PyISH: Python Integral Field Spectroscopy Simulation for HWO
Grace Sweetak, Breann Sitarski, Kevin France, Randall McEntaffer, and Richard Cartwright

TL;DR
PyISH is a high-fidelity simulation tool for the ultraviolet integral field spectrograph on the Habitable Worlds Observatory, aiding scientists and engineers in exploring science cases and instrument architectures.
Contribution
The paper introduces PyISH, a modular simulation tool specifically designed for modeling the UV IFS on HWO, enabling detailed science and engineering trade studies.
Findings
PyISH successfully simulates specific science cases for HWO's UV IFS.
The tool supports exploration of instrument architecture trade spaces.
PyISH enhances understanding of science and engineering trade-offs for HWO.
Abstract
The Habitable Worlds Observatory (HWO) will be a large ultraviolet/optical/near-infrared space telescope operating at the Sun-Earth Lagrange point L2. HWO was highly recommended by the National Academies` 2020 decadal survey and will be the first telescope designed specifically to search for life on planets orbiting other stars. HWO will also be able to perform a host of other transformational astrophysics, including cosmology, galaxy evolution, solar system science, and beyond. The development of the telescope and instrument suite is an iterative process. Example observatory architectures, called exploratory analytic cases (EACs) by the HWO Technology Maturation Project Office (TMPO), are modeled end-to-end to explore the engineering and science trade space. Recently, an ultraviolet Integral Field Spectrograph (UV IFS) was added to HWO's instrument suite for the EACs 4 and 5. To…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Photocathodes and Microchannel Plates · Stellar, planetary, and galactic studies
