Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/SpitlertagP2886tp.pdf Дата изменения: Thu Sep 11 21:11:58 2014 Дата индексирования: Mon Apr 11 16:50:57 2016 Кодировка: Поисковые слова: п п п п п п п п п п п п п п п п п п

Proposal Identification No.:

P2886

Date Received:

2014-Sep-01 11:29:31

Technical Page
This proposal has been submitted before. The previous proposal number is P2886. Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Pulsars Transient 10 Hours 1 hour

Follow-up of the First Fast Radio Burst Discovered with Arecibo

Fast radio bursts (FRBs) are a new class of short-duration radio bursts discovered in archival data from pulsar surveys. FRBs may represent a new class of astrophysical sources at extragalactic distances ­ inferred from their large dispersion measures. Seven FRBs are now in the published literature with the first six discovered by the Parkes Radio Telescope in Australia. Recently, Arecibo became the first independent telescope to confirm the existence of FRBs when a burst was discovered by the Pulsar ALFA survey. No repeat events have been seen from any FRB sky position, although most follow-up has been fairly limited. We propose to follow-up the Arecibo FRB with a larger field-of-view, more time, and greater range of observing frequencies than has been done for any other FRB. As repeatability (or lack thereof ) is crucial to understanding the nature of these sources, systematic and thorough follow-up is essential.

Name Laura G Spitler

Institution Max-Planck-Institut for Radio Astronomy

E-mail lspitler@mpifr-bonn.mpg.de

Phone +49228525108

Student no

Remote Observing Request

Observer will travel to AO X Remote Observing In Absentia (instructions to operator)

Instrument Setup
327 ALFA

Atmospheric Observation Instruments:

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Sp ecial Equipment or setup: Both ALFA and the 327 MHz receivers are needed for each session.

RFI Considerations Frequency Ranges Planned
302 - 352 1214 - 1536 This proposal requires coordination with Punta Salinas radar within the band 1222-1381 MHz.. This proposal requires coordination with GPS L3 at 1381 MHz.

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