RX J1039.7+6545 , the SIMBAD biblio

RX J1039.7+6545 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST18:05:35

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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
2003A&A...406..535Z viz 15       D               1 10257 80 The Hamburg/RASS Catalogue of optical identifications. Northern high-galactic latitude ROSAT Bright Source Catalogue X-ray sources. ZICKGRAF F.-J., ENGELS D., HAGEN H.-J., et al.
2004A&A...418..357K viz 15       D               1 57785 7 The Pul-3 catalogue of 58483 stars in the Tycho-2 system. KHRUTSKAYA E.V., KHOVRITCHEV M.Y. and BRONNIKOVA N.M.
2007AJ....133.2495D viz 15       D               2 197 2 Spectral classification of optical counterparts to ROSAT all-sky survey X-ray sources. DRAGOMIR D., ROY P. and RUTLEDGE R.E.
2007AJ....133.2825R viz 15       D               441 69 Meeting the cool neighbors. XI. Beyond the NLTT catalog. REID I.N., CRUZ K.L. and ALLEN P.R.
2009ApJS..181..444A viz 15       D               1 836 25 X-ray-emitting stars identified from the ROSAT All-Sky Survey and the Sloan Digital Sky Survey. AGUEROS M.A., ANDERSON S.F., COVEY K.R., 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.
2016ApJS..224...36K viz 16       D               1 45304 70 The AllWISE motion survey, part 2. KIRKPATRICK J.D., KELLOGG K., SCHNEIDER A.C., et al.
2017RMxAA..53..439M viz 16       D               1 89 ~ Absolute NUV magnitudes of Gaia DR1 astrometric stars and a search for hot companions in nearby systems. MAKAROV V.V.
2020ApJS..247...11R viz 16       D               1 46229 22 Radial velocity photon limits for the dwarf stars of spectral classes F-M. REINERS A. and ZECHMEISTER M.
2022ApJ...935..143P 17       D               2 19 4 Statistical Analysis of Stellar Flares from the First Three Years of TESS Observations. PIETRAS M., FALEWICZ R., SIARKOWSKI M., et al.

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