Data

Parkes observations for project P574 semester 2009OCTS

Commonwealth Scientific and Industrial Research Organisation
Weltevrede, Patrick ; Possenti, Andrea ; Manchester, Dick ; Johnston, Simon ; Kramer, Michael ; Hobbs, George ; Keith, Michael ; Romani, R ; Thompson, David J. ; Thorsett, Stephen ; Roberts, Mallory
Viewed: [[ro.stat.viewed]] Cited: [[ro.stat.cited]] Accessed: [[ro.stat.accessed]]
ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.4225/08/5220D98386199&rft.title=Parkes observations for project P574 semester 2009OCTS&rft.identifier=https://doi.org/10.4225/08/5220D98386199&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We request time to observe 160 pulsars on a regular basis in order to provide accurate ephemerides necessary for the detection of gamma-ray pulsars with the Fermi and AGILE satellites. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, to characterise their high energy spectra and phase resolved spectroscopy of the brightest pulsars. In the radio, the observations will also allow us to find glitches, characterise timing noise, investigate dispersion and rotation measure variability and enhance our knowledge of single pulse phenomenology. To date, we are (co-)authors on 2 Agile papers, 4 Fermi papers, 3 radio papers and authors on 3 papers in submission. The data are contributing to the PhD theses of Lucas Guillemot and Damien Parent from the Bordeaux Fermi group.&rft.creator=Weltevrede, Patrick &rft.creator=Possenti, Andrea &rft.creator=Manchester, Dick &rft.creator=Johnston, Simon &rft.creator=Kramer, Michael &rft.creator=Hobbs, George &rft.creator=Keith, Michael &rft.creator=Romani, R &rft.creator=Thompson, David J. &rft.creator=Thorsett, Stephen &rft.creator=Roberts, Mallory &rft.date=2013&rft.edition=v2&rft_rights=Creative Commons Attribution 3.0 Unported Licence https://creativecommons.org/licenses/by/3.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO Australia 2011.&rft_subject=pulsars&rft_subject=neutron stars&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data

Licence & Rights:

Open Licence view details
CC-BY

Creative Commons Attribution 3.0 Unported Licence
https://creativecommons.org/licenses/by/3.0/

Data is accessible online and may be reused in accordance with licence conditions

All Rights (including copyright) CSIRO Australia 2011.

Access:

Open view details

Accessible for free

Contact Information



Full description

We request time to observe 160 pulsars on a regular basis in order to provide accurate ephemerides necessary for the detection of gamma-ray pulsars with the Fermi and AGILE satellites. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, to characterise their high energy spectra and phase resolved spectroscopy of the brightest pulsars. In the radio, the observations will also allow us to find glitches, characterise timing noise, investigate dispersion and rotation measure variability and enhance our knowledge of single pulse phenomenology. To date, we are (co-)authors on 2 Agile papers, 4 Fermi papers, 3 radio papers and authors on 3 papers in submission. The data are contributing to the PhD theses of Lucas Guillemot and Damien Parent from the Bordeaux Fermi group.

Available: 2013-08-31

Data time period: 2009-10-01 to 2010-03-31

This dataset is part of a larger collection

Click to explore relationships graph
Subjects

User Contributed Tags    

Login to tag this record with meaningful keywords to make it easier to discover

ACN 633 798 857