[YHW2016] 141.64780+29.57281 , the SIMBAD biblio

[YHW2016] 141.64780+29.57281 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST03:46:06

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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
2010ApJ...723.1119L viz 15       D               1 1041 41 On the populations of radio galaxies with extended morphology at z < 0.3. LIN Y.-T., SHEN Y., STRAUSS M.A., et al.
2010ApJS..191..254H viz 15       D               1 20101 235 A GMBCG galaxy cluster catalog of 55,424 rich clusters from SDSS DR7. HAO J., McKAY T.A., KOESTER B.P., et al.
2012MNRAS.421.1569B viz 15       D               2 18458 511 On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties. BEST P.N. and HECKMAN T.M.
2012ApJ...756..116A viz 15       D               1 156 20 The lifetime and powers of FR IIs in galaxy clusters. ANTOGNINI J., BIRD J. and MARTINI P.
2013ApJ...769...52W viz 15       D               1 276 15 A new approach to identifying the most powerful gravitational lensing telescopes. WONG K.C., ZABLUDOFF A.I., AMMONS S.M., et al.
2014ApJ...785..104R viz 15       D               1 72334 578 redMaPPer. I. Algorithm and SDSS DR8 catalog. RYKOFF E.S., ROZO E., BUSHA M.T., et al.
2016ApJS..224....1R viz 16       D               1 670875 246 The redMaPPer galaxy cluster catalog from DES science verification data. RYKOFF E.S., ROZO E., HOLLOWOOD D., et al.
2016MNRAS.460.3669Y viz 16       D               1 7138 25 Radio luminosity function of brightest cluster galaxies. YUAN Z.S., HAN J.L. and WEN Z.L.
2017MNRAS.466.4346M viz 16       D               1 1437 66 The nuclear properties and extended morphologies of powerful radio galaxies: the roles of host galaxy and environment. MIRAGHAEI H. and BEST P.N.
2018AJ....155..188L viz 16       D               1 13497 1 An analysis framework for understanding the origin of nuclear activity in low-power radio galaxies. LIN Y.-T., HUANG H.-J. and CHEN Y.-C.

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