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Proposal Identification No.:

P2337

Date Received:

2007-Jun-02 09:32:47

Technical Page
Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 21 Hours 45

Arecibo Timing Observations of GLAST Gamma-Ray Pulsar Candidates

We propose to time three energetic young pulsars, all of which are very likely to have gamma-ray emission detectable by the Large Area Telescope on board the GLAST satellite. The main goal is to maintain knowledge of the rotational phase of these pulsars to an accuracy approaching 1%, allowing accurate folding of their gamma-ray photons. We are also likely to detect several glitches, which will improve our knowledge of the rotational behavior of the pulsars being monitored.

Name Paulo C Freire

Institution Arecibo Observatory

E-mail pfreire@naic.edu

Phone Ext. 358

Student no

Remote Observing Request

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

Instrument Setup
L-wide 327

Atmospheric Observation Instruments:

Sp ecial Equipment or setup:

none

RFI Considerations Frequency Ranges Planned
1120 - 1220 1360 - 1560 1


This proposal requires coordination with GPS L3 at 1381 MHz.

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