||
|
2015ApJS..217...16R
|
16 | D | 1 | 8625 | 149 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
|
2020AJ....159..139L
|
17 | D | 1 | 5493 | 20 | Robo-AO M-dwarf multiplicity survey: catalog. | LAMMAN C., BARANEC C., BERTA-THOMPSON Z.K., et al. | ||
|
2021A&A...649A...6G
|
17 | D | 1 | 89188 | 168 | Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. | GAIA COLLABORATION, SMART R.L., SARRO L.M., et al. | ||
|
2022ApJS..259...50S
|
18 | D | 1 | 1632 | 9 | New Pulsating Stars Detected in EA-type Eclipsing-binary Systems Based on TESS Data. | SHI X.-D., QIAN S.-B. and LI L.-J. |
