Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-26T04:11:43.833Z Has data issue: false hasContentIssue false

Getting Ready for TESS: an On-hand Software Tutorial

Workshop 3

Published online by Cambridge University Press:  29 August 2019

J. Burt
Affiliation:
Massachusetts Institute of Technology, Cambridge, MA, USA email: jennburt@mit.edu
T. Barclay
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The launch of NASA’s next exoplanet mission, the Transiting Exoplanet Survey Satellite (TESS), took place successfully on 2018 April 18, and has now commenced science operations. TESS is specifically designed to search for exoplanets transiting the closest and brightest stars using high-cadence photometric measurements. The images employed for detecting those planets can also be used for a wide variety of time-domain astronomy, especially when considering the full-frame images that TESS takes every 30 minutes. This (pre-launch) workshop familiarised participants with the details of how TESS will operate, described the expected data products and how to access them, introduced the software suite PyKE, which can be used to analyse TESS data, and highlighted ways for participants to request additional TESS targets.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

Bouma, L. G., Winn, J. N., Kosiarek, J., & McCullough, P. R. 2017, arXiv:1705.08891Google Scholar
Ricker, G. R., et al. 2015, J. Astron. Telescopes, Instruments, and Systems, 1, 014003CrossRefGoogle Scholar
Stassun, K. G., et al. 2017, arXiv:1706.00495Google Scholar
Still, M., & Barclay, T. 2012, Astrophys. Source Code Library, 1208.004Google Scholar
Sullivan, P. W. 2015, ApJ, 809, 1CrossRefGoogle Scholar
Vinícius, Z., Barentsen, G., Gully-Santiago, M., Cody, A. M., Hedges, C., Still, M., & Barclay, T. 2017, doi:10.5281/zenodo.835583CrossRefGoogle Scholar