| Title: | Radio Observations of the Pulse Profiles and Dispersion Measures of Twelve Pulsars |
|---|---|
| Description: | Successive pulses from CP 1919, the first pulsar discovered. The pulses occur every 1.337 seconds. They are caused by rapidly spinning neutron star. |
| Authors: | Mauricio Vargas Sepulveda [aut, cre] (ORCID: <https://orcid.org/0000-0003-1017-7574>) |
| Maintainer: | Mauricio Vargas Sepulveda <[email protected]> |
| License: | CC0 |
| Version: | 0.1 |
| Built: | 2026-06-30 16:48:56 UTC |
| Source: | https://github.com/cran/cp1919 |
Successive pulses from CP 1919, the first pulsar discovered. The pulses occur every 1.337 seconds. They are caused by rapidly spinning neutron star.
pulsarpulsar
## 'pulsar' A data frame with 24,000 rows and 4 columns:
Labels successive pulses. The dataset contains 80 consecutive radio pulses.
The duration of individual, consecutive radio pulses emitted by the rotating neutron star CP 1919. Each pulse lasts about 0.04 seconds.
The peaks and troughs of each individual pulse.
<https://www.proquest.com/docview/302499144/abstract?sourcetype=Dissertations
head(pulsar)head(pulsar)