Published July 19, 2021 | Version v1
Poster Open

A Flexible Python Observatory Automation Framework for the George Mason University Campus Telescope

  • 1. Department of Physics and Astronomy, George Mason University, 4400 University Dr, MS 3F3, Fairfax VA, USA, 22030
  • 2. Department of Physics and Astronomy, Rochester Institute of Technology, 1 Lomb Memorial Dr, Rochester NY, USA, 14623
  • 3. NASA Goddard Space Flight Center, 8800 Greenbelt Rd, Greenbelt MD, USA, 20771
  • 4. Department of Physics and Astronomy, George Mason University, 4400 University Dr, MS 3F3, Fairfax VA, USA, 22030; Woodson High School, 9525 Main St, Fairfax VA, USA, 22031
  • 5. Department of Physics and Astronomy, George Mason University, 4400 University Dr, MS 3F3, Fairfax VA, USA, 22030; NASA Goddard Space Flight Center, 8800 Greenbelt Rd, Greenbelt MD, USA, 20771
  • 6. Department of Physics and Astronomy, George Mason University, 4400 University Dr, MS 3F3, Fairfax VA, USA, 22030; Thomas Jefferson High School, for Science and Technology, 656 Braddock Rd, Alexandria VA, USA, 22312
  • 7. Department of Physics and Astronomy, George Mason University, 4400 University Dr, MS 3F3, Fairfax VA, USA, 22030; Flint Hill School, 3320 Jermantown Rd, Oakton VA, USA, 22124

Description

We present a unique implementation of python coding in an asynchronous object-oriented framework to fully automate the process of collecting data with the George Mason University Observatory’s 0.8-meter telescope. The goal of this project is to streamline the process of collecting research data and monitoring weather, most often for follow-up observations for the TESS mission. We have automated slews and dome movements, CCD exposures, saving FITS images, focusing and guiding on the target, and taking calibration images (darks and flats). We also have automated periodically checking weather conditions to automate the decision-making involved in whether a shutdown is necessary. We are now able to input the specifications of the desired target in a user-friendly GUI that generates an input configuration file and launches the command-line code at the beginning of the night. The code, in its current state, has been tested and used for observations without error on at least 110 nights.

Files

Michael Reefe - TSC2 Poster.pdf

Files (2.0 MB)

Name Size Download all
md5:b6c10da7365c063111afe8f3d29df74b
2.0 MB Preview Download

Additional details

References

  • W. J. Borucki, D. Koch, G. Basri, et al., "Kepler planet-detection mission: Introduction and first results," Science 327(5968), 977–980 (2010).
  • G. R. Ricker, J. N. Winn, R. Vanderspek, et al., "Transiting Exoplanet Survey Satellite," Journal of Astronomical Telescopes, Instruments, and Systems 1(1), 1 – 10 (2014).
  • D. Nesvorny and A. Morbidelli, "Mass and orbit determination from transit timing variations of exoplanets," The Astrophysical Journal 688, 636–646 (2008).
  • C. Baranec, R. Riddle, A. N. Ramaprakash, et al., "Robo-ao: autonomous and replicable laser-adaptive-optics and science system," Adaptive Optics Systems III (2012).
  • J. J. Swift, M. Bottom, J. A. Johnson, et al., "Miniature exoplanet radial velocity array i: design, commissioning, and early photometric results," Journal of Astronomical Telescopes, Instruments, and Systems 1, 027002 (2015).
  • J. Eastman, B. S. Gaudi, R. Siverd, et al., "DEMONEX: the DEdicated MONitor of EXo-transits," in Ground-based and Airborne Telescopes III, L. M. Stepp, R. Gilmozzi, and H. J. Hall, Eds., 7733, 1243 – 1250, International Society for Optics and Photonics, SPIE (2010).
  • K. Collins and J. Kielkopf, "Astroimagej: Imagej for astronomy," (2013). Astrophysics source code library.