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Дата изменения: Thu May 1 22:22:49 2014
Дата индексирования: Mon Apr 11 15:20:01 2016
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Proposal Identification No.:

P2030

Date Received:

2014-Mar-03 16:48:20

Technical Page
This proposal has been submitted before. The previous proposal number is P2030. Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 272 Hours

Continuing the PALFA Galactic Plane Survey

We propose to continue the PALFA survey of the Arecibo-visible Galactic Plane. The most sensitive pulsar survey ever done, PALFA is yielding high-impact science in a variety of astrophysical fields, including: fast radio bursts, high-precision tests of relativistic gravity theories, constraints on the equation-of-state of supra-nuclear matter, detectability of gravitational waves, and unification of the neutron star zoo. Additionally this survey constrains fundamental properties of the overall neutron-star population. PALFA has already discovered 132 pulsars, nearly doubling the number known in the survey region. For the coming year, we request a total of 272 hr of inner Galaxy time in order to complete our survey to |b|<2.0 deg, as well as to be secondary commensal partners with ongoing surveys of the outer Galactic Plane. With the requested inner Galaxy time we expect to discover an additional 40-80 radio pulsars and constrain models of the Galactic distribution of pulsars.

Name Victoria M Kaspi

Institution McGill University

E-mail vkaspi@physics.mcgill.ca

Phone 514-398-6412

Student no

Remote Observing Request

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

Instrument Setup
ALFA Atmospheric Observation Instruments:

1


Sp ecial Equipment or setup:

none

RFI Considerations Frequency Ranges Planned
1215 - 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.

2