SPHERE IFS: the spectro differential imager of the VLT for exoplanets search
SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets in the
vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
[PDF][PDF] SPHERE IFS: the spectro differential imager of the VLT for Exoplanets search
RU Claudi, M Turatto, E Giro, D Mesa, U Anselmi… - academia.edu
The SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
[PDF][PDF] SPHERE IFS: the spectro differential imager of the VLT for Exoplanets search
RU Claudi, M Turattob, E Giroa, D Mesaa, U Anselmia… - scholar.archive.org
The SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
[PDF][PDF] SPHERE IFS: the spectro differential imager of the VLT for Exoplanets search
RU Claudi, M Turattob, E Giroa, D Mesaa, U Anselmia… - researchgate.net
The SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
SPHERE IFS: the spectro differential imager of the VLT for exoplanets search
RU Claudi, M Turatto, RG Gratton… - Ground-based and …, 2008 - ui.adsabs.harvard.edu
SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets in the
vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
[引用][C] SPHERE IFS: the spectro differential imager of the VLT for exoplanets search
RU Claudi, M Turatto, RG Gratton, J Antichi… - SPIE …, 2008 - cir.nii.ac.jp
SPHERE IFS: the spectro differential imager of the VLT for exoplanets search | CiNii Research
CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データを …
CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データを …
[引用][C] SPHERE IFS: The spectro differential imager of the VLT for exoplanets search
RU CLAUDI, M TURATTO, D MESA… - … of SPIE, the …, 2008 - pascal-francis.inist.fr
SPHERE IFS : The spectro differential imager of the VLT for exoplanets search CNRS Inist
Pascal-Francis CNRS Pascal and Francis Bibliographic Databases Simple search Advanced …
Pascal-Francis CNRS Pascal and Francis Bibliographic Databases Simple search Advanced …
[PDF][PDF] SPHERE IFS: the spectro differential imager of the VLT for Exoplanets search
RU Claudi, M Turattob, E Giroa, D Mesaa, U Anselmia… - eso.org
The SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
SPHERE IFS: the spectro differential imager of the VLT for exoplanets search
R Claudi, M Turatto, R Gratton, J Antichi… - Proc. of SPIE … - spiedigitallibrary.org
ABSTRACT SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar
planets in the vicinity of bright stars and to characterize them through spectroscopic and …
planets in the vicinity of bright stars and to characterize them through spectroscopic and …
[PDF][PDF] SPHERE IFS: the spectro differential imager of the VLT for Exoplanets search
RU Claudi, M Turattob, E Giroa, D Mesaa, U Anselmia… - scholar.archive.org
The SPHERE is an exo-solar planet imager, which goal is to detect giant exo-solar planets
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …
in the vicinity of bright stars and to characterize them through spectroscopic and polarimetric …