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20062009
most citedDark matter content and internal dynamics of NGC 4697: NMAGIC particle models from slit data and planetary nebulae velocities

101 citations · 332 across the 7 of their papers we have counts for

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14 papers · 1 filter

astro-ph20082 cited

White dwarfs in the Capodimonte deep field

R. Silvotti, S. Catalan, M. Cignoni +4

In this article we describe the search for white dwarfs (WDs) in the multi-band photometric data of the Capodimonte deep field survey. The WD candidates were selected through the V…

astro-ph2008101 cited

Dark matter content and internal dynamics of NGC 4697: NMAGIC particle models from slit data and planetary nebulae velocities

Flavio De Lorenzi, Ortwin Gerhard, Roberto P. Saglia +4

We present a dynamical study of NGC 4697, an almost edge-on, intermediate-luminosity, E4 elliptical galaxy, combining new surface brightness photometry, new as well as published lo…

astro-ph200753 cited

Presence of dust with a UV bump in massive, star-forming galaxies at 1 < z < 2.5

S. Noll, D. Pierini, M. Pannella +1

Fundamental properties of the extinction curve, like the slope in the rest-frame ultraviolet (UV) and the presence/absence of a broad absorption excess centred at 2175 A (the UV bu…

astro-ph200762 cited

The supermassive black hole in NGC4486a detected with SINFONI at the VLT

N. Nowak, R. P. Saglia, J. Thomas +4

The near-infrared integral field spectrograph SINFONI at the ESO VLT opens a new window for the study of central supermassive black holes. With a near-IR spatial resolution similar…

astro-ph2006

The Evolution of Galaxy Dust Properties for 1<z<2.5

Stefan Noll, Daniele Pierini, Maurilio Pannella +1

Fundamental properties of the extinction curve, like the slope in the rest-frame UV and the presence/absence of a broad absorption excess centred at 2175A (the UV bump), are invest…

astro-ph20068 cited

The Galactic Halo density distribution from photometric survey data: results of a pilot study

M. Cignoni, V. Ripepi, M. Marconi +4

Our goal is to recover the Galactic Halo spatial density by means of field stars. To this aim, we apply a new technique to the Capodimonte Deep Field (OACDF, Alcala' et al. 2004),…