[HCS2000] NIC J141727.28+522637.4 , the SIMBAD biblio

[HCS2000] NIC J141727.28+522637.4 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST07:19:57


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Title First 3 Authors
1991AJ....102.1258F 94 169 The micro-Jansky radio source population at 5 GHz. FOMALONT E.B., WINDHORST R.A., KRISTIAN J.A., et al.
1995MNRAS.276.1085H 41 60 The Canada-France redshift survey - VII. Optical counterparts of microjansky radio sources. HAMMER F., CRAMPTON D., LILLY S.J., et al.
1998AJ....116.2644O 158 28 The Hubble space telescope medium deep survey cluster sample: methodology and data. OSTRANDER E.J., NICHOL R.C., RATNATUNGA K.U., et al.
1998ApJ...499..112B viz 340 228 Hubble space telescope imaging of the CFRS and LDSS redshift surveys. I. Morphological properties. BRINCHMANN J., ABRAHAM R., SCHADE D., et al.
2000AJ....120.2843H 38 81 Star formation in galaxies between redshifts of 0.7 and 1.8. HOPKINS A.M., CONNOLLY A.J. and SZALAY A.S.
2000ApJ...544..641H 80 192 Faint radio sources and star formation history. HAARSMA D.B., PARTRIDGE R.B., WINDHORST R.A., et al.
2002ApJS..142....1S viz 15       D               1 7449 389 The DEEP Groth Strip Survey. II. Hubble Space Telescope structural parameters of galaxies in the Groth Strip. SIMARD L., WILLMER C.N.A., VOGT N.P., et al.
2005A&A...430..115H viz 174 227 Did most present-day spirals form during the last 8 Gyr? A formation history with violent episodes revealed by panchromatic observations. HAMMER F., FLORES H., ELBAZ D., et al.
2005A&A...435..507Z viz 76 34 HST/WFPC2 morphologies and bar structures of field galaxies at 0.4 < z < 1. ZHENG X.Z., HAMMER F., FLORES H., et al.
2005ApJ...620..595W 863 158 The DEEP Groth Strip galaxy redshift survey. III. Redshift catalog and properties of galaxies. WEINER B.J., PHILLIPS A.C., FABER S.M., et al.
2019A&A...631A...9B viz 17       D               1 8367 ~ The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue. BONGIOVANNI A., RAMON-PEREZ M., PEREZ GARCIA A.M., et al.
2021A&A...647A..89N viz 17       D               1 3659 ~ The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass-size relation up to z = 2. NADOLNY J., BONGIOVANNI A., CEPA J., et al.

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