HARMONI at ELT: system analysis and performance estimation of the high-contrast module
HARMONI at ELT: system analysis and performance estimation of the high-contrast module
复制标题
HARMONI at ELT:高对比度模块的系统分析和性能评估
DOI:
10.1117/12.2628927
复制
发表时间:
2022
期刊:
影响因子:
--
通讯作者:
Carlotti A
中科院分区:
文献类型:
--
作者:
Carlotti A
HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000 and spatial sampling from 60mas to 4mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The project is preparing for Final Design Reviews. The high-contrast module (HCM) has been designed to characterize planets as close as 100mas from their host star (goal: 50mas), and presenting a 1e-6 flux ratio with it. To do so, it will use (1) a passive atmospheric dispersion corrector, (2) a set of amplitude apodizers and focal plane masks to lower the diffracted intensity next to the star and attenuate the PSF core, (3) a dedicated Zernike wavefront sensor to track the non-common path aberrations with the SCAO subsystem at a 0.1Hz frequency, and (4) post-processing algorithms that will rely on the temporal and spectral diversity of the IFS data to separate the planetary signals from the noise. This communication details several trade-off analyses involved in the co-design of the hardware of the HCM. It also presents contrast performance estimates that have been derived through an analysis of post-processed, simulated IFS data obtained with an end-to-end numerical model of the HCM and the rest of HARMONI. The respective interests of ADI and molecular mapping are compared in this specific case.
登录
查看更多内容
DOI:
--
发表时间:
2018
期刊:
Astronomical Telescopes + Instrumentation
影响因子:
--
作者:
J. Males;L. Close;K. Miller;L. Schatz;D. Doelman;J. Lumbres;F. Snik;A. Rodack;J. Knight;Kyle Van Gorkom;J. Long;A. Hedglen;M. Kautz;N. Jovanovic;K. Morzinski;O. Guyon;Ewan S Douglas;K. Follette;J. Lozi;Chris Bohlman;O. Durney;V. Gasho;P. Hinz;M. Ireland;M. Jean;C. Keller;M. Kenworthy;B. Mazin;J. Noenickx;D. Alfred;Kevin Perez;Anna Sanchez;C. Sauve;A. Weinberger;A. Conrad
通讯作者:
A. Conrad
影响因子:
6.5
作者:
H. J. Hoeijmakers;H. Schwarz;I. Snellen;R. Kok;M. Bonnefoy;G. Chauvin;A. Lagrange;Julien H. Girard
通讯作者:
Julien H. Girard
DOI:
--
发表时间:
2020
期刊:
Astronomical Telescopes + Instrumentation
影响因子:
--
作者:
L. Marafatto;M. Bergomi;F. Biondi;E. Carolo;M. De Pascale;D. Greggio;L. Lessio;D. Mesa;K. K. Radhakrishnan Santhakumari;G. Umbriaco;D. Vassallo;V. Viotto;A. Bianco;M. Dima;V. D’Orazi;P. Grenz;J. Leisenring;L. Mohr;M. Montoya;A. Zanutta;S. Antoniucci;C. Arcidiacono;F. Bacciotti;C. Baffa;A. Baruffolo;A. Bongiorno;A. Carlotti;S. Chinellato;L. Close;S. Di Filippo;S. Esposito;G. Farisato;O. Guyon;P. Hinz;D. Magrin;F. Pedichini;E. Pinna;E. Portaluri;A. Puglisi;R. Ragazzoni;F. Rossi;J. Farinato
通讯作者:
J. Farinato
DOI:
--
发表时间:
2018
期刊:
Astronomical Telescopes + Instrumentation
影响因子:
--
作者:
F. Hénault;A. Carlotti;P. Rabou;Y. Magnard;E. Sradler;D. Mouillet;G. Chauvin;M. Bonnefoy;J. Sauvage;K. Dohlen;A. Vigan;T. Fusco;K. El Hadi;P. Vola;F. Clarke;N. Thatte;I. Bryson;H. Schnetler;M. Tecza;C. Vérinaud
通讯作者:
C. Vérinaud
DOI:
--
发表时间:
2018
期刊:
Astronomical Telescopes + Instrumentation
影响因子:
--
作者:
A. Carlotti;F. Hénault;K. Dohlen;J. Sauvage;P. Rabou;Y. Magnard;A. Vigan;D. Mouillet;G. Chauvin;P. Vola;M. Bonnefoy;T. Fusco;K. El Hadi;N. Thatte;F. Clarke;M. Tecza;I. Bryson;H. Schnetler;C. Vérinaud
通讯作者:
C. Vérinaud