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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7970
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dc.contributor.authorBane Kshitij, Suhas Trupti-
dc.contributor.authorBarve, Indrajit V-
dc.contributor.authorGireesh, G. V. S-
dc.contributor.authorKathiravan, C-
dc.contributor.authorRamesh, R-
dc.date.accessioned2022-06-30T05:14:44Z-
dc.date.available2022-06-30T05:14:44Z-
dc.date.issued2022-01-
dc.identifier.citationJournal of Astronomical Telescopes, Instruments, and Systems, Vol. 8, No. 1, 017001en_US
dc.identifier.issn2329-4221-
dc.identifier.urihttp://hdl.handle.net/2248/7970-
dc.descriptionRestricted Accessen_US
dc.description.abstractA prototype for dedicated observations of pulsars and other astrophysical transients in the frequency range of 50 to 80 MHz has been recently commissioned in the Gauribidanur Radio Observatory near Bangalore in India. The antenna setup, the analog and digital receiver systems, and the initial observations are presented.en_US
dc.language.isoenen_US
dc.publisherSPIE-The International Society for Optical Engineeringen_US
dc.relation.urihttps://doi.org/10.1117/1.JATIS.8.1.017001-
dc.rights© SPIE-The International Society for Optical Engineering-
dc.subjectPulsarsen_US
dc.subjectRadio observationsen_US
dc.subjectLow frequenciesen_US
dc.subjectInstrumentationen_US
dc.titlePrototype for pulsar observations at low radio frequencies using log-periodic dipole antennasen_US
dc.typeArticleen_US
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