Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/HankinstagP1977tp.ps Дата изменения: Mon Aug 30 23:55:56 2004 Дата индексирования: Sat Dec 22 22:38:00 2007 Кодировка: Поисковые слова: galaxy cluster

Proposal Identication No.: P1977 Date Received: 2004-Jun-01 13:12:45
Technical Page
Proposal Type: Regular
General Category: Pulsars
Observation Category:
Total Time Requested: 20 Hours
Proposal Title: Microstructure of two ve-component pulsars
ABSTRACT:
The signals from the ve-component pulsars B1237+25 and B1737+13 originate in both conal and core regions of
the emission region. Recent single pulse polarimetrly studies of B1237+25 reveals short structure in some of the
components. We propose to investigate the microstructure of these pulsars to test the hypothesis that the
longitudinal dependence will show signicant dierences in the core and conal regions.
Name Institution E-mail Phone Student
Timothy H Hankins thankins@nrao.edu (505) 835-5340 no
Service Observing Request Remot e Observing Request
X None X No
All of the observing run. Maybe
Part of the observing run. Yes
Queue Observing
Instrument Setup
610 327
Atmospheric Observation Instruments:
Description of Observer Equipment: New Mexico Tech Fast Pulsar Data Recorder
Special Equipment or setup: None
RFI Considerations
Frequency Ranges Planned
310-340 MHz
600-612 MHz
1