Scipediacontent: Scipediacontent moved page Draft Content 433589427 to Mol et al 2010a

2021-02-02T02:53:41Z

Scipediacontent moved page Draft Content 433589427 to Mol et al 2010a

Scipediacontent: Created page with " == Abstract == Transient radio phenomena and pulsars are one of six LOFAR Key Science Projects (KSPs). As part of the Transients KSP, the Pulsar Working Group (PWG) has been..."

2021-02-02T02:53:35Z

Created page with " == Abstract == Transient radio phenomena and pulsars are one of six LOFAR Key Science Projects (KSPs). As part of the Transients KSP, the Pulsar Working Group (PWG) has been..."

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== Abstract ==

Transient radio phenomena and pulsars are one of six LOFAR Key Science Projects (KSPs). As part of the Transients KSP, the Pulsar Working Group (PWG) has been developing the LOFAR Pulsar Data Pipelines to both study known pulsars as well as search for new ones. The pipelines are being developed for the Blue Gene/P (BG/P) supercomputer and a large Linux cluster in order to utilize enormous amounts of computational capabilities (50Tflops) to process data streams of up to 23TB/hour. The LOFAR pipeline output will be using the Hierarchical Data Format 5 (HDF5) to efficiently store large amounts of numerical data, and to manage complex data encompassing a variety of data types, across distributed storage and processing architectures. We present the LOFAR Known Pulsar Data Pipeline overview, the pulsar beam-formed data format, the status of the pipeline processing as well as our future plans for developing the LOFAR Pulsar Search Pipeline. These LOFAR pipelines and software tools are being developed as the next generation toolset for pulsar processing in Radio Astronomy.

Comment: 6 pages, 1 figure. Accepted for publication in proceedings of "ISKAF2010 Science Meeting", PoS(ISKAF2010)60A

== Original document ==

The different versions of the original document can be found in:

* [http://arxiv.org/abs/1012.1583 http://arxiv.org/abs/1012.1583] under the license https://creativecommons.org/licenses/by-nc-sa

* [http://dx.doi.org/10.22323/1.112.0060 http://dx.doi.org/10.22323/1.112.0060]

* [https://dare.uva.nl/personal/pure/en/publications/the-lofar-known-pulsar-data-pipeline(ad8f15be-d1bd-4a2f-a190-74f99477adf2).html https://dare.uva.nl/personal/pure/en/publications/the-lofar-known-pulsar-data-pipeline(ad8f15be-d1bd-4a2f-a190-74f99477adf2).html]

* [https://pos.sissa.it/112/060/pdf https://pos.sissa.it/112/060/pdf]

* [https://pos.sissa.it/112/060/pdf https://pos.sissa.it/112/060/pdf],
: [https://pure.uva.nl/ws/files/1416984/90019_337557.pdf https://pure.uva.nl/ws/files/1416984/90019_337557.pdf],
: [https://core.ac.uk/display/85802556 https://core.ac.uk/display/85802556],
: [https://www.narcis.nl/publication/RecordID/oai%3Adare.uva.nl%3Apublications%2Fad8f15be-d1bd-4a2f-a190-74f99477adf2 https://www.narcis.nl/publication/RecordID/oai%3Adare.uva.nl%3Apublications%2Fad8f15be-d1bd-4a2f-a190-74f99477adf2],
: [http://ui.adsabs.harvard.edu/abs/2010iska.meetE..60A/abstract http://ui.adsabs.harvard.edu/abs/2010iska.meetE..60A/abstract],
: [https://www.researchgate.net/profile/JJD_Mol/publication/253042465_The_LOFAR_Known_Pulsar_Data_Pipeline/links/0046352260834b4694000000.pdf https://www.researchgate.net/profile/JJD_Mol/publication/253042465_The_LOFAR_Known_Pulsar_Data_Pipeline/links/0046352260834b4694000000.pdf],
: [https://pos.sissa.it/112/060 https://pos.sissa.it/112/060],
: [http://dare.uva.nl/document/2/90019 http://dare.uva.nl/document/2/90019],
: [http://dare.uva.nl/record/1/337557 http://dare.uva.nl/record/1/337557],
: [https://www.researchgate.net/profile/JJD_Mol/publication/253042465_The_LOFAR_Pulsar_Data_Pipeline/links/0046352260834b4694000000.pdf https://www.researchgate.net/profile/JJD_Mol/publication/253042465_The_LOFAR_Pulsar_Data_Pipeline/links/0046352260834b4694000000.pdf],
: [https://academic.microsoft.com/#/detail/2109926288 https://academic.microsoft.com/#/detail/2109926288] under the license cc-by-nc-sa

* [ ]

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Mol et al 2010a - Revision history

Scipediacontent: Scipediacontent moved page Draft Content 433589427 to Mol et al 2010a

Scipediacontent: Created page with " == Abstract == Transient radio phenomena and pulsars are one of six LOFAR Key Science Projects (KSPs). As part of the Transients KSP, the Pulsar Working Group (PWG) has been..."