LEDA 29197 , the SIMBAD biblio

LEDA 29197 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST03:51:08


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Title First 3 Authors
1984Afz....20...21M 131 26 The second Byurakan spectral sky survey. II. The results of the area centred on alpha = 09h 50m, delta = +55 00. MARKARIAN B.E. and STEPANIAN J.A.
1988Afz....29..548L 41 3 The second Byurakan sky survey. Spectra of galaxies. III. LIPOVETSKY V.A., STEPANIAN J.A., ERASTOVA L.K., et al.
1990AJ....100.1014M 144 73 High-redshift radio galaxies from Molonglo catalogue. McCARTHY P.J., KAPAHI V.K., VAN BREUGEL W., et al.
1990AJ....100.1028S 131 4 Accurate optical positions for 110 Byurakan objects and 24 blue stars from the "Second Byurakan spectral sky survey (II)". SEAL J., CHAVEZ D. and KOJOIAN G.
2003A&A...412...45P viz 15       D               1 956205 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2005RMxAA..41..155S viz 3231 23 The Second Byurakan Survey. General Catalogue. STEPANIAN J.A.
2008Ap.....51..349G viz 15       D               1 160 0 The relation of Second Byurakan Survey galaxies with Zwicky clusters. I. Data. GYULZADIAN M.V. and PETROSIAN A.R.
2009Ap.....52..205G 38           X         1 142 0 Relationship of galaxies from the second Byurakan survey to Zwicky clusters. II. Discussion. GYULZADIAN M.V., PETROSIAN A.R. and McLEAN B.
2014ApJ...788...45T viz 16       D               1 224162 54 Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. TOBA Y., OYABU S., MATSUHARA H., et al.
2018MNRAS.473.4731K viz 16       D               1 3462 68 Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images. KRUK S.J., LINTOTT C.J., BAMFORD S.P., et al.
2020ApJS..246....2A viz 17       D               1 36251 ~ GalWeight application: a publicly available catalog of dynamical parameters of 1800 galaxy clusters from SDSS-DR13, (GalWCat19). ABDULLAH M.H., WILSON G., KLYPIN A., et al.

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