An open source collection of computer programs has been developed and presented to the use of researchers to reduce the spectra taken with the multi-object spectrograph spectra used as the focal plane instrument of RTT150 telescope in the Tübitak National Observatory. Since the spectrograph has moving parts (i.e. grism, mask) and the pinholes on the mask are located at various locations with respect to dispersion axis, the spectrum produced in the focal plane is exposed to some effects such as order tilts and wavelength shifts. A dedicated algorithm has been applied to determine and correct order tilt and wavelength shifts to extract the spectra from different pinholes, which can provide the basis of a pipeline reduction for the Observatory. The geometric distortion on the observed spectrum is found to be negligible which eliminates the need for complex algorithms for aperture extraction.
Special thanks to Hicran BAKIŞ, Aytap SEZER and Günay PAYLI for making their MOS data available during the development of MRS.
Primary Language | English |
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Subjects | Astronomical Sciences (Other) |
Journal Section | Articles |
Authors | |
Publication Date | June 30, 2021 |
Submission Date | March 24, 2021 |
Acceptance Date | May 31, 2021 |
Published in Issue | Year 2021 Volume: 2 Issue: 1 |
TJAA is a publication of Turkish Astronomical Society (TAD).