activity
19982024
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 32.4k across the 529 of their papers we have counts for

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Showing 2002Show all

6 papers · 1 filter

astro-ph2002★ 11 cited

Ho Measurement from VLT Deep I-band Surface Brightness Fluctuations in NGC 564 and NGC 7619

S. Mei, M. Scodeggio, D. R. Silva +1

We have measured the Hubble constant Ho in NGC 564 at cz ~ 5800 km/s and in NGC 7619 at cz ~ 3700 km/s with deep I-band Surface Brightness Fluctuation distance measurements at the…

astro-ph2002★ 345 cited

Introducing GOLDMine: A new Galaxy Database on the WEB

G. Gavazzi, A. Boselli, A. Donati +2

The new World Wide Web site "GOLDMine" (Galaxy On Line Database Milano Network) (http://goldmine.mib.infn.it) contains a multiwavelength data-base of an optically selected sample o…

astro-ph2002★ 19 cited

Optically-selected clusters at 0.8 < z < 1.3 in the EIS Cluster Survey

C. Benoist, L. da Costa, H. E. Jørgensen +9

This paper presents preliminary results of a spectroscopic survey being conducted at the VLT of fields with optically-selected cluster candidates identified in the EIS I-band surve…

astro-ph2002

Spectro-photometry of galaxies in the Virgo cluster

Giuseppe Gavazzi, Christian Bonfanti, Gerry Sanvito +2

As a result of an extensive observational campaign targeting the Virgo cluster, we obtained integrated (drift-scan mode) optical spectra and multiwavelength (UV,U,B,V,H) photometry…

astro-ph2002★ 46 cited

1.65 micron (H-band) surface photometry of galaxies. IX: photometric and structural properties of galaxies

M. Scodeggio, G. Gavazzi, P. Franzetti +3

As a result of a systematic NIR H-band (1.65 micron) imaging survey of normal galaxies in the local universe, we are able to measure in a highly homogeneous way photometric and str…

astro-ph2002★ 7 cited

1.65 micron (H-band) surface photometry of galaxies. VIII: the near-IR k-space at z=0

D. Pierini, G. Gavazzi, P. Franzetti +2

We present the distribution of a statistical sample of nearby galaxies in the k-space (k1 ~ log M, k2 ~ log Ie, k3 ~ log M/L). Our study is based on near-IR (H-band: lambda = 1.65…