Citing GWpy¶

If you have used GWpy as part of a project that leads to a scientific publication, please acknowledge this by citing the GWpy paper: D. M. Macleod et al, SoftwareX, 13, 100657 (2021). The citation in various formats is given below:

BibTeX

@article{gwpy,
    title = "{GWpy: A Python package for gravitational-wave astrophysics}",
   author = {{Macleod}, D.~M. and {Areeda}, J.~S. and {Coughlin}, S.~B. and {Massinger}, T.~J. and {Urban}, A.~L.},
  journal = {SoftwareX},
   volume = 13,
    pages = 100657,
     year = 2021,
     issn = {2352-7110},
      doi = {10.1016/j.softx.2021.100657},
      url = {https://www.sciencedirect.com/science/article/pii/S2352711021000029},
}

RIS

TY  - JOUR
T1  - GWpy: A Python package for gravitational-wave astrophysics
AU  - Macleod, Duncan M.
AU  - Areeda, Joseph S.
AU  - Coughlin, Scott B.
AU  - Massinger, Thomas J.
AU  - Urban, Alexander L.
JO  - SoftwareX
VL  - 13
SP  - 100657
PY  - 2021
DA  - 2021/01/01/
SN  - 2352-7110
DO  - 10.1016/j.softx.2021.100657
UR  - https://www.sciencedirect.com/science/article/pii/S2352711021000029
ER  -

EndNode

%0 Journal Article
%T GWpy: A Python package for gravitational-wave astrophysics
%A Macleod, Duncan M.
%A Areeda, Joseph S.
%A Coughlin, Scott B.
%A Massinger, Thomas J.
%A Urban, Alexander L.
%J SoftwareX
%V 13
%P 100657
%D 2021
%R 10.1016/j.softx.2021.100657
%@ 2352-7110

RefWorks

RT Journal
T1 GWpy: A Python package for gravitational-wave astrophysics
A1 Macleod, Duncan M.
A1 Areeda, Joseph S.
A1 Coughlin, Scott B.
A1 Massinger, Thomas J.
A1 Urban, Alexander L.
JF SoftwareX
VO 13
SP 100657
YR 2021
DO DOI: 10.1016/j.softx.2021.100657
SN 2352-7110

Also cite the DOI for the version of GWpy that you have used. Each of the DOIs below resolves a Zenodo record for that version. See the Export section on each page for formatted citations in a number of common styles.

The list below includes only the 10 most recent releases of GWpy. For older versions, please click here.

Citing GWpy¶

2.1.3¶

2.1.2¶

2.1.1¶

2.1.0¶

2.0.4¶

2.0.3¶

2.0.2¶

2.0.1¶

2.0.0¶

1.0.1¶