dc.contributor.author | Hoak, Daniel | |
dc.contributor.author | Barrett, John | |
dc.contributor.author | Crew, Geoffrey | |
dc.contributor.author | Pfeiffer, Violet | |
dc.date.accessioned | 2022-12-23T13:03:42Z | |
dc.date.available | 2022-12-23T13:03:42Z | |
dc.date.issued | 2022-12-17 | |
dc.identifier.uri | https://hdl.handle.net/1721.1/146937 | |
dc.description.abstract | The Haystack Observatory Postprocessing System (HOPS) is a multipurpose tool for post-correlation calibration and data analysis in Very-Long Baseline Interferometry experiments. The requirements on stations, baselines, and bandwidth for the Next Generation Event Horizon Telescope (ngEHT) have motivated a significant refactoring of the HOPS codebase. In this paper, we present the requirements, specifications, and design of HOPS 4.0 and the current state of the refactoring, and we discuss future work. | en_US |
dc.publisher | Multidisciplinary Digital Publishing Institute | en_US |
dc.relation.isversionof | http://dx.doi.org/10.3390/galaxies10060119 | en_US |
dc.rights | Creative Commons Attribution | en_US |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | en_US |
dc.source | Multidisciplinary Digital Publishing Institute | en_US |
dc.title | Progress on the Haystack Observatory Postprocessing System | en_US |
dc.type | Article | en_US |
dc.identifier.citation | Galaxies 10 (6): 119 (2022) | en_US |
dc.contributor.department | Haystack Observatory | |
dc.identifier.mitlicense | PUBLISHER_CC | |
dc.eprint.version | Final published version | en_US |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
dc.date.updated | 2022-12-22T14:35:09Z | |
dspace.date.submission | 2022-12-22T14:35:09Z | |
mit.license | PUBLISHER_CC | |
mit.metadata.status | Authority Work and Publication Information Needed | en_US |