A robotic reflective Schmidt telescope for Dome C

Abstract This paper lays out a wide‐field robotic Schmidt telescope (RST) for the Antarctic site Dome C. The telescope is based on 80/120 cm reflective Schmidt optics, built originally for a space project, and a mosaic of four 7.5 k × 7.5 k 8‐ μ m thinned CCDs from the PEPSI/LBT wafer run. The teles...

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Bibliographic Details
Published in:Astronomische Nachrichten
Main Authors: Strassmeier, K. G., Andersen, M. I., Steinbach, M.
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2004
Subjects:
Antarctic
The Antarctic
Antarc*
Online Access:http://dx.doi.org/10.1002/asna.200410303
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2Fasna.200410303
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.200410303
Description
Summary:Abstract This paper lays out a wide‐field robotic Schmidt telescope (RST) for the Antarctic site Dome C. The telescope is based on 80/120 cm reflective Schmidt optics, built originally for a space project, and a mosaic of four 7.5 k × 7.5 k 8‐ μ m thinned CCDs from the PEPSI/LBT wafer run. The telescope's total field of view (FOV) would be 5° circular (minimum 3° × 3° square) with a plate scale of 0.7 arcsec per pixel. Limiting magnitude is expected to be V = 21.5 mag in 60 sec for a field of 9 square degrees. (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

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