GRIS : The GREGOR Infrared Spectrograph

M. Collados; R. López; E. Páez; E. Hernández; M. Reyes; A. Calcines; E. Ballesteros; J. J. Díaz; C. Denker; A. Lagg; R. Schlichenmaier; W. Schmidt; S. K. Solanki; K. G. Strassmeier; O. von der Lühe; R. Volkmer

doi:10.1002/asna.201211738

GRIS : The GREGOR Infrared Spectrograph

M. Collados^*
, R. López
, E. Páez
, E. Hernández
, M. Reyes
, A. Calcines
, E. Ballesteros
, J. J. Díaz
, C. Denker
, A. Lagg
, R. Schlichenmaier
, W. Schmidt
, S. K. Solanki
, K. G. Strassmeier
, O. von der Lühe
, R. Volkmer

^*Corresponding author for this work

Not published at Aalto University

Research output: Contribution to journal › Article › Scientific › peer-review

149 Citations (Scopus)

Abstract

This paper describes the main characteristics of GRIS (GREGOR Infrared Spectrograph), the grating spectrograph installed in the recently inaugurated (May 2012) 1.5-meter GREGOR telescope located at the Observatorio del Teide in Tenerife. The spectrograph has a standard Czerny-Turner configuration with parabolic collimator and camera mirrors that belong to the same conic surface. Although nothing prevents its use at visible wavelengths, the spectrograph will be initially used in combination with the infrared detector of the Tenerife Infrared Polarimeter (TIP-II) in standard spectroscopic mode as well as for spectropolarimetric measurements.

Original language	English
Pages (from-to)	872-879
Number of pages	8
Journal	Astronomische Nachrichten
Volume	333
Issue number	9
DOIs	https://doi.org/10.1002/asna.201211738
Publication status	Published - Nov 2012
MoE publication type	A1 Journal article-refereed

Keywords

Instrumentation: spectrographs
Techniques: spectroscopic
Telescopes

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10.1002/asna.201211738

Cite this

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title = "GRIS : The GREGOR Infrared Spectrograph",

abstract = "This paper describes the main characteristics of GRIS (GREGOR Infrared Spectrograph), the grating spectrograph installed in the recently inaugurated (May 2012) 1.5-meter GREGOR telescope located at the Observatorio del Teide in Tenerife. The spectrograph has a standard Czerny-Turner configuration with parabolic collimator and camera mirrors that belong to the same conic surface. Although nothing prevents its use at visible wavelengths, the spectrograph will be initially used in combination with the infrared detector of the Tenerife Infrared Polarimeter (TIP-II) in standard spectroscopic mode as well as for spectropolarimetric measurements.",

keywords = "Instrumentation: spectrographs, Techniques: spectroscopic, Telescopes",

author = "M. Collados and R. L{\'o}pez and E. P{\'a}ez and E. Hern{\'a}ndez and M. Reyes and A. Calcines and E. Ballesteros and D{\'i}az, \{J. J.\} and C. Denker and A. Lagg and R. Schlichenmaier and W. Schmidt and Solanki, \{S. K.\} and Strassmeier, \{K. G.\} and \{von der L{\"u}he\}, O. and R. Volkmer",

year = "2012",

month = nov,

doi = "10.1002/asna.201211738",

language = "English",

volume = "333",

pages = "872--879",

journal = "Astronomische Nachrichten",

issn = "1521-3994",

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T1 - GRIS : The GREGOR Infrared Spectrograph

AU - Collados, M.

AU - López, R.

AU - Páez, E.

AU - Hernández, E.

AU - Reyes, M.

AU - Calcines, A.

AU - Ballesteros, E.

AU - Díaz, J. J.

AU - Denker, C.

AU - Lagg, A.

AU - Schlichenmaier, R.

AU - Schmidt, W.

AU - Solanki, S. K.

AU - Strassmeier, K. G.

AU - von der Lühe, O.

AU - Volkmer, R.

PY - 2012/11

Y1 - 2012/11

N2 - This paper describes the main characteristics of GRIS (GREGOR Infrared Spectrograph), the grating spectrograph installed in the recently inaugurated (May 2012) 1.5-meter GREGOR telescope located at the Observatorio del Teide in Tenerife. The spectrograph has a standard Czerny-Turner configuration with parabolic collimator and camera mirrors that belong to the same conic surface. Although nothing prevents its use at visible wavelengths, the spectrograph will be initially used in combination with the infrared detector of the Tenerife Infrared Polarimeter (TIP-II) in standard spectroscopic mode as well as for spectropolarimetric measurements.

AB - This paper describes the main characteristics of GRIS (GREGOR Infrared Spectrograph), the grating spectrograph installed in the recently inaugurated (May 2012) 1.5-meter GREGOR telescope located at the Observatorio del Teide in Tenerife. The spectrograph has a standard Czerny-Turner configuration with parabolic collimator and camera mirrors that belong to the same conic surface. Although nothing prevents its use at visible wavelengths, the spectrograph will be initially used in combination with the infrared detector of the Tenerife Infrared Polarimeter (TIP-II) in standard spectroscopic mode as well as for spectropolarimetric measurements.

KW - Instrumentation: spectrographs

KW - Techniques: spectroscopic

KW - Telescopes

UR - https://www.scopus.com/pages/publications/84868706329

U2 - 10.1002/asna.201211738

DO - 10.1002/asna.201211738

M3 - Article

AN - SCOPUS:84868706329

SN - 1521-3994

VL - 333

SP - 872

EP - 879

JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

IS - 9

ER -

GRIS : The GREGOR Infrared Spectrograph

Abstract

Keywords

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