3XMM J082247.4+224145 , the SIMBAD biblio

3XMM J082247.4+224145 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST03:33:16


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Title First 3 Authors
2009MNRAS.399.1191C 17       D               1 90 378 Galaxy Zoo green peas: discovery of a class of compact extremely star-forming galaxies. CARDAMONE C., SCHAWINSKI K., SARZI M., et al.
2011ApJ...728..161I 1 77 185 Green pea galaxies and cohorts: luminous compact emission-line galaxies in the Sloan Digital Sky Survey. IZOTOV Yu.I., GUSEVA N.G. and THUAN T.X.
2012ApJ...746L...6C 92       D         F     1 9 13 Radio detection of green peas: implications for magnetic fields in young galaxies. CHAKRABORTI S., YADAV N., CARDAMONE C., et al.
2014A&A...561A..33I viz 15       D               1 99 36 Multi-wavelength study of 14000 star-forming galaxies from the Sloan Digital Sky Survey. IZOTOV Y.I., GUSEVA N.G., FRICKE K.J., et al.
2017A&A...599A..71D viz 16       D               1 209271 41 Aperture-free star formation rate of SDSS star-forming galaxies. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.
2017ApJ...844..171Y viz 17       D               1 43 129 Lyα profile, dust, and prediction of Lyα escape fraction in Green Pea galaxies. YANG H., MALHOTRA S., GRONKE M., et al.
2019ApJ...872..146J 16       D               1 39 2 Correlation between SFR surface density and thermal pressure of ionized gas in local analogs of high-redshift galaxies. JIANG T., MALHOTRA S., YANG H., et al.
2019ApJ...880..144S 2615       D     X C       64 8 3 Green Peas in X-rays. SVOBODA J., DOUNA V., ORLITOVA I., et al.
2019ApJ...881...48K 1665 T K A D S   X C       39 2 ~ A NuSTAR and XMM-Newton study of the two most actively star-forming Green Pea galaxies (SDSS J0749+3337 and
SDSS
J0822+2241
).
KAWAMURO T., UEDA Y., ICHIKAWA K., et al.
2020ApJ...891...19L 16       D               1 32 ~ VLT/X-Shooter spectroscopy of Lyman break analogs: direct-method O/H abundances and nitrogen enhancements. LOAIZA-AGUDELO M., OVERZIER R.A. and HECKMAN T.M.
2020ApJ...892...48R 16       D               1 66 24 The Lyman Alpha Reference Sample. X. Predicting Lyα output from star-forming galaxies using multivariate regression. RUNNHOLM A., HAYES M., MELINDER J., et al.
2020ApJ...893..134K 16       D               1 50 14 The importance of star formation intensity in Lyα escape from Green Pea galaxies and Lyman Break Galaxy Analogs. KIM K., MALHOTRA S., RHOADS J.E., et al.
2020MNRAS.498.3043M 83             C       1 12 12 The nature of CR7 revealed with MUSE: a young starburst powering extended Ly α emission at z = 6.6. MATTHEE J., PEZZULLI G., MACKENZIE R., et al.
2021ApJ...914....2K 17       D               1 43 15 The compact UV size of Green Pea galaxies as local analogs of high-redshift Lyα-emitters. KIM K.J., MALHOTRA S., RHOADS J.E., et al.
2022A&A...666A.186D viz 17       D               1 194359 6 Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.
2023MNRAS.520.5903H 17       D               1 75 7 Spectral shapes of the Ly α emission from galaxies - II. The influence of stellar properties and nebular conditions on the emergent Ly α profiles. HAYES M.J., RUNNHOLM A., SCARLATA C., et al.
2024A&A...686A.223P viz 18       D               1 1349 ~ What excites the optical emission in X-ray-selected galaxies? PULATOVA N.G., RIX H.-W., TUGAY A.V., et al.
2024A&A...687A.137B 1093       D     X C       24 37 ~ Radio properties of green pea galaxies. BORKAR A., GROSSOVA R., SVOBODA J., et al.
2024A&A...689A.170L 18       D               2 10 ~ The origin of the X-ray luminosity of the green pea galaxies: X-ray binaries or active galactic nuclei? LIU S., LUO A.-L., ZHENG Z., et al.
2024A&A...691A..27A 18       D               1 12 ~ X-ray observations of Blueberry galaxies. ADAMCOVA B., SVOBODA J., KYRITSIS E., et al.
2025ApJ...988..157B 6653     A     X C       142 6 ~ XMM-Newton Conclusively Identifies an Active Galactic Nucleus in a Green Pea Galaxy. BOORMAN P.G., SVOBODA J., STERN D., et al.

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