If you use this software in a publication, please refer to its Astrophysics Source Code Library identifier:

    Bachetti, M. 2015, MaLTPyNT, Astrophysics Source Code Library, record ascl:1502.021.

In particular, if you use the cospectrum, please also refer to:

    Bachetti et al. 2015, ApJ , 800, 109.

@MISC{2015ascl.soft02021B,
   author = {{Bachetti}, M.},
    title = "{MaLTPyNT: Quick look timing analysis for NuSTAR data}",
 keywords = {Software},
howpublished = {Astrophysics Source Code Library},
     year = 2015,
    month = feb,
archivePrefix = "ascl",
   eprint = {1502.021},
   adsurl = {http://adsabs.harvard.edu/abs/2015ascl.soft02021B},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2015ApJ...800..109B,
   author = {{Bachetti}, M. and {Harrison}, F.~A. and {Cook}, R. and {Tomsick}, J. and
	{Schmid}, C. and {Grefenstette}, B.~W. and {Barret}, D. and
	{Boggs}, S.~E. and {Christensen}, F.~E. and {Craig}, W.~W. and
	{Fabian}, A.~C. and {F{\"u}rst}, F. and {Gandhi}, P. and {Hailey}, C.~J. and
	{Kara}, E. and {Maccarone}, T.~J. and {Miller}, J.~M. and {Pottschmidt}, K. and
	{Stern}, D. and {Uttley}, P. and {Walton}, D.~J. and {Wilms}, J. and
	{Zhang}, W.~W.},
    title = "{No Time for Dead Time: Timing Analysis of Bright Black Hole Binaries with NuSTAR}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1409.3248},
 primaryClass = "astro-ph.HE",
 keywords = {accretion, accretion disks, black hole physics, methods: data analysis, methods: statistical, X-rays: stars},
     year = 2015,
    month = feb,
   volume = 800,
      eid = {109},
    pages = {109},
      doi = {10.1088/0004-637X/800/2/109},
   adsurl = {http://adsabs.harvard.edu/abs/2015ApJ...800..109B},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

