PM J04263+4820 , the SIMBAD biblio

PM J04263+4820 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:04:06


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Title First 3 Authors
2013AJ....145..136L viz 15       D               1 205 21 Toward a spectroscopic census of white dwarfs within 40 pc of the Sun. LIMOGES M.-M., LEPINE S. and BERGERON P.
2015ApJS..219...19L viz 367       D     X C       9 651 82 Physical properties of the current census of northern white dwarfs within 40 pc of the Sun. LIMOGES M.-M., BERGERON P. and LEPINE S.
2016yCat....1.2035M viz 16       D               14271 ~ A Catalogue of Spectroscopically Identified White Dwarfs MCCOOK G.P. and SION E.M.
2019MNRAS.482.4570G viz 16       D               1 486646 296 A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS. GENTILE FUSILLO N.P., TREMBLAY P.-E., GANSICKE B.T., et al.
2019MNRAS.488.2892P viz 16       D               1 5860 40 Gaia Data Release 2 catalogue of extremely low-mass white dwarf candidates. PELISOLI I. and VOS J.
2021MNRAS.508.3877G viz 17       D               1 451937 102 A catalogue of white dwarfs in Gaia EDR3. GENTILE FUSILLO N.P., TREMBLAY P.-E., CUKANOVAITE E., et al.
2022MNRAS.509.2674G viz 17       D               1 3067 5 White dwarfs identified in LAMOST Data Release 5. GUO J., ZHAO J., ZHANG H., et al.
2022ApJ...936....5W viz 17       D               1 146 4 Extremely Low-mass White Dwarf Stars Observed in Gaia DR2 and LAMOST DR8. WANG K., NEMETH P., LUO Y., 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.
2024A&A...682A...5V viz 18       D               1 100886 ~ Classification and parameterization of a large Gaia sample of white dwarfs using XP spectra. VINCENT O., BARSTOW M.A., JORDAN S., et al.
2026ApJ...998..153X 20       D               1 432 ~ A Multiband Photometric Selection of Period Bouncer Candidates in the Solar Neighborhood with Gaia, GALEX, WISE, eROSITA, and XMM-Newton Data. XU X.-J., SHAO Y., HE W.-L., et al.

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