activity
20002026
most citedDeep ROSAT-HRI observations of the NGC 1399/NGC 1404 region: morphology and structure of the X-ray halo

128 citations · 851 across the 30 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 17 cited

Gauging the dark matter fraction in a S0 galaxy at z=0.47 through gravitational lensing from deep HST/ACS imaging

G. Covone, M. Paolillo, N. R. Napolitano +9

We analyze a new gravitational lens, OAC-GL J1223-1239, serendipitously found in a deep I-band image of the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS). The lens…

astro-ph2008★ 24 cited

The dynamical state of RX J1347.5-1145 from a combined strong lensing and X-ray analysis

M. Miranda, M. Sereno, E. De Filippis +1

We perform a combined X-ray and strong lensing analysis of RX J1347.5-1145, one of the most luminous galaxy clusters at X-ray wavelengths. We show that evidence from strong lensing…

astro-ph2005★ 27 cited

Further spectroscopic observations of the CSL-1 object

M. Sazhin, M. Capaccioli, G. Longo +2

CSL-1 is a peculiar object (R.A._{2000}= 12h 23m 30.5"; Dec_{2000}= -12deg 38' 57.0") which, for its photometric and spectroscopic properties, is possibly the first case of gravita…

astro-ph2001★ 10 cited

Photometric validation of a model independent procedure to extract galaxy clusters

E. Puddu, S. Andreon, G. Longo +3

By means of CCD photometry in three bands (Gunn g, r, i) we investigate the existence of 12 candidate clusters extracted via a model independent peak finding algorithm (\cite{memsa…

astro-ph2001★ 128 cited

Deep ROSAT-HRI observations of the NGC 1399/NGC 1404 region: morphology and structure of the X-ray halo

M. Paolillo, G. Fabbiano, G. Peres +1

We present the analysis of a deep (167 ks) ROSAT HRI observation of the cD galaxy NGC 1399 in the Fornax cluster. Using both HRI and, at larger radii, archival PSPC data, we find t…

astro-ph2000★ 80 cited

Luminosity function of clusters of galaxies

M. Paolillo, S. Andreon, G. Longo +5

The composite galaxy luminosity function (hereafter LF) of 39 Abell clusters of galaxies is derived by computing the statistical excess of galaxy counts in the cluster direction wi…