File:Correlation vs angular separation between pulsars.svg

From Wikimedia Commons, the free media repository
Jump to navigation Jump to search

Original file (SVG file, nominally 512 × 341 pixels, file size: 6 KB)

Captions

Captions

Add a one-line explanation of what this file represents

Summary

[edit]
Description Plot of correlation between pulsars observed by NANOGrav vs angular separation between pulsars, compared with a theoretical model (dashed purple) and if there were no gravitational wave background (solid green) by CMG Lee based on http://iopscience.iop.org/collections/apjl-230623-245-Focus-on-NANOGrav-15-year and http://news.berkeley.edu/2023/06/28/after-15-years-pulsar-timing-yields-evidence-of-cosmic-gravitational-wave-background .
Source Own work
Author Cmglee

Licensing

[edit]
I, the copyright holder of this work, hereby publish it under the following licenses:
w:en:Creative Commons
attribution share alike
This file is licensed under the Creative Commons Attribution-Share Alike 4.0 International license.
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
  • share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.
You may select the license of your choice.

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current00:24, 2 July 2023Thumbnail for version as of 00:24, 2 July 2023512 × 341 (6 KB)Cmglee (talk | contribs)Lighten grid
23:48, 1 July 2023Thumbnail for version as of 23:48, 1 July 2023512 × 341 (6 KB)Cmglee (talk | contribs)Try to work around new librsvg bug
23:46, 1 July 2023Thumbnail for version as of 23:46, 1 July 2023512 × 341 (6 KB)Cmglee (talk | contribs){{Information |Description=Plot of correlation between pulsars observed by NANOGrav vs angular separation between pulsars, compared with a theoretical model (dashed purple) and if there were no gravitational wave background (solid green) by CMG Lee based on http://iopscience.iop.org/collections/apjl-230623-245-Focus-on-NANOGrav-15-year and http://news.berkeley.edu/2023/06/28/after-15-years-pulsar-timing-yields-evidence-of-cosmic-gravitational-wave-background . |Source={{own}} |Date= |Author=...

You cannot overwrite this file.

There are no pages that use this file.

File usage on other wikis

Metadata

This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.

Retrieved from "https://commons.wikimedia.org/w/index.php?title=File:Correlation_vs_angular_separation_between_pulsars.svg&oldid=895676910"