Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 710681.0, MPI für Astronomie / Publikationen_mpia
High contrast polarimetry in the infrared with SPHERE on the VLT
Authors:Langlois, M.; Dohlen, K.; Vigan, A.; Zurlo, A.; Moutou, C.; Schmid, H. M.; Mili, J.; Beuzit, J.-L.; Boccaletti, A.; Carle, M.; Costille, A.; Dorn, R.; Gluck, L.; Hubin, N.; Feldt, M.; Kasper, M.; Lizon, L.; Madec, F.; Le Mignant, D.; Mouillet, D.; Puget, J. -. P.; Sauvage, J.-F.; Wildi, F.
Place of Publication:Bellingham, Wash.
Publisher:SPIE
Date of Publication (YYYY-MM-DD):2014
Audience:Not Specified
Abstract / Description:The instrument SPHERE (Spectro-Polarimetric High-contrast Exoplanet REsearch), recently installed on the VLT-UT3, aims to detected and characterize giant extra-solar planets and the circumstellar environments in the very close vicinity of bright stars. The extreme brightness contrast and small angular separation between the planets or disks and their parent stars have so far proven very challenging. SPHERE will meet this challenge by using an extreme AO, stellar coronagraphs, an infrared dual band and polarimetric imager called IRDIS, an integral field spectrograph, and a visible polarimetric differential imager called ZIMPOL. Polarimetry allows a separation of the light coming from an unpolarized source such as a star and the polarized source such as a planet or protoplanetary disks. In this paper we present the performance of the infrared polarimetric imager based on experimental validations performed within SPHERE before the preliminary acceptance in Europe. We report on the level of instrumental polarization in the infrared and its calibration limit. Using differential polarimetry technique, we quantify the level of speckle suppression, and hence improved sensitivity in the context of imaging extended stellar environments.
External Publication Status:published
Document Type:Other
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://cdsads.u-strasbg.fr/abs/2014SPIE.9147E..1RL
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.