BD+00 646 , the SIMBAD biblio

BD+00 646 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:51:45


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Title First 3 Authors
2009AJ....137.4598S viz 15       D               1 286 9 Photometry of type II Cepheid candidates from the northern part of the All Sky Automated Survey. SCHMIDT E.G., HEMEN B., ROGALLA D., et al.
2011AJ....141...53S viz 15       D               9 323 13 Spectra of type II cepheid candidates and related stars. SCHMIDT E.G., ROGALLA D. and THACKER-LYNN L.
2015MNRAS.449.1401H viz 16       D               1 3011 6 A large sample of metallic-line star candidates from LAMOST Data Release 1. HOU W., LUO A., YANG H., et al.
2019ApJ...879...69T viz 16       D               1 222610 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., 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.
2022ApJS..259...63S viz 17       D               1 10269 2 Objective Separation between CP1 and CP2 Based on Feature Extraction with Machine Learning. SHANG L.-H., LUO A.-L., WANG L., et al.
2023ApJS..264...17Z viz 17       D               1 31380 1 Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. ZHANG L.-Y., SU T., MISRA P., et al.
2023ApJS..266...14T viz 17       D               1 21501 ~ A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST. TIAN X.-M., WANG Z.-H., ZHU L.-Y., et al.

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