Bayesian Multi-wavelength Imaging of the LMC SN1987A with SRG/eROSITA
arXiv:2410.14599 · doi:10.1051/0004-6361/202452669
Abstract
The eROSITA Early Data Release (EDR) and eROSITA All-Sky Survey (eRASS1) data have already revealed a remarkable number of undiscovered X-ray sources. Using Bayesian inference and generative modeling techniques for X-ray imaging, we aim to increase the sensitivity and scientific value of these observations by denoising, deconvolving, and decomposing the X-ray sky. Leveraging information field theory, we can exploit the spatial and spectral correlation structures of the different physical components of the sky with non-parametric priors to enhance the image reconstruction. By incorporating instrumental effects into the forward model, we develop a comprehensive Bayesian imaging algorithm for eROSITA pointing observations. Finally, we apply the developed algorithm to EDR data of the Large Magellanic Cloud (LMC) SN1987A, fusing data sets from observations made by five different telescope modules. The final result is a denoised, deconvolved, and decomposed view of the LMC, which enables the analysis of its fine-scale structures, the identification of point sources in this region, and enhanced calibration for future work.
References in corpus (23)
- The eROSITA X-ray telescope on SRG
- The SRG X-ray orbital observatory, its telescopes and first scientific results
- The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere
- The eROSITA Final Equatorial Depth Survey (eFEDS): The X-ray catalog
- Information field theory for cosmological perturbation reconstruction and non-linear signal analysis
- The X-ray Remnant of SN1987A
- Detecting edges in the X-ray surface brightness of galaxy clusters
- NIFTY - Numerical Information Field Theory - a versatile Python library for signal inference
- Variable structures in M87* from space, time and frequency resolved interferometry
- Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
- The Formal Underpinnings of the Response Functions used in X-Ray Spectral Analysis
- High-resolution radio observations of SNR 1987A at high frequencies
- Information theory for fields
- Geometric variational inference
- XMM-Newton observations of SN1987A
- DPO - Denoising, Deconvolving, and Decomposing Photon Observations
- Background-Source Separation in astronomical images with Bayesian probability theory (I): the method
- Establishing the X-ray Source Detection Strategy for eROSITA with Simulations
- Re-Envisioning Numerical Information Field Theory (NIFTy.re): A Library for Gaussian Processes and Variational Inference
- First Study of the Supernova Remnant Population in the Large Magellanic Cloud with eROSITA
- Denoising, deconvolving and decomposing multi-domain photon observations- The D4PO algorithm
- Multi-Component Imaging of the Fermi Gamma-ray Sky in the Spatio-spectral Domain
- First spatio-spectral Bayesian imaging of SN1006 in X-ray