cosmos.iasf-milano.inaf.it

Observational Cosmology Group at IASF-Mi

Multi-band infrared image (Blue=1μm, Green=1.3μm, Red=2.2μm) of the 1.7 square deg COSMOS field obtained with the ESA/VISTA telescope at Paranal Observatory. This is the widest deep view of the sky in the constellation of Sextans ever taken in infrared light with a total exposure time of 55 hours. More than 200,000 galaxies have been identified in this image. Credit: ESO/UltraVISTA Team/TERAPIX/CNRS/INSU/CASU. Welcome to the Observational Cosmology. The VIMOS Public Extragalactic Redshift Survey ( VIPERS.

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Observational Cosmology Group at IASF-Mi | cosmos.iasf-milano.inaf.it Reviews

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Multi-band infrared image (Blue=1μm, Green=1.3μm, Red=2.2μm) of the 1.7 square deg COSMOS field obtained with the ESA/VISTA telescope at Paranal Observatory. This is the widest deep view of the sky in the constellation of Sextans ever taken in infrared light with a total exposure time of 55 hours. More than 200,000 galaxies have been identified in this image. Credit: ESO/UltraVISTA Team/TERAPIX/CNRS/INSU/CASU. Welcome to the Observational Cosmology. The VIMOS Public Extragalactic Redshift Survey ( VIPERS.

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2 iasf

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5 recent publications

6 about the name

7 highlights

8 the pandora

9 research areas

10 astronomical projects

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Observational Cosmology Group at IASF-Mi | cosmos.iasf-milano.inaf.it Reviews

https://cosmos.iasf-milano.inaf.it

Multi-band infrared image (Blue=1μm, Green=1.3μm, Red=2.2μm) of the 1.7 square deg COSMOS field obtained with the ESA/VISTA telescope at Paranal Observatory. This is the widest deep view of the sky in the constellation of Sextans ever taken in infrared light with a total exposure time of 55 hours. More than 200,000 galaxies have been identified in this image. Credit: ESO/UltraVISTA Team/TERAPIX/CNRS/INSU/CASU. Welcome to the Observational Cosmology. The VIMOS Public Extragalactic Redshift Survey ( VIPERS.

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cosmos.iasf-milano.inaf.it

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Observational Cosmology Group at IASF-Mi

http://cosmos.iasf-milano.inaf.it/bianca/massiv.html

MASSIV: Mass assembly survey with SINFONI in VVDS. MASSIV aims at probing the galaxy kinematics between redshifts z 1 and 2 in order to gain insight into the assembly of mass along cosmic time, at a crucial epoch corresponding to the peak of cosmic star formation activity and which is likely to contain a wide range of galactic types. Multiwavelength survey in the Lockman Hole. Cluster Lensing And Supernova survey with Hubble. Mass Assembly Survey with SINFONI in VVDS. VIMOS VLT Deep Survey.

2

Observational Cosmology Group at IASF-Mi

http://cosmos.iasf-milano.inaf.it/bianca/euclid.html

Euclid: ESA Dark Energy mission. IASF-Milano has been deeply involved in all phases of the project, starting from the original SPACE proposal. Currently our activities are concentrated mainly in the following areas:. Within the Near Infrared Imaging Spectrograph (NISP) Instrument Team, we are in charge of the Instrument Scientific Performance Evaluation, and we participate to the global mission end-to-end simulations group. The Euclid Consortium Web page. The Euclid Web page at ESA. VIMOS VLT Deep Survey.

3

XMDS & XMM-LSS

http://cosmos.iasf-milano.inaf.it/dario/xmds_project.html

XMDS (X-RAY MEDIUM DEEP SURVEY). XMM-LSS (LARGE SCALE STRUCTURE SURVEY). Includes in its central area the XMDS, a deeper survey covering 2 square degrees of sky, located where the VVDS. Is going to be carried out. The XMDS is a collaboration between IFCTR, the Institut d'Astrophysique et de Géophysique de l'Université de Liège, and the Service d'Astrophysique - CEA Saclay, which pooled their XMM guaranteed time.

4

Euro3D

http://cosmos.iasf-milano.inaf.it/bianca/euro3D_project.html

Promoting 3D Spectroscopy in Europe. Is a project founded by the European Community within the RTN program, aimed at providing the Astronomical community with a tool for analysing three dimensional spectroscopical data. Eleven astronomical Institutes spread all over Europe participate to the project: AIP. In Postdam (Dr. M. Roth, Team leader), Institute of Astronomy. In Cambridge, University of Durham. Physics Department, ESO. In Garching, MPE. In Garching, Leiden Observatory. In Canary islands, and IFCTR.

5

PANDORA: Programs for AstroNomical Data Organization Reduction and Analysis

http://cosmos.iasf-milano.inaf.it/pandora

After more than five years, due to lack of manpower and funds, we cannot support the PANDORA programs and help-desk any more. Even the petition. Addressed to INAF President and top management. In support of PANDORA activity has failed to produce any improvement in the situation. Therefore, as of March 2011, the PANDORA project has been terminated.

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iasf-milano.inaf.it

..::IASF Milano / Projects:::..

http://www.iasf-milano.inaf.it/projects.html

EU Cookie Directive: This website is for scientific purposes and does not use cookies. High Energy Astrophysics Missions. Observational cosmology, surveys. FPGA Radiation Effects and Testing. Most research projects in which IASF-MI. Staff is involved are large, international scientific collaborations. Aim to take an integrated approach, whereby its staff is involved both in the hardware design and in the scientific data analysis phases. Short descriptions of the main.

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Observational Cosmology Group at IASF-Mi

Multi-band infrared image (Blue=1μm, Green=1.3μm, Red=2.2μm) of the 1.7 square deg COSMOS field obtained with the ESA/VISTA telescope at Paranal Observatory. This is the widest deep view of the sky in the constellation of Sextans ever taken in infrared light with a total exposure time of 55 hours. More than 200,000 galaxies have been identified in this image. Credit: ESO/UltraVISTA Team/TERAPIX/CNRS/INSU/CASU. Welcome to the Observational Cosmology. The VIMOS Public Extragalactic Redshift Survey ( VIPERS.

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