期刊
ASTRONOMICAL JOURNAL
卷 139, 期 1, 页码 168-175出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/139/1/168
关键词
polarization; pulsars: general
资金
- National Science Foundation [AST-8917722, AST-9618408, AST-9986754, AST-0139641.]
We present Arecibo time-aligned, total intensity profiles for 46 pulsars over an unusually wide range of radio frequencies and multi-frequency, polarization-angle density diagrams, and/or polarization profiles for 57 pulsars at some or all of the frequencies 50, 111/130, 430, and 1400 MHz. The frequency-dependent dispersion delay has been removed in order to align the profiles for study of their spectral evolution, and wherever possible the profiles of each pulsar are displayed on the same longitude scale. Most of the pulsars within Arecibo's declination range that are sufficiently bright for such spectral or single pulse analysis are included in this survey. The calibrated single pulse sequences and average profiles are available by web download for further study.
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