The SPHEREx Sky Simulator: Science Data Modeling for the First All-Sky Near-Infrared Spectral Survey
arXiv:2505.24856 · doi:10.3847/1538-4365/ae04cc
Abstract
We describe the SPHEREx Sky Simulator, a software tool designed to model science data for NASA's SPHEREx mission that will carry out a series of all-sky spectrophotometric surveys at 6'' spatial resolution in 102 spectral channels spanning 0.75 to 5 m. The Simulator software implements models for astrophysical emission, instrument characteristics, and survey strategy to generate realistic infrared sky scenes as they will be observed by SPHEREx. The simulated data includes a variety of realistic noise and systematic effects that are estimated using up-to-date astrophysical measurements and information from pre-launch instrument characterization campaigns. Through the pre-flight mission phases the Simulator has been critical in predicting the impact of various effects on SPHEREx science performance, and has played an important role guiding the development of the SPHEREx data analysis pipeline. In this paper, we describe the \skysim\ architecture, pre-flight instrument and sky models, and summarize high-level predictions from the Simulator, including a pre-launch prediction for the 5 point source sensitivity of SPHEREx, which we estimate to be 18.5--19 from 0.75 to 3.8~m and 16.6--18 from 3.8 to 5 m, with the sensitivity limited by the zodiacal light background at all wavelengths. In the future, on-orbit data will be used to improve the Simulator, which will form the basis of a variety of forward-modeling tools that will be used to model myriad instrumental and astrophysical processes to characterize their systematic effects on our final data products and analyses.
References in corpus (14)
- Array Programming with NumPy
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- EAZY: A Fast, Public Photometric Redshift Code
- The CatWISE2020 Catalog
- Techniques and Review of Absolute Flux Calibration from the Ultraviolet to the Mid-Infrared
- The WISE Extended Source Catalogue (WXSC) I: The 100 Largest Galaxies
- Impact of the SpaceX Starlink Satellites on the Zwicky Transient Facility Survey Observations
- SPHEREx: NASA's Near-Infrared Spectrophotmetric All-Sky Survey
- Ultraviolet to optical diffuse sky emission as seen by the Hubble Space Telescope Faint Object Spectrograph
- Measurements of the mean diffuse galactic light spectrum in the 0.95 μm to 1.65 μm band from CIBER
- A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 AU New Horizons-LORRI Data
- The SPHEREx Target List of Ice Sources (SPLICES)
- Noise Reduction Methods for Large-scale Intensity-mapping Measurements with Infrared Detector Arrays
- Image persistence flagging for SPHEREx
Cited by in corpus (6)
- Spectral response of SPHEREx
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- SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths
- The WEAVE acquisition and guiding software: pattern recognition-based acquisition and multi-fibre guiding
- Spectral Map Making with SPHEREx
- The Redshifts from 122 Bands: Comparative Redshift Forecast for Low-Resolution Spectra from SPHEREx and 7-Dimensional Sky Survey (7DS)