2026A&A...706A.229E


Query : 2026A&A...706A.229E

2026A&A...706A.229E - Astronomy and Astrophysics, volume 706A229 (2026/2-1)

Bayesian multiband imaging of SN1987A in the Large Magellanic Cloud with SRG/eROSITA.

EBERLE V., GUARDIANI M., WESTERKAMP M., FRANK P., FREYBERG M., SALVATO M. and ENSSLIN T.

Abstract (from CDS):

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 developed a comprehensive Bayesian imaging algorithm for eROSITA pointing observations. Finally, we applied the developed algorithm to EDR data of the Large Magellanic Cloud (LMC) SN1987A, fusing datasets 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.

Abstract Copyright: © The Authors 2026

Journal keyword(s): methods: data analysis - techniques: image processing - ISM: general - X-rays: general

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
2 SN 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
3 NAME 30 Dor C Superbubble Rad 05 35 50.8 -69 12 22           ~ 54 0
4 NAME 30 Dor Nebula SFR 05 38 36.0 -69 05 11           ~ 1276 2
5 RMC 136 Cl* 05 38 42.396 -69 06 03.36   5.81 5.40     ~ 2236 2

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