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19962007
most citedA highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope

44 citations · 64 across the 3 of their papers we have counts for

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8 papers · 1 filter

astro-ph200720 cited

Deep u*- and g-band Imaging of the Spitzer Space Telescope First Look Survey Field : Observations and Source Catalogs

Hyunjin Shim, Myungshin Im, Soojong Pak +4

We present deep u*-, and g-band images taken with the MegaCam on the 3.6 m Canada-France-Hawaii Telescope (CFHT) to support the extragalactic component of the Spitzer First Look Su…

astro-ph200644 cited

A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope

M. Magliocchetti, L. Silva, A. Lapi +4

The ~800 optically unseen (R>25.5) 24mum-selected sources in the complete Spitzer First Look Survey sample (Fadda et al. 2006) with F[24mum]>0.35 mJy are found to be very strongly…

astro-ph2002

The LARI Method for ISO-CAM/PHOT Data Reduction and Analysis

Carlo Lari, Mattia Vaccari, Giulia Rodighiero +5

The techniques and software tools developed for the reduction and analysis of ISO-CAM/PHOT data with the LARI method are presented. The method, designed for the detection of faint…

astro-ph2001

The dark side of star formation in galaxy clusters: spectroscopic follow-up of clusters observed with ISOCAM

Dario Fadda, Pierre-Alain Duc

The evolution of galaxies in cluster environments can be studied using mid-IR observations which trace star forming regions hidden by dust. The optical follow-up of A1689 (z=0.2),…

astro-ph2000

An excess of mid-IR luminous galaxies in Abell 1689?

D. Fadda, D. Elbaz, P. -A. Duc +4

We present the results of infrared observations of Abell 1689 which was observed with ISOCAM, at 6.7\mic and 15\mic, and ISOPHOT at 200\mic. The cluster galaxies detected above a s…

astro-ph1998

Deep ISOCAM Observations of Galaxy Clusters

Dario Fadda, David Elbaz

Ten galaxy clusters, with redshift ranging from 0.2 to 1, have been observed with the ISO camera in the two bands LW2 and LW3 (centered respectively at 6.75 and 15 microns). We pre…