The VLT second generation instrument SPHERE (Spectro-Polarimetric High-contrast Exoplanets Research) was commissioned in the Summer of 2014, and offered to the community in the Spring of 2015. SPHERE is a high contrast imager that exploits its three scientific channels in order to observe and discover young warm exoplanets in the glare of their host stars. The three scientific instrument are: ZIMPOL, a polarization analyzer and imager that works in the visible range of wavelength, IRDIS a dual band imager and spectro polarimetric Camera that works in the NIR range up to K band, and IFS, an integral field spectrograph working in the YJH band. Very important is the complementarity between IRDIS and IFS. The former has a larger Field of view (about 12 arcseconds) while the IFS push its examination very close to the central star (FoV ∼ 1.7 arcsec). In one year of operational time a lot of very interesting scientific cases were investigated and very nice results were gathered. In this paper we would like to focus the attention on the high quality results and performances obtained with the IFS.
|Title of host publication||Ground-based and Airborne Instrumentation for Astronomy VI|
|Editors||Christopher J. Evans, Luc Simard, Hideki Takami|
|Place of Publication||Bellingham, WA|
|Number of pages||11|
|Publication status||Published - 2016|
|Event||Ground-Based and Airborne Instrumentation for Astronomy VI - Edinburgh, United Kingdom|
Duration: 26 Jun 2016 → 30 Jun 2016
|Name||Proceedings of SPIE|
|Other||Ground-Based and Airborne Instrumentation for Astronomy VI|
|Period||26/06/16 → 30/06/16|
Bibliographical noteCopyright 2016 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
- Extrasolar Planets
- High Contrast Imaging
- Integral Field Spectrograph