Abstract

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.

Highlights

  • The main instrument for the South African Astronomical Observatory (SAAO) 1.9-m1 telescope has long been a Cassegrain spectrograph

  • In 1997, the introduction of a charge-coupled device (CCD) was seen, and a few years later, it was decided that the spectrograph’s inefficient Maksutov– Cassegrain camera optics would be replaced with a more elegant folded-Schmidt design to increase the throughput of the instrument

  • The spectrograph upgrade project received intermittent attention while observatory efforts were focused on the Southern African Large Telescope (SALT)

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Summary

Introduction

The main instrument for the South African Astronomical Observatory (SAAO) 1.9-m1 telescope has long been a Cassegrain spectrograph. A programmable logic controller (PLC) system was introduced in 2009 to enable most of the moving components (stepper motors and pneumatic actuators) and on/off toggles for lamps within the spectrograph to be placed under software control. This simplified the operation of the instrument, but the daily focusing of the camera optics remained a time-consuming manual task. The technical details of the modified instrument, Spectrograph Upgrade: Newly Improved Cassegrain (SpUpNIC),[2] were presented at the 2016 SPIE Astronomical Telescopes and Instrumentation conference, and this paper focuses on operational aspects and scientific performance

Optics
Detector
Rear-of-Slit Camera
Software
Operation
Grating Setup
15 GR8 10
Hartmann Focus Routine
Target Acquisition
Observing Sequences
Quick-Look Extractions
Data Storage and Transfer
Throughput Improvement
Wavelength Ranges and Resolutions
Radial Velocity Precision
Grating Stability
Image Quality
Findings
Summary
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