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  1. No Access

    Chapter and Conference Paper

    Shapley Supercluster Survey

    Our multi-wavelength survey of the Shapley supercluster (z  \(\sim\)  0.05) covers a contiguous area of 260 h 70 −2 Mpc2 includ...

    P. Merluzzi, G. Busarello, C. P. Haines, A. Mercurio… in The Universe of Digital Sky Surveys (2016)

  2. No Access

    Chapter and Conference Paper

    UV–IR Luminosity Functions and Stellar Mass Functions of Galaxies in the Shapley Supercluster Core

    We present a panchromatic study of luminosity functions (LFs) and stellar mass functions (SMFs) of galaxies in the core of the Shapley supercluster at z  = 0.048, in order to investigate how the dense environm...

    A. Mercurio, C. P. Haines, P. Merluzzi… in Environment and the Formation of Galaxies:… (2011)

  3. No Access

    Chapter and Conference Paper

    The VIMOS VLT Deep Survey (VVDS)

    This paper1 reviews the main results obtained so far by the VIRMOS VLT Deep Survey (VVDS) collaboration. The VVDS is one of the leading extragalactic surveys, started in 2002 using GTO awarded for the construc...

    R. Pelló, O. Le Fèvre, C. Adami, M. Arnaboldi… in Highlights of Spanish Astrophysics IV (2007)

  4. No Access

    Article

    A large population of galaxies 9 to 12 billion years back in the history of the Universe

    A survey of the distant Universe has revealed a much larger population of star-forming galaxies at high cosmological redshift than was previously known. A count of 970 galaxies with redshifts between 1.4 and 5...

    O. Le Fèvre, S. Paltani, S. Arnouts, S. Charlot, S. Foucaud, O. Ilbert… in Nature (2005)

  5. No Access

    Chapter and Conference Paper

    The VVDS: Early Results on the Large Scale Structure Distribution of Galaxies out to z~1.5

    The VIMOS VLT Deep Survey (VVDS) is an on-going program to map the evolution of galaxies, large scale structures and AGNs from the redshift measurement of more than 100000 objects down to a magnitude I ...

    O. Le Fèvre, G. Vettolani, D. Maccagni… in Multiwavelength Map** of Galaxy Formatio… (2005)

  6. No Access

    Chapter and Conference Paper

    The Vimos Vlt Deep Survey: Redshift Distribution of a I AB ≤ 24 Sample, and the Effect of Environment on Galaxy Evolution

    The knowledge of the general framework of galaxy evolution from direct observation is necessary to understand the morphologies and substructures like bars which are frequently observed in nearby galaxies. We r...

    Olivier Le Fevre, O. Ilbert, C. Marinoni… in Penetrating Bars through Masks of Cosmic D… (2004)

  7. No Access

    Chapter and Conference Paper

    The VIRMOS-VLT Deep Survey

    The aim of the VIRMOS VLT Deep Survey (VVDS) is to study of the evolution of galaxies, large scale structures and AGNs from a sample of more than 150,000 galaxies with measured redshifts in the range ...

    O. Le Fèvre, G. Vettolani, D. Maccagni, D. Mancini, A. Mazure, Y. Mellier… in Deep Fields (2001)

  8. No Access

    Chapter and Conference Paper

    Molecular clouds in LMC: Evaluation of physical parameters by means of MM observations

    P. Merluzzi, P. Andreani, L. Colangeli… in The Physics and Chemistry of Interstellar … (1995)

  9. No Access

    Article

    Comet P/grigg-Skjellerup: Ground-based observations after the encounter with the Giotto spacecraft

    After the encounter with the Giotto spacecraft, the comet P/Grigg-Skjellerup was observed with the 2.2 m ESO telescope. Imaging in theV andR bands and infrared photometry with theJ andH filters were performed. Fr...

    V. Mennella, L. Colangeli, A. Rotundi, P. Merluzzi, M. Fulle… in Il Nuovo Cimento C (1993)

  10. No Access

    Article

    Dehydrogenation study of cosmic-dust analogue grains

    New infrared and optical-absorption measurements performed on hydrogenated amorphous-carbon grains are presented. In particular, the spectral modifications produced by dehydrogenation of the samples are analys...

    V. Mennella, L. Colangeli, E. Bussoletti, P. Merluzzi, A. Rotundi in Il Nuovo Cimento C (1993)

  11. No Access

    Article

    Interstellar-dust properties as deduced from FIR and millimetric observations

    We have considered some millimetric observations of our Galaxy and of the Large Magellanic Cloud (LMC) taken at the Italian Base in Antarctica. Using other submm data and fitting all the observations with a mo...

    P. Merluzzi, A. Rotundi, L. Colangeli, V. Mennella, P. Andreani… in Il Nuovo Cimento C (1993)

  12. No Access

    Article

    Interstellar extinction: a parametrical study by using laboratory data

    In this paper we present a comparative study between laboratory data, astronomical observations and theoretical models in order to provide a contribution to the characterization ofcosmic-dust properties. In parti...

    A. Rotundi, P. Merluzzi, L. Colangeli, V. Mennella, E. Bussoletti in Il Nuovo Cimento C (1993)

  13. No Access

    Chapter and Conference Paper

    Dust and gas masses from mm continuum observations of LMC and SMC

    G. Dall'Oglio, P. Andreani, P. Merluzzi… in New Aspects of Magellanic Cloud Research (1993)

  14. No Access

    Article

    The Italian Astrophysical Observatory in Antarctica: OASI

    OASI (Infrared and Sub-mm Antarctic Observatory) is the first large telescope permanently installed in Antarctica. It is located close to the Italian Base in Antarctica (Terra Nova Bay Station, latitude: 74.39...

    G. Dall'oglio, P. A. R. Ade, P. Andreani, P. Calisse, M. Cappai… in Experimental Astronomy (1992)

  15. No Access

    Chapter and Conference Paper

    MM Observations of the Magellanic Clouds from Antarctica

    During the austral summer 1987/88 and 1989/90, we performed two Antarctic expeditions with the main purpose of installing the first permanent Antarctic Infrared Observatory O.A.S.I. (Osservatorio Antartico Sub...

    P. Calisse, G. Dall’Oglio, M. T. Di Bari… in Morphological and Physical Classification … (1992)