|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| UPM J1928+4801 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST16:55:36 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2014ApJS..211...24M |
15 | D | 1 | 34022 | 573 | Rotation periods of 34,030 Kepler main-sequence stars: the full autocorrelation sample. | McQUILLAN A., MAZEH T. and AIGRAIN S. | ||
|
2014AJ....148..119F |
15 | D | 1 | 1765 | 12 | UCAC4 nearby star survey: a search for our stellar neighbors. | FINCH C.T., ZACHARIAS N., SUBASAVAGE J.P., et al. | ||
|
2015ApJ...807...45D |
16 | D | 1 | 2707 | 726 | The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity. | DRESSING C.D. and CHARBONNEAU D. | ||
|
2016AJ....151..160F |
16 | D | 1 | 1080 | 18 | Parallax results from URAT epoch data. | FINCH C.T. and ZACHARIAS N. | ||
|
2016MNRAS.457.2877G |
39 | X | 1 | 4245 | 141 | They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. | GAIDOS E., MANN A.W., KRAUS A.L., et al. | ||
|
2016A&A...594A..39F |
16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
|
2017ApJ...849...36Y |
16 | D | 1 | 542 | 111 | The flaring activity of M dwarfs in the Kepler field. | YANG H., LIU J., GAO Q., et al. | ||
|
2018AJ....155..176F |
16 | D | 2 | 1583 | 5 | URAT south parallax results. | FINCH C.T., ZACHARIAS N. and JAO W.-C. | ||
|
2018MNRAS.476..908F |
16 | D | 1 | 752 | 35 | Stellar activity with LAMOST - II. Chromospheric activity in open clusters. | FANG X.-S., ZHAO G., ZHAO J.-K., et al. | ||
|
2019ApJS..241...29Y |
16 | D | 1 | 3420 | 70 | The flare catalog and the flare activity in the Kepler mission. | YANG H. and LIU J. | ||
|
2019AJ....158...75H |
97 | D | C | 2 | 581 | 108 | Kepler planet occurrence rates for mid-type M dwarfs as a function of spectral type. | HARDEGREE-ULLMAN K.K., CUSHING M.C., MUIRHEAD P.S., et al. | |
|
2020ApJ...892...31B |
16 | D | 1 | 14873 | 35 | Temperatures and metallicities of M dwarfs in the APOGEE Survey. | BIRKY J., HOGG D.W., MANN A.W., et al. | ||
|
2020AJ....160...90A |
16 | D | 1 | 13200 | 33 | Exploring the evolution of stellar rotation using galactic kinematics. | ANGUS R., BEANE A., PRICE-WHELAN A.M., et al. | ||
|
2020AJ....160..120J |
16 | D | 1 | 365763 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
|
2021AJ....161..189L |
17 | D | 1 | 29956 | 19 | Gyro-kinematic ages for around 30,000 Kepler stars. | LU Y., ANGUS R., CURTIS J.L., et al. | ||
|
2021A&A...650A.115D |
17 | D | 1 | 2056 | 6 | Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars. | DREAU G., MOSSER B., LEBRETON Y., et al. | ||
|
2022AJ....163..152S |
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., et al. | ||
|
2022ApJS..259...35A |
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2022A&A...664A..78F |
17 | D | 1 | 7452 | 7 | Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. | FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al. | ||
|
2025A&A...695A..21Y |
19 | D | 1 | 201 | ~ | Flaring activities of fast rotating stars have a solar-like latitudinal distribution. | YANG H., CHENG X., LIU J., et al. |