SpUpNIC_JATIS.pdf (7.94 MB)
SpUpNIC (Spectrograph Upgrade: Newly Improved Cassegrain): a versatile and efficient low- to medium-resolution, long-slit spectrograph on the South African Astronomical Observatory's 1.9-m telescope
journal contributionposted on 2019-10-07, 10:28 authored by LA Crause, D Gilbank, C van Gend, HL Worters, C Sass, EJ Kotze, S Potter, A Sickafoose, R Sefako, J Southworth, L Macri, J Thorstensen, C Galan, P Skelton, C Engelbrecht, I Braker, H Winkler, D Pienkowski, D Surgit, A Erdem, M Burleigh
We report on the extensively upgraded Cassegrain spectrograph on the South African Astronomical Observatory (SAAO) 1.9-m telescope. The introduction of new collimator and camera optics, a new detector and controller, a rear-of-slit viewing camera to facilitate acquisition, and a new instrument control and quick-look data-reduction software (to take advantage of the entire system now being governed by a programmable logic controller) has revolutionized this workhorse instrument on Africa’s second largest optical telescope. The improvement in throughput over the previous incarnation of the spectrograph is ∼50 % in the red, increasing to a factor of four at the blue end. A selection of 10 surface-relief diffraction gratings is available to users, offering a variety of wavelength ranges and resolutions, with resolving powers between ∼500 and 6500. SpUpNIC (Spectrograph Upgrade: Newly Improved Cassegrain) has been scheduled for ∼80 % of the time available on the 1.9-m since being installed on the telescope in late October 2015, providing the single-object spectroscopic capability to support the broad research interests of the SAAO’s local and international user community. We present an assortment of data obtained for various observing programs to demonstrate different aspects of the instrument’s enhanced performance following this comprehensive upgrade.
This paper uses observations made at the South African Astronomical Observatory, which is supported by the National Research Foundation (NRF) of South Africa. We acknowledge financial assistance from the Leverhulme Trust, in the form of a Philip Leverhulme Prize, which supported JS and enabled the purchase of G13. CG and DP have been financially supported by a Polish National Science Centre grant SONATA No. DEC 2015/19/D/ST9/02974. We gratefully acknowledge John Booth’s invaluable mechanical engineering insights that helped us to resolve many a tricky problem on this instrument. Close colleagues and friends of the remarkable Darragh O'Donoghue will forever wish that he was still with us and able to enjoy observing with the spectrograph’s wonderful new camera optics that he designed many years ago.
CitationJournal of Astronomical Telescopes, Instruments, and Systems, 2019, 5(2), 024007
Author affiliation/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
- VoR (Version of Record)
Published inJournal of Astronomical Telescopes
PublisherSociety of Photo-optical Instrumentation Engineers (SPIE)