PISCES: high contrast integral field spectrograph simulations and data reduction pipeline

2015 ◽  
Author(s):  
Jorge Llop Sayson ◽  
Nargess Memarsadeghi ◽  
Michael W. McElwain ◽  
Qian Gong ◽  
Marshall Perrin ◽  
...  
Keyword(s):  
Data Reduction ◽  
High Contrast ◽  
Integral Field Spectrograph ◽  
Integral Field

scholarly journals DARKNESS: A Microwave Kinetic Inductance Detector Integral Field Spectrograph for High-contrast Astronomy

2018 ◽  
Vol 130 (988) ◽  
pp. 065001 ◽  
Author(s):  
Seth R. Meeker ◽  
Benjamin A. Mazin ◽  
Alex B. Walter ◽  
Paschal Strader ◽  
Neelay Fruitwala ◽  
...  
Keyword(s):  
Kinetic Inductance Detector ◽  
Kinetic Inductance ◽  
High Contrast ◽  
Microwave Kinetic Inductance Detector ◽  
Integral Field Spectrograph ◽  
Integral Field

First light of the High Contrast Integral Field Spectrograph (HCIFS)

2018 ◽  
Author(s):  
He Sun ◽  
Tyler D. Groff ◽  
Maxime Rizzo ◽  
Mary Anne Limbach ◽  
Michael Galvin ◽  
...  
Keyword(s):  
High Contrast ◽  
Integral Field Spectrograph ◽  
Integral Field

scholarly journals Reduction of 3D Spectral Data, Obtained with the 6-meter Telescope

1995 ◽  
Vol 149 ◽  
pp. 308-310
Author(s):  
V. V. Vlasiouk
Keyword(s):  
Spectral Data ◽  
Spectral Methods ◽  
Data Reduction ◽  
Simultaneous Detection ◽  
Personal Computers ◽  
Specialized Software ◽  
Fabry Perot ◽  
Extended Sources ◽  
Integral Field Spectrograph ◽  
Integral Field

Development of 3D spectral methods on the 6-meter telescope prompted the necessity of creating specialized software for data reduction, adapted to personal computers IBM AT/386/486 class. We had to concentrate our efforts on preparing the software for bidimensional spectral data produced by Multi-Pupil Integral Field Spectrograph of the 6-meter telescope (MPFS) and analog of panoramic spectrophotometer with spectral channeling, using scanning Fabry-Perot interferometer (PYTHEAS-6).MPFS - analog of spectrograph TIGER (Courtes et al., 1988), developed for the 6-meter telescope, provides bidimensional spectroscopy of extended sources, allowing the simultaneous detection of 99 individual spectra, produced by a lens raster from 9 by 11 microlenses. The main features of this instrument are described in (Afanasiev et al, 1994).

scholarly journals Scientific design of a high contrast integral field spectrograph for the Subaru Telescope

2012 ◽  
Author(s):  
Michael W. McElwain ◽  
Timothy D. Brandt ◽  
Markus Janson ◽  
Gillian R. Knapp ◽  
Mary A. Peters ◽  
...  
Keyword(s):  
High Contrast ◽  
Integral Field Spectrograph ◽  
Integral Field

scholarly journals A fully automated data reduction pipeline for the FRODOSpec integral field spectrograph

2012 ◽  
Vol 333 (2) ◽  
pp. 101-117 ◽  
Author(s):  
R.M. Barnsley ◽  
R.J. Smith ◽  
I.A. Steele
Keyword(s):  
Data Reduction ◽  
Integral Field Spectrograph ◽  
Integral Field

scholarly journals Performance tests on the SPHERE-IFS

2013 ◽  
Vol 8 (S299) ◽  
pp. 54-55
Author(s):  
Dino Mesa ◽  
Raffaele Gratton ◽  
Riccardo U. Claudi ◽  
Silvano Desidera ◽  
Enrico Giro ◽  
...  
Keyword(s):  
Spectral Type ◽  
Extrasolar Planets ◽  
Imaging Method ◽  
Performance Tests ◽  
High Contrast ◽  
Direct Imaging ◽  
Critical Issues ◽  
Integral Field Spectrograph ◽  
Integral Field

AbstractUntil now, just a few extrasolar planets (30 out of 860) have been found through the direct imaging method. This number should greatly improve when the next generation of High Contrast Instruments like Gemini Planet Imager (GPI) at Gemini South Telescope or SPHERE at VLT will became operative at the end of this year. In particular, the Integral Field Spectrograph (IFS), one of the SPHERE subsystems, should allow a first characterization of the spectral type of the found extrasolar planets. Here we present the results of the last performance tests that we have done on the IFS instrument at the Institut de Planetologie et d'Astrophysique de Grenoble (IPAG) in condition as similar as possible to the ones that we will find at the telescope. We have found that we should be able to reach contrast down to 5 × 10−7 and make astrometry at sub-mas level with the instrument in the actual conditions. A number of critical issues have been identified. The resolution of these problems could allow to further improve the performance of the instrument.

scholarly journals High-contrast integral field spectrograph (HCIFS): multi-spectral wavefront control and reduced-dimensional system identification

2020 ◽  
Vol 28 (15) ◽  
pp. 22412
Author(s):  
He Sun ◽  
Alexei Goun ◽  
Susan Redmond ◽  
Michael Galvin ◽  
Tyler Groff ◽  
...  
Keyword(s):  
System Identification ◽  
Dimensional System ◽  
High Contrast ◽  
Wavefront Control ◽  
Integral Field Spectrograph ◽  
Integral Field

scholarly journals Data reduction pipeline for the CHARIS integral-field spectrograph I: detector readout calibration and data cube extraction

2017 ◽  
Vol 3 (04) ◽  
pp. 1 ◽  
Author(s):  
Timothy D. Brandt ◽  
Maxime Rizzo ◽  
Tyler Groff ◽  
Jeffrey Chilcote ◽  
Johnny P. Greco ◽  
...  
Keyword(s):  
Data Reduction ◽  
Data Cube ◽  
Integral Field Spectrograph ◽  
Integral Field

scholarly journals First light of the CHARIS high-contrast integral-field spectrograph

2017 ◽  
Author(s):  
Maxime Rizzo ◽  
Thayne Currie ◽  
Tyler D. Groff ◽  
Jeffrey K. Chilcote ◽  
Timothy Brandt ◽  
...  
Keyword(s):  
High Contrast ◽  
Integral Field Spectrograph ◽  
Integral Field
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