Package {cp1919}

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:

• https://github.com/pachadotdev/cp1919

• Report bugs at https://github.com/pachadotdev/cp1919/issues

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)