NEAR: First Results from the Search for Low-Mass Planets in α Cen
NEAR: First Results from the Search for Low-Mass Planets in α Cen
复制标题
NEAR:在 α Cen 寻找低质量行星的初步结果
DOI:
10.18727/0722-6691/5163
复制
发表时间:
2019
期刊:
影响因子:
--
通讯作者:
A. Carlotti
中科院分区:
文献类型:
--
作者:
M. Kasper;R. Arsenault;U. Käufl;G. Jakob;S. Leveratto;G. Zins;E. Pantin;P. Duhoux;M. Riquelme;J. Kirchbauer;J. Kolb;P. Pathak;R. Siebenmorgen;C. Soenke;E. Fuenteseca;M. Sterzik;N. Ageorges;S. Gutruf;D. Kampf;A. Reutlinger;O. Absil;C. Delacroix;A. Maire;E. Huby;O. Guyon;P. Klupar;D. Mawet;G. Ruane;M. Karlsson;K. Dohlen;A. Vigan;M. N’diaye;S. Quanz;A. Carlotti
The Messenger 178 – Quarter 4 | 2019 ESO 3.6-metre telescope at La Silla, was modified and used to carry out the acceptance tests of the internal chopper. This was followed by a performance evaluation of the Annular Groove Phase Mask (AGPM) coronagraph with a dedicated optical setup incorporating a line-tunable CO2 laser, elliptical mirrors and germanium lenses. Four AGPM coronagraphs were tested, three specifically optimised for the NEAR filter (10–12.5 μm) and an older sample manufactured in 2012 and optimised for wavelengths between 11 and 13.1 μm. Surprisingly, the older coronagraph performed best, with a rejection ratio of up to 400 at 10.5 μm, and a contrast level of < 10– 4 at 3 λ/D.