Wayne - A Simulator for HST WFC3 IR Grism Spectroscopy

@article{Varley2015WayneA,
  title={Wayne - A Simulator for HST WFC3 IR Grism Spectroscopy},
  author={R. Varley and A. Tsiaras and K. Karpouzas},
  journal={Astrophysical Journal Supplement Series},
  year={2015},
  volume={231},
  pages={13}
}
Wayne is an algorithm that simulates Hubble Space Telescope Wide Field Camera 3 (WFC3) grism spectroscopic frames, including sources of noise and systematics. It can simulate both staring and spatial scan modes, and observations such as the transit and the eclipse of an exoplanet. Unlike many other instrument simulators, the focus of Wayne is on creating frames with realistic systematics in order to test the effectiveness of different data analysis methods in a variety of different scenarios… Expand
A Population Study of Gaseous Exoplanets
ARES I: WASP-76 b, A Tale of Two HST Spectra.

References

SHOWING 1-10 OF 50 REFERENCES
A new approach to analysing HST spatial scans: the transmission spectrum of HD 209458 b
WFC3 detectors: on-orbit performance
Revised Flux Calibration of the WFC3 G102 and G141 grisms
Master sky images for the WFC3 G102 and G141 grisms
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