Simulated JWST datasets for multispectral and hyperspectral image fusion
arXiv:2001.02618 · doi:10.3847/1538-3881/ab9301
Abstract
This paper aims at providing a comprehensive framework to generate an astrophysical scene and to simulate realistic hyperspectral and multispectral data acquired by two JWST instruments, namely NIRCam Imager and NIRSpec IFU. We want to show that this simulation framework can be resorted to assess the benefits of fusing these images to recover an image of high spatial and spectral resolutions. To do so, we create a synthetic scene associated with a canonical infrared source, the Orion Bar. This scene combines pre-existing modelled spectra provided by the JWST Early Release Science Program 1288 and real high resolution spatial maps from the Hubble space and ALMA telescopes. We develop forward models including corresponding noises for the two JWST instruments based on their technical designs and physical features. JWST observations are then simulated by applying the forward models to the aforementioned synthetic scene. We test a dedicated fusion algorithm we developed on these simulated observations. We show the fusion process reconstructs the high spatio-spectral resolution scene with a good accuracy on most areas, and we identify some limitations of the method to be tackled in future works. The synthetic scene and observations presented in the paper are made publicly available and can be used for instance to evaluate instrument models (aboard the JWST or on the ground), pipelines, or more sophisticated algorithms dedicated to JWST data analysis. Besides, fusion methods such as the one presented in this paper are shown to be promising tools to fully exploit the unprecedented capabilities of the JWST.
References in corpus (25)
- The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
- Dust Grain Size Distributions and Extinction in the Milky Way, LMC, and SMC
- The James Webb Space Telescope
- A convex formulation for hyperspectral image superresolution via subspace-based regularization
- A model for atomic and molecular interstellar gas: The Meudon PDR code
- The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: II. Model of the Interplanetary Dust Cloud
- Fast Fusion of Multi-Band Images Based on Solving a Sylvester Equation
- The Mid-Infrared Instrument for the James Webb Space Telescope I: Introduction
- Photoevaporation of Circumstellar Disks due to External FUV Radiation in Stellar Aggregates
- Photoevaporation of Circumstellar Disks by FUV, EUV and X-ray Radiation from the Central Star
- The global dust SED: Tracing the nature and evolution of dust with DustEM
- A PDR-Code Comparison Study
- Top-down formation of fullerenes in the interstellar medium
- Compression and ablation of the photo-irradiated cloud the Orion Bar
- Evaporating Very Small Grains as tracers of the UV radiation field in Photo-dissociation Regions
- Pandeia: A Multi-mission Exposure Time Calculator for JWST and WFIRST
- Structure of photodissociation fronts in star-forming regions revealed by observations of high-J CO emission lines with Herschel
- The PAH emission characteristics of the reflection nebula NGC2023
- Surface chemistry in the Interstellar Medium II. formation on dust with random temperature fluctuations
- Photon-Dominated Chemistry in the Nucleus of M82: Widespread HOC+ emission in the inner 650 pc disk
- Detectors for the James Webb Space Telescope Near-Infrared Spectrograph I: Readout Mode, Noise Model, and Calibration Considerations
- Excitation of H in photodissociation regions as seen by Spitzer
- On surface completion and image inpainting by biharmonic functions: Numerical aspects
- Polycyclic aromatic hydrocarbons and molecular hydrogen in oxygen-rich planetary nebulae: the case of NGC6720
- Herschel survey and modelling of externally-illuminated photoevaporating protoplanetary disks
Cited by in corpus (5)
- PDRs4All: A JWST Early Release Science Program on radiative feedback from massive stars
- Unmixing methods based on nonnegativity and weakly mixed pixels for astronomical hyperspectral datasets
- The distribution of mutual inclinations arising from the stellar quadrupole moment
- Fusion of JWST data: Demonstrating practical feasibility
- Best of both worlds: Fusing hyperspectral data from two generations of spectro-imagers for X-ray astrophysics