Analysis of Lossless Compressors Applied to Integer and Floating-Point Astronomical Data
In this work, lossless compression algorithms are evaluated on a variety of real, current as-tronomical images. The test dataset comprises raw (integer) and processed (floating-point) images of discrete and extensive astronomical objects, captured by spatial or terrestrial tele-scopes. Compression t...
| Authors: | , , , |
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| Format: | book part |
| Publication Date: | 2022 |
| Country: | España |
| Institution: | Universitat Autònoma de Barcelona |
| Repository: | Dipòsit Digital de Documents de la UAB |
| Language: | English |
| OAI Identifier: | oai:ddd.uab.cat:304347 |
| Online Access: | https://ddd.uab.cat/record/304347 https://dx.doi.org/urn:doi:10.1109/DCC52660.2022.00047 |
| Access Level: | Open access |
| Keyword: | Observatories Image coding Data compression Compressors Encoding Compression algorithms Compressor Lossless Compression Astronomical Data Integer Data Source Code Compression Ratio Celestial Bodies Discrete Objects Spatial Dimensions Wavelet Transform Spectral Properties Technical Data Image Compression Coding Tree High Compression Ratio Dominant Background Entropy Coding Burrows-Wheeler Transform |
| Summary: | In this work, lossless compression algorithms are evaluated on a variety of real, current as-tronomical images. The test dataset comprises raw (integer) and processed (floating-point) images of discrete and extensive astronomical objects, captured by spatial or terrestrial tele-scopes. Compression techniques herein analyzed are chosen to be representative of the most recent algorithms devised for astronomical data, as well as the most commonly employed compressors employed in real observatories. Experimental results suggest that coding techniques such as RICE and HCOMPRESS, typically employed in world-class observatories such as Roque de los Muchachos, do not produce the best possible lossless compression results. Instead, JPEG-LS, LZMA and NDZIP yield the best compression ratio results for 16-bit data (2.72), floating-point data (2.38) and radio data (1.81), respectively. Therefore, the efficiency with which data are stored and transmitted by these observatories could be significantly improved by selectively employing the aforementioned algorithms. |
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