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Performance results of HESP physical model

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dc.contributor.author Anantha, Ch
dc.contributor.author Sivarani, T
dc.contributor.author Jones, D
dc.contributor.author Giridhar, S
dc.contributor.author Grobler, D
dc.contributor.author Jakobsson, R
dc.date.accessioned 2020-11-17T02:29:45Z
dc.date.available 2020-11-17T02:29:45Z
dc.date.issued 2017-02
dc.identifier.citation Experimental Astronomy, Vol. 43, No. 1, pp. 39-58 en_US
dc.identifier.issn 1572-9508
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7027
dc.description Restricted Access The original publication is available at springerlink.com © Springer http://dx.doi.org/10.1007/s10686-016-9519-9 en_US
dc.description.abstract As a continuation to the published work on model based calibration technique with HESP(Hanle Echelle Spectrograph) as a case study, in this paper we present the performance results of the technique. We also describe how the open parameters were chosen in the model for optimization, the glass data accuracy and handling the discrepancies. It is observed through simulations that the discrepancies in glass data can be identified but not quantifiable. So having an accurate glass data is important which is possible to obtain from the glass manufacturers. The model’s performance in various aspects is presented using the ThAr calibration frames from HESP during its pre-shipment tests. Accuracy of model predictions and its wave length calibration comparison with conventional empirical fitting, the behaviour of open parameters in optimization, model’s ability to track instrumental drifts in the spectrum and the double fibres performance were discussed. It is observed that the optimized model is able to predict to a high accuracy the drifts in the spectrum from environmental fluctuations. It is also observed that the pattern in the spectral drifts across the 2D spectrum which vary from image to image is predictable with the optimized model. We will also discuss the possible science cases where the model can contribute. en_US
dc.language.iso en en_US
dc.subject Astronomical spectrographs en_US
dc.subject High spectral resolution en_US
dc.subject Calibrations en_US
dc.subject Instrument modelling en_US
dc.subject Physical model based calibrations en_US
dc.subject Simultaneous reference observations en_US
dc.subject Double fibre en_US
dc.subject Wavelength calibrations en_US
dc.subject Instrumental drifts en_US
dc.title Performance results of HESP physical model en_US
dc.type Article en_US


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