2MASS J03104437+3239291 , the SIMBAD biblio

2MASS J03104437+3239291 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST16:49:11


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Title First 3 Authors
2001ChJAA...1...46X 23 3 Optical identifications of X-ray selected AGNs. XU D.-W., WEI J.-Y. and HU J.-Y.
2006A&A...455..773V viz 108223 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2009ApJS..184..138H viz 15       D               1 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.
2010ApJS..186..378T viz 15       D               1 471 205 The 22 month Swift-BAT all-sky hard X-ray survey. TUELLER J., BAUMGARTNER W.H., MARKWARDT C.B., et al.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2010A&A...524A..64C viz 15       D               1 1294 157 The Palermo Swift-BAT hard X-ray catalogue. III. Results after 54 months of sky survey. CUSUMANO G., LA PAROLA V., SEGRETO A., et al.
2012ApJ...751...52E viz 15       D               1 4327 67 Reliable identifications of active galactic nuclei from the WISE, 2MASS, and ROSAT all-sky surveys. EDELSON R. and MALKAN M.
2013ApJS..207...19B viz 15       D               1 1212 487 The 70 month Swift-BAT all-sky hard X-ray survey. BAUMGARTNER W.H., TUELLER J., MARKWARDT C.B., et al.
2017ApJ...835...74I viz 16       D               1 606 73 The complete infrared view of active galactic nuclei from the 70 month Swift/BAT catalog. ICHIKAWA K., RICCI C., UEDA Y., et al.
2017ApJS..233...17R viz 16       D               1 863 302 BAT AGN spectroscopic survey. V. X-ray properties of the Swift/BAT 70-month AGN catalog. RICCI C., TRAKHTENBROT B., KOSS M.J., et al.
2018ApJS..235....4O viz 16       D               1 1636 246 The 105-month Swift-BAT all-sky hard X-ray survey. OH K., KOSS M., MARKWARDT C.B., et al.
2019ApJ...870...31I viz 16       D               1 606 69 BAT AGN spectroscopic survey. XI. The covering factor of dust and gas in Swift/BAT active galactic nuclei. ICHIKAWA K., RICCI C., UEDA Y., et al.
2020MNRAS.492..315G viz 16       D               1 290 ~ Comparison of SEDs of very massive radio-loud and radio-quiet AGN. GUPTA M., SIKORA M. and RUSINEK K.
2020ApJ...896..122L viz 16       D               1 823 10 The BAT AGN spectroscopic survey. XVIII. Searching for supermassive black hole binaries in X-rays. LIU T., KOSS M., BLECHA L., et al.
2020ApJ...900..125R viz 16       D               1 314 ~ On the diversity of jet production efficiency in Swift/BAT AGNs. RUSINEK K., SIKORA M., KOZIEL-WIERZBOWSKA D., et al.
2021A&A...645A..18D viz 17       D               1 1681 ~ Onboard catalogue of known X-ray sources for SVOM/ECLAIRs. DAGONEAU N., SCHANNE S., RODRIGUEZ J., et al.
2021AJ....162..206S 17       D               1 77 21 Searching for changing-state AGNs in massive data sets. I. Applying deep learning and anomaly-detection techniques to find AGNs with anomalous variability behaviors. SANCHEZ-SAEZ P., LIRA H., MARTI L., et al.
2022ApJS..261....2K viz 17       D               1 912 22 BASS. XXII. The BASS DR2 AGN Catalog and Data. KOSS M.J., RICCI C., TRAKHTENBROT B., et al.
2022ApJS..261....4O viz 17       D               1 744 15 BASS. XXIV. The BASS DR2 Spectroscopic Line Measurements and AGN Demographics. OH K., KOSS M.J., UEDA Y., et al.
2023A&A...675A..65S viz 17       D               1 447 ~ A machine learning algorithm for reliably predicting active galactic nucleus absorbing column densities. SILVER R., TORRES-ALBA N., ZHAO X., et al.
2025A&A...700A.111P viz 19       D               1 1181 ~ BASS XLIV. Morphological preferences of local hard X-ray selected AGNs. PARRA TELLO M., BAUER F.E., DE CICCO D., et al.
2025ApJ...991..116W 19       D               1 76 ~ BASS. LII. The Prevalence of Double-peaked Broad Lines at Low Accretion Rates among Hard X-Ray Selected Active Galactic Nuclei. WARD C., KOSS M.J., ERACLEOUS M., et al.

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