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20022026
most citedThe Herschel ATLAS

596 citations · 19.1k across the 253 of their papers we have counts for

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24 papers · 1 filter

astro-ph2008★ 121 cited

Galaxies appear simpler than expected

M. J. Disney, J. D. Romano, D. A. Garcia-Appadoo +3

Galaxies are complex systems the evolution of which apparently results from the interplay of dynamics, star formation, chemical enrichment, and feedback from supernova explosions a…

astro-ph2008★ 32 cited

Correlations among the properties of galaxies found in a blind HI survey, which also have SDSS optical data

Diego A. Garcia-Appadoo, Andrew A. West, Julianne J. Dalcanton +2

We have used the Parkes Multibeam system and the Sloan Digital Sky Survey (SDSS) to assemble a sample of 195 galaxies selected originally from their HI signature to avoid biases ag…

astro-ph2008★ 43 cited

The UV luminosity function and star formation rate of the Coma cluster

L. Cortese, G. Gavazzi, A. Boselli

We present estimates of the GALEX NUV and FUV luminosity functions (LFs) of the Coma cluster, over a total area of ~9 deg^2 (~25 Mpc^2), i.e. from the cluster center to the virial…

astro-ph2008★ 82 cited

The origin of the mu_e - M_B and Kormendy relations in dwarf elliptical galaxies

A. Boselli, S. Boissier, L. Cortese +1

The present work is aimed at studying the distribution of galaxies of different types and luminosities along different structural scaling relations to see whether massive and dwarf…

astro-ph2008

Neutral Hydrogen and Star Formation in the Coma-Abell1367 Supercluster

Luca Cortese

We present preliminary results of a multi-wavelength study focused on the evolution of spiral galaxies in the UV-optical colour-magnitude (CM) diagram. By combining HI, UV and opti…

astro-ph2008★ 153 cited

UV Dust Attenuation in Star-forming Galaxies: II Calibrating the A(UV) vs. L_TIR/L_UV relation

L. Cortese, A. Boselli, P. Franzetti +4

We investigate the dependence of the total-infrared (TIR) to UV luminosity ratio method for calculating the UV dust attenuation A(UV) from the age of the underlying stellar populat…