skip to main content
US FlagAn official website of the United States government
dot gov icon
Official websites use .gov
A .gov website belongs to an official government organization in the United States.
https lock icon
Secure .gov websites use HTTPS
A lock ( lock ) or https:// means you've safely connected to the .gov website. Share sensitive information only on official, secure websites.

Explore Research Products in the PAR
It may take a few hours for recently added research products to appear in PAR search results.


  • Home
  • Search Results
  • Page 1 of 1

Search for: All records

Creators/Authors contains: "Capano, Collin D"

Note: When clicking on a Digital Object Identifier (DOI) number, you will be taken to an external site maintained by the publisher. Some full text articles may not yet be available without a charge during the embargo (administrative interval).
What is a DOI Number?

Some links on this page may take you to non-federal websites. Their policies may differ from this site.

  1. ; ; ; ; ; ; ; (, Physical Review D)
    Full Text Available 
  2. ; ; ; ; ; ; ; ; (, Computing in Science & Engineering)
    Full Text Available 
  3. ; ; ; (, Neural Computing and Applications)
    null (Ed.)
    Full Text Available 
  4. ; ; ; ; (, Physical Review D)
    null (Ed.)
    Full Text Available 
  5. ; ; ; ; ; ; ; ; (, Nature Astronomy)
    null (Ed.)
    Full Text Available 
  6. ; ; ; (, Journal of Cosmology and Astroparticle Physics)
    Full Text Available 
  7. ; ; ; ; (, Scientific Data)
    Abstract This paper presents a parameter estimation analysis of the seven binary black hole mergers—GW170104, GW170608, GW170729, GW170809, GW170814, GW170818, and GW170823—detected during the second observing run of the Advanced LIGO and Virgo observatories using the gravitational-wave open data. We describe the methodology for parameter estimation of compact binaries using gravitational-wave data, and we present the posterior distributions of the inferred astrophysical parameters. We release our samples of the posterior probability density function with tutorials on using and replicating our results presented in this paper. 
    more » « less
  8. ; ; ; ; ; ; (, Publications of the Astronomical Society of the Pacific)
    Full Text Available