RX J0707.0+5752 , the SIMBAD biblio

RX J0707.0+5752 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST12:03:48


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
1998ApJS..117..319A viz 765 84 Identification of a complete sample of northern ROSAT all-sky survey X-ray sources. III. The catalog. APPENZELLER I., THIERING I., ZICKGRAF F.-J., et al.
2005A&A...433..151Z viz 257 19 Identification of a complete sample of northern ROSAT All-Sky Survey X-ray sources .VIII. The late-type stellar component. ZICKGRAF F.-J., KRAUTTER J., REFFERT S., et al.
2009ApJS..184..138H viz 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.
2011AJ....142..138L viz 15       D               1 8898 232 An all-sky catalog of bright M dwarfs. LEPINE S. and GAIDOS E.
2013MNRAS.435.2161F viz 15       D               1 8411 18 A catalogue of bright (K < 9) M dwarfs. FRITH J., PINFIELD D.J., JONES H.R.A., et al.
2020AJ....160..120J viz 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.
2022AJ....163..152S viz 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 viz 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.
2024MNRAS.533..395L viz 18       D               1 1559 ~ Atmospheric parameters and chemical abundances within 100 pc: a sample of G, K, and M main-sequence stars. LOPEZ-VALDIVIA R., ADAME L., ZAGALA LAGUNAS E., et al.

goto View the references in ADS