PhoSim-NIRCam: photon-by-photon image simulations of the James Webb Space Telescope’s near-infrared camera
Author
Burke, Colin J.Peterson, John R.
Egami, Eiichi
Leisenring, Jarron M.
Sembroski, Glenn H.
Rieke, Marcia J.
Affiliation
Univ Arizona, Steward ObservIssue Date
2019-06-06Keywords
James Webb Space Telescope's near-infrared cameraimage simulation
instrumentation
photon simulator
weak lensing
systematic
Metadata
Show full item recordCitation
Burke, C. J., Peterson, J. R., Egami, E., Leisenring, J. M., Sembroski, G. H., & Rieke, M. J. (2019). PhoSim-NIRCam: photon-by-photon image simulations of the James Webb Space Telescope’s near-infrared camera. Journal of Astronomical Telescopes, Instruments, and Systems, 5(3), 038002.Rights
© 2019 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Recent instrumentation projects have allocated resources to develop codes for simulating astronomical images. Physics-based models are essential for understanding telescope, instrument, and environmental systematics in observations. A deep understanding of these systematics is especially important in the context of weak gravitational lensing, galaxy morphology, and other sensitive measurements. We present an adaptation of a physics-based ab initio image simulator: the photon simulator (PhoSim). We modify PhoSim for use with the near-infrared camera (NIRCam)-the primary imaging instrument aboard the James Webb Space Telescope. This photon Monte Carlo code replicates the observational catalog, telescope and camera optics, detector physics, and readout modes/electronics. Importantly, PhoSim-NIRCam simulates both geometric aberration and diffraction across the field of view. Full field- and wavelength-dependent point spread functions are presented. Simulated images of an extragalactic field are presented. Extensive validation is planned during in-orbit commissioning. (C) 2019 Society of Photo-Optical Instrumentation Engineers (SPIE)ISSN
2329-4124Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/1.jatis.5.3.038002
