Pregled bibliografske jedinice broj: 1081052
Synthetic astronomical image sequence generation
Synthetic astronomical image sequence generation // MIPRO 2020 43rd International Convention - Proceedings / Skala, Karolj (ur.).
Rijeka, 2020. str. 1347-1352 (predavanje, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
CROSBI ID: 1081052 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Synthetic astronomical image sequence generation
Autori
Gribl, Anita ; Petrinović, Davor
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
MIPRO 2020 43rd International Convention - Proceedings
/ Skala, Karolj - Rijeka, 2020, 1347-1352
Skup
43rd International Convention on Information and Communication Technology, Electronics and Microelectronics (MIPRO 2020) ; Business Intelligence Systems (miproBIS 2020)
Mjesto i datum
Opatija, Hrvatska, 28.09.2020. - 02.10.2020
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
synthetic astronomical image generation ; super-resolution ; compressed sensing ; geometric transformation ; optical aberrations modeling ; PSF ; MTF
Sažetak
Astronomical image reconstruction from multiple observations requires detailed knowledge of the imaging system. The reconstruction accuracy is determined by the imaging model correctness. Numerous parameters determine the model, and their precise estimation is a precondition for successful recon- struction. The best way to measure the model sensitivity on the parameter accuracy is a detailed simulation of the whole imaging process that takes into account all of the model parameters. The simulation enables an artificial manipulation of these parameters to reach the required accuracy. This paper describes a novel approach to generate a synthetic astronomical image sequence from the chosen star catalogs. Synthesis assumes point sources extracted from the catalogs and described through their angular position and magnitude in different spectral bands. The model parameters shall be tuned to the actual raw image captured by the SLR camera and chosen lens. The sequence of synthetic images of approximately the same part of the sky, but slightly shifted, is generated. The small shifts result that the light field integrates into different spatially displaced sampling grids, thus facilitating high-resolution image reconstruction from spatially subsampled projections.
Izvorni jezik
Engleski
Znanstvena područja
Fizika, Elektrotehnika, Računarstvo
POVEZANOST RADA
Projekti:
0036054
HRZZ-IP-2019-04-6703 - Renesansa teorije uzorkovanja (SamplingRenaissance) (Seršić, Damir, HRZZ ) ( CroRIS)
Ustanove:
Fakultet elektrotehnike i računarstva, Zagreb