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| Ton 415 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST23:03:03 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 1957BOTT....2p...3I | 807 | 21 | Estrellas azules en el casquete galactico norte. | IRIARTE B. and CHAVIRA E. | |||||
| 1983ApJS...51..171P | 162 | 88 | The Case low-dispersion northern sky survey. I. | PESCH P. and SANDULEAK N. | |||||
| 1995PASP..107.1059E | 124 | 5 | Hot subluminous stars and blue objects in the case low-dispersion northern sky survey. II. Quasar candidates. | EVERETT M.E. and WAGNER R.M. | |||||
2013MNRAS.429.2143C 
|
16 | D | 1 | 1968 | 63 | A search for the hidden population of AM CVn binaries in the Sloan digital sky survey. | CARTER P.J., MARSH T.R., STEEGHS D., et al. | ||
|
2015MNRAS.452..765G
|
16 | D | 1 | 1185 | 8 | An independent test of the photometric selection of white dwarf candidates using LAMOST DR3. | GENTILE FUSILLO N.P., REBASSA-MANSERGAS A., GANSICKE B.T., et al. | ||
|
2017A&A...600A..50G
|
16 | D | 5613 | 59 | The population of hot subdwarf stars studied with Gaia. I. The catalog of known hot subdwarf stars. | GEIER S., OSTENSEN R.H., NEMETH P., et al. | |||
|
2017ApJ...845..171B
|
16 | D | 1 | 1444 | 3 | A search for rapidly pulsating hot subdwarf stars in the GALEX survey. | BOUDREAUX T.M., BARLOW B.N., FLEMING S.W., et al. | ||
|
2018MNRAS.475.2480P
|
16 | D | 1 | 1459 | 13 | The sdA problem - I. Physical properties. | PELISOLI I., KEPLER S.O. and KOESTER D. | ||
|
2020A&A...635A.193G
|
17 | D | 2 | 6177 | 44 | The population of hot subdwarf stars studied with Gaia. III. Catalogue of known hot subdwarf stars: Data Release 2. | GEIER S. | ||
|
2022A&A...662A..40C
|
18 | D | 1 | 62976 | 9 | The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3. | CULPAN R., GEIER S., REINDL N., et al. |
