@Book{Crochiere1996,
author = {Ronald E. Crochiere
and Lawrence R. Rabiner},
title = {Multirate Digital Signal Processing},
year = {1996},
isbn = {0136051626},
publisher = {Prentice Hall PTR},
address = {USA},
edition = {1st},
abstract = {From the Publisher:This title is no longer being mass-produced. It is now being printed on demand by the publisher. While this process keeps information readily available, the print quality of these books is generally that of a copier and not of a normal book. This is a copy of the original book. Intended for a one-semester advanced graduate course in digitalsignal processing or as a reference for practicing engineers andresearchers.}
}

@Article{Harris2020,
author={Harris, Charles R.
and Millman, K. Jarrod
and van der Walt, St{\'e}fan J.
and Gommers, Ralf
and Virtanen, Pauli
and Cournapeau, David
and Wieser, Eric
and Taylor, Julian
and Berg, Sebastian
and Smith, Nathaniel J.
and Kern, Robert
and Picus, Matti
and Hoyer, Stephan
and van Kerkwijk, Marten H.
and Brett, Matthew
and Haldane, Allan
and del R{\'i}o, Jaime Fern{\'a}ndez
and Wiebe, Mark
and Peterson, Pearu
and G{\'e}rard-Marchant, Pierre
and Sheppard, Kevin
and Reddy, Tyler
and Weckesser, Warren
and Abbasi, Hameer
and Gohlke, Christoph
and Oliphant, Travis E.},
title={Array programming with NumPy},
journal={Nature},
year={2020},
month={Sep},
day={01},
volume={585},
number={7825},
pages={357-362},
abstract={Array programming provides a powerful, compact and expressive syntax for accessing, manipulating and operating on data in vectors, matrices and higher-dimensional arrays. NumPy is the primary array programming library for the Python language. It has an essential role in research analysis pipelines in fields as diverse as physics, chemistry, astronomy, geoscience, biology, psychology, materials science, engineering, finance and economics. For example, in astronomy, NumPy was an important part of the software stack used in the discovery of gravitational waves1 and in the first imaging of a black hole2. Here we review how a few fundamental array concepts lead to a simple and powerful programming paradigm for organizing, exploring and analysing scientific data. NumPy is the foundation upon which the scientific Python ecosystem is constructed. It is so pervasive that several projects, targeting audiences with specialized needs, have developed their own NumPy-like interfaces and array objects. Owing to its central position in the ecosystem, NumPy increasingly acts as an interoperability layer between such array computation libraries and, together with its application programming interface (API), provides a flexible framework to support the next decade of scientific and industrial analysis.},
issn={1476-4687},
doi={10.1038/s41586-020-2649-2},
url={https://doi.org/10.1038/s41586-020-2649-2}
}

@Article{Hunter:2007,
  Author    = {Hunter, J. D.},
  Title     = {Matplotlib: A 2D graphics environment},
  Journal   = {Computing in Science \& Engineering},
  Volume    = {9},
  Number    = {3},
  Pages     = {90--95},
  abstract  = {Matplotlib is a 2D graphics package used for Python for
  application development, interactive scripting, and publication-quality
  image generation across user interfaces and operating systems.},
  publisher = {IEEE COMPUTER SOC},
  doi       = {10.1109/MCSE.2007.55},
  year      = 2007
}

@Book{Price:2021,
  author      = "Danny C. Price",
  title       = "Spectrometers and Polyphase Filterbanks in Radio Astronomy",
  editor      = "David N. Burrows",
  booktitle   = "The WSPC Handbook of Astronomical Instrumentation",
  publisher   = "World Scientific",
  series      = "World Scientific Series in Astrophysics",
  year        = 2021,
  volume      = 1,
  doi         = {10.1142/9446}
}

@Book{Dillinger:2003,
  author      = "Markus Dillinger, Kambiz Madani, Nancy Alonistioti",
  booktitle   = "Software Defined Radio: Architectures, Systems and Functions",
  publisher   = "John Wiley & Sons",
  series      = "Wiley Series in Software Radio",
  year        = 2003,
  volume      = 1,
  isbn        = {0470851643}
}

@article{astropy:2013,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...558A..33A},
Archiveprefix = {arXiv},
Author = {{Astropy Collaboration} and {Robitaille}, T.~P. and {Tollerud}, E.~J. and {Greenfield}, P. and {Droettboom}, M. and {Bray}, E. and {Aldcroft}, T. and {Davis}, M. and {Ginsburg}, A. and {Price-Whelan}, A.~M. and {Kerzendorf}, W.~E. and {Conley}, A. and {Crighton}, N. and {Barbary}, K. and {Muna}, D. and {Ferguson}, H. and {Grollier}, F. and {Parikh}, M.~M. and {Nair}, P.~H. and {Unther}, H.~M. and {Deil}, C. and {Woillez}, J. and {Conseil}, S. and {Kramer}, R. and {Turner}, J.~E.~H. and {Singer}, L. and {Fox}, R. and {Weaver}, B.~A. and {Zabalza}, V. and {Edwards}, Z.~I. and {Azalee Bostroem}, K. and {Burke}, D.~J. and {Casey}, A.~R. and {Crawford}, S.~M. and {Dencheva}, N. and {Ely}, J. and {Jenness}, T. and {Labrie}, K. and {Lim}, P.~L. and {Pierfederici}, F. and {Pontzen}, A. and {Ptak}, A. and {Refsdal}, B. and {Servillat}, M. and {Streicher}, O.},
Doi = {10.1051/0004-6361/201322068},
Eid = {A33},
Eprint = {1307.6212},
Journal = {\aap},
Keywords = {methods: data analysis, methods: miscellaneous, virtual observatory tools},
Month = oct,
Pages = {A33},
Primaryclass = {astro-ph.IM},
Title = {{Astropy: A community Python package for astronomy}},
Volume = 558,
Year = 2013,
Bdsk-Url-1 = {https://dx.doi.org/10.1051/0004-6361/201322068}}

@ARTICLE{astropy:2018,
       author = {{Astropy Collaboration} and {Price-Whelan}, A.~M. and
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         {Crawford}, S.~M. and {Conseil}, S. and {Shupe}, D.~L. and
         {Craig}, M.~W. and {Dencheva}, N. and {Ginsburg}, A. and {Vand
        erPlas}, J.~T. and {Bradley}, L.~D. and {P{'e}rez-Su{'a}rez}, D. and
         {de Val-Borro}, M. and {Aldcroft}, T.~L. and {Cruz}, K.~L. and
         {Robitaille}, T.~P. and {Tollerud}, E.~J. and {Ardelean}, C. and
         {Babej}, T. and {Bach}, Y.~P. and {Bachetti}, M. and {Bakanov}, A.~V. and
         {Bamford}, S.~P. and {Barentsen}, G. and {Barmby}, P. and
         {Baumbach}, A. and {Berry}, K.~L. and {Biscani}, F. and {Boquien}, M. and
         {Bostroem}, K.~A. and {Bouma}, L.~G. and {Brammer}, G.~B. and
         {Bray}, E.~M. and {Breytenbach}, H. and {Buddelmeijer}, H. and
         {Burke}, D.~J. and {Calderone}, G. and {Cano Rodr{'i}guez}, J.~L. and
         {Cara}, M. and {Cardoso}, J.~V.~M. and {Cheedella}, S. and {Copin}, Y. and
         {Corrales}, L. and {Crichton}, D. and {D'Avella}, D. and {Deil}, C. and
         {Depagne}, {'E}. and {Dietrich}, J.~P. and {Donath}, A. and
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         {Ferreira}, L.~A. and {Finethy}, T. and {Fox}, R.~T. and
         {Garrison}, L.~H. and {Gibbons}, S.~L.~J. and {Goldstein}, D.~A. and
         {Gommers}, R. and {Greco}, J.~P. and {Greenfield}, P. and
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         {Kulkarni}, A.~M. and {Kumar}, A. and {Lee}, A. and {Lenz}, D. and
         {Littlefair}, S.~P. and {Ma}, Z. and {Macleod}, D.~M. and
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         {Morris}, B.~M. and {Mueller}, M. and {Mumford}, S.~J. and {Muna}, D. and
         {Murphy}, N.~A. and {Nelson}, S. and {Nguyen}, G.~H. and
         {Ninan}, J.~P. and {N{"o}the}, M. and {Ogaz}, S. and {Oh}, S. and
         {Parejko}, J.~K. and {Parley}, N. and {Pascual}, S. and {Patil}, R. and
         {Patil}, A.~A. and {Plunkett}, A.~L. and {Prochaska}, J.~X. and
         {Rastogi}, T. and {Reddy Janga}, V. and {Sabater}, J. and
         {Sakurikar}, P. and {Seifert}, M. and {Sherbert}, L.~E. and
         {Sherwood-Taylor}, H. and {Shih}, A.~Y. and {Sick}, J. and
         {Silbiger}, M.~T. and {Singanamalla}, S. and {Singer}, L.~P. and
         {Sladen}, P.~H. and {Sooley}, K.~A. and {Sornarajah}, S. and
         {Streicher}, O. and {Teuben}, P. and {Thomas}, S.~W. and
         {Tremblay}, G.~R. and {Turner}, J.~E.~H. and {Terr{'o}n}, V. and
         {van Kerkwijk}, M.~H. and {de la Vega}, A. and {Watkins}, L.~L. and
         {Weaver}, B.~A. and {Whitmore}, J.~B. and {Woillez}, J. and
         {Zabalza}, V. and {Astropy Contributors}},
        title = "{The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package}",
      journal = {aj},
     keywords = {methods: data analysis, methods: miscellaneous, methods: statistical, reference systems, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = sep,
       volume = {156},
       number = {3},
          eid = {123},
        pages = {123},
          doi = {10.3847/1538-3881/aabc4f},
archivePrefix = {arXiv},
       eprint = {1801.02634},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018AJ....156..123A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Kalberla2005,
  doi = {10.1051/0004-6361:20041864},
  url = {https://doi.org/10.1051/0004-6361:20041864},
  year = {2005},
  month = sep,
  publisher = {{EDP} Sciences},
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  number = {2},
  pages = {775--782},
  author = {P. M. W. Kalberla and W. B. Burton and Dap Hartmann and E. M. Arnal and E. Bajaja and R. Morras and W. G. L. P\"{o}ppel},
  title = {The Leiden/Argentine/Bonn ({LAB}) Survey of Galactic {HI}},
  journal = {Astronomy {\&} Astrophysics}
}

@ARTICLE{Pence2010,
       author = {{Pence}, W.~D. and {Chiappetti}, L. and {Page}, C.~G. and {Shaw}, R.~A. and {Stobie}, E.},
        title = "{Definition of the Flexible Image Transport System (FITS), version 3.0}",
      journal = {\aap},
     keywords = {instrumentation: miscellaneous, methods: miscellaneous, techniques: miscellaneous, reference systems, standards, astronomical databases: miscellaneous},
         year = 2010,
        month = dec,
       volume = {524},
          eid = {A42},
        pages = {A42},
          doi = {10.1051/0004-6361/201015362},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010A&A...524A..42P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
