| Type: | Package |
| 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. |
| Version: | 0.1 |
| Suggests: | roxygen2 |
| Depends: | R(≥ 4.0.0) |
| License: | CC0 |
| BugReports: | https://github.com/pachadotdev/cp1919/issues |
| URL: | https://github.com/pachadotdev/cp1919 |
| RoxygenNote: | 8.0.0 |
| Encoding: | UTF-8 |
| NeedsCompilation: | yes |
| LazyData: | true |
| Packaged: | 2026-06-24 10:37:37 UTC; pacha |
| Author: | Mauricio Vargas Sepulveda
 [aut, cre] |
| Maintainer: | Mauricio Vargas Sepulveda <m.vargas.sepulveda@gmail.com> |
| Repository: | CRAN |
| Date/Publication: | 2026-06-30 11:10:08 UTC |
cp1919: 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.
Author(s)
Maintainer: Mauricio Vargas Sepulveda m.vargas.sepulveda@gmail.com (ORCID)
Authors:
Mauricio Vargas Sepulveda m.vargas.sepulveda@gmail.com (ORCID)
See Also
Useful links:
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.
Usage
pulsar
Format
## 'pulsar' A data frame with 24,000 rows and 4 columns:
- measurement
Labels successive pulses. The dataset contains 80 consecutive radio pulses.
- time
The duration of individual, consecutive radio pulses emitted by the rotating neutron star CP 1919. Each pulse lasts about 0.04 seconds.
- radio_intensity
The peaks and troughs of each individual pulse.
Source
<https://www.proquest.com/docview/302499144/abstract?sourcetype=Dissertations
Examples
head(pulsar)