Proceedings Paper
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Paper Abstract
The instrumentation plan for the E-ELT foresees a High Resolution Spectrograph (HIRES). Among its main goals are the detection of atmospheres of exoplanets and the determination of fundamental physical constants. For this, high radial velocity precision and accuracy are required. HIRES will be designed for maximum intrinsic stability. Systematic errors from effects like intrapixel variations or random errors like fiber noise need to be calibrated. Based on the main requirements for the calibration of HIRES, we discuss different potential calibration sources and how they can be applied. We outline the frequency calibration concept for HIRES using these sources.
Paper Details
Date Published: 26 June 2017
PDF: 19 pages
Proc. SPIE 10329, Optical Measurement Systems for Industrial Inspection X, 103292M (26 June 2017); doi: 10.1117/12.2271782
Published in SPIE Proceedings Vol. 10329:
Optical Measurement Systems for Industrial Inspection X
Peter Lehmann; Wolfgang Osten; Armando Albertazzi Gonçalves Jr., Editor(s)
PDF: 19 pages
Proc. SPIE 10329, Optical Measurement Systems for Industrial Inspection X, 103292M (26 June 2017); doi: 10.1117/12.2271782
Show Author Affiliations
Philipp Huke, Georg-August-Univ. Göttingen (Germany)
Livia Origlia, INAF - Osservatorio Astronomico di Bologna (Italy)
Marco Riva, INAF - Osservatorio Astronomico di Brera (Switzerland)
Jake Charsley, Scottish Univ. Physics Alliance, Heriot-Watt Univ. (United Kingdom)
Richard McCracken, Scottish Univ. Physics Alliance, Heriot-Watt Univ. (United Kingdom)
Derryck Reid, Scottish Univ. Physics Alliance, Heriot-Watt Univ. (United Kingdom)
Grzegorz Kowzan, Nicolaus Copernicus Univ. (Poland)
Piotr Maslowski, Nicolaus Copernicus Univ. (Poland)
Karen Disseau, Georg-August-Univ. Göttingen (Germany)
Sebastian Schäfer, Georg-August-Univ. Göttingen (Germany)
Livia Origlia, INAF - Osservatorio Astronomico di Bologna (Italy)
Marco Riva, INAF - Osservatorio Astronomico di Brera (Switzerland)
Jake Charsley, Scottish Univ. Physics Alliance, Heriot-Watt Univ. (United Kingdom)
Richard McCracken, Scottish Univ. Physics Alliance, Heriot-Watt Univ. (United Kingdom)
Derryck Reid, Scottish Univ. Physics Alliance, Heriot-Watt Univ. (United Kingdom)
Grzegorz Kowzan, Nicolaus Copernicus Univ. (Poland)
Piotr Maslowski, Nicolaus Copernicus Univ. (Poland)
Karen Disseau, Georg-August-Univ. Göttingen (Germany)
Sebastian Schäfer, Georg-August-Univ. Göttingen (Germany)
Christopher Broeg, Univ. Bern (Switzerland)
Mirsad Sarajlic, Univ. Bern (Switzerland)
François Dolon, Observatoire de Haute-Provence (France)
Heidi Korhonen, Dark Cosmology Ctr., Niels Bohr Institute (Denmark)
Ansgar Reiners, Georg-August-Univ. Göttingen (Germany)
Isabelle Boisse, Lab. d'Astrophysique de Marseille (France)
Sandrine Perruchot, Observatoire de Haute-Provence (France)
Sebastien Ottogalli, Lab. J.L. Lagrange (France)
Francesco Pepe, Univ. de Genève (Switzerland)
Ernesto Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Mirsad Sarajlic, Univ. Bern (Switzerland)
François Dolon, Observatoire de Haute-Provence (France)
Heidi Korhonen, Dark Cosmology Ctr., Niels Bohr Institute (Denmark)
Ansgar Reiners, Georg-August-Univ. Göttingen (Germany)
Isabelle Boisse, Lab. d'Astrophysique de Marseille (France)
Sandrine Perruchot, Observatoire de Haute-Provence (France)
Sebastien Ottogalli, Lab. J.L. Lagrange (France)
Francesco Pepe, Univ. de Genève (Switzerland)
Ernesto Oliva, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Published in SPIE Proceedings Vol. 10329:
Optical Measurement Systems for Industrial Inspection X
Peter Lehmann; Wolfgang Osten; Armando Albertazzi Gonçalves Jr., Editor(s)
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