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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/8020
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dc.contributor.authorShaw, Abinash Kumar-
dc.contributor.authorJagannath, Manoj-
dc.contributor.authorMazumder, Aishrila-
dc.contributor.authorChakraborty, Arnab-
dc.contributor.authorPatra, Narendra Nath-
dc.contributor.authorMondal, Rajesh-
dc.contributor.authorChoudhuri, Samir-
dc.date.accessioned2023-01-06T09:10:42Z-
dc.date.available2023-01-06T09:10:42Z-
dc.date.issued2022-12-15-
dc.identifier.citationJournal of Astrophysics and Astronomy, 2022, Vol.43, Article Number 99en_US
dc.identifier.issn0250-6335-
dc.identifier.issn0973-7758 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/8020-
dc.descriptionOpen Access from Indian Academy of Sciencesen_US
dc.description.abstractThe upcoming square kilometer array (SKA) is expected to produce humongous amount of data for undertaking H i science. We have developed an MPI-based Python pipeline to deal with the large data efficiently with the present computational resources. Our pipeline divides such large H i 21-cm spectral cubes into several small cubelets, and then processes them in parallel using publicly available H i source finder SoFiA-2. The pipeline also takes care of sources at the boundaries of the cubelets and also filters out false and redundant detections. By comapring with the true source catalog, we find that the detection efficiency depends on the SoFiA-2 parameters, such as the smoothing kernel size, linking length and threshold values. We find the optimal kernel size for all flux bins to be between 3–5 and 7–15 pixels, respectively, in the spatial and frequency directions. Comparing the recovered source parameters with the original values, we find that the output of SoFiA-2 is highly dependent on kernel sizes and a single choice of kernel is not sufficient for all types of H i galaxies. We also propose the use of alternative methods to SoFiA-2, which can be used in our pipeline to find sources more robustly.en_US
dc.language.isoenen_US
dc.publisherIndian Academy of Sciences, Bengaluruen_US
dc.relation.urihttps://ui.adsabs.harvard.edu/abs/2022JApA...43...99S/abstracten_US
dc.relation.urihttps://arxiv.org/abs/2211.02041en_US
dc.relation.urihttps://doi.org/10.1007/s12036-022-09880-1en_US
dc.rights2022 Indian Academy of Sciences, Bengaluruen_US
dc.subjectstatistical methodsen_US
dc.subjectdata analysisen_US
dc.subjectinterformetricen_US
dc.subjectcosmologyen_US
dc.subjectdiffuse radiationen_US
dc.titleDetecting galaxies in a large H i spectral cubeen_US
dc.typeArticleen_US
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