@misc{crichton2021hydrogen,
  abstract = {The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a radio
interferometer array currently in development, with an initial 256-element
array to be deployed at the South African Radio Astronomy Observatory (SARAO)
Square Kilometer Array (SKA) site in South Africa. Each of the 6~m, $f/0.23$
dishes will be instrumented with dual-polarisation feeds operating over a
frequency range of 400-800 MHz. Through intensity mapping of the 21 cm emission
line of neutral hydrogen, HIRAX will provide a cosmological survey of the
distribution of large-scale structure over the redshift range of $0.775 < z <
2.55$ over $\sim$15,000 square degrees of the southern sky. The statistical
power of such a survey is sufficient to produce $\sim$7 percent constraints on
the dark energy equation of state parameter when combined with measurements
from the Planck satellite. Additionally, HIRAX will provide a highly
competitive platform for radio transient and HI absorber science while enabling
a multitude of cross-correlation studies. In these proceedings, we describe the
science goals of the experiment, overview of the design and status of the
sub-components of the telescope system, and describe the expected performance
of the initial 256-element array as well as the planned future expansion to the
final, 1024-element array.},
  added-at = {2021-09-29T18:03:45.000+0200},
  author = {Crichton, Devin and Aich, Moumita and Amara, Adam and Bandura, Kevin and Bassett, Bruce A. and Bengaly, Carlos and Berner, Pascale and Bhatporia, Shruti and Bucher, Martin and Chang, Tzu-Ching and Chiang, H. Cynthia and Cliche, Jean-Francois and Crichton, Carolyn and Dave, Romeel and de Villiers, Dirk I. L. and Dobbs, Matt A. and Ewall-Wice, Aaron M. and Eyono, Scott and Finlay, Christopher and Gaddam, Sindhu and Ganga, Ken and Gayley, Kevin G. and Gerodias, Kit and Gibbon, Tim and Gumba, Austin and Gupta, Neeraj and Harris, Maile and Heilgendorf, Heiko and Hilton, Matt and Hincks, Adam D. and Hitz, Pascal and Jalilvand, Mona and Julie, Roufurd and Kader, Zahra and Kania, Joseph and Karagiannis, Dionysios and Karastergiou, Aris and Kesebonye, Kabelo and Kittiwisit, Piyanat and Kneib, Jean-Paul and Knowles, Kenda and Kuhn, Emily R. and Kunz, Martin and Maartens, Roy and MacKay, Vincent and MacPherson, Stuart and Monstein, Christian and Moodley, Kavilan and Mugundhan, V. and Naidoo, Warren and Naidu, Arun and Newburgh, Laura B. and Nistane, Viraj and Di Nitto, Amanda and Ölçek, Deniz and Pan, Xinyu and Paul, Sourabh and Peterson, Jeffrey B. and Pieters, Elizabeth and Pieterse, Carla and Pillay, Aritha and Polish, Anna R. and Randrianjanahary, Liantsoa and Refregier, Alexandre and Renard, Andre and Retana-Montenegro, Edwin and Rout, Ian H. and Russeeawon, Cyndie and Sadr, Alireza Vafaei and Saliwanchik, Benjamin R. B. and Sampath, Ajith and Sanghavi, Pranav and Santos, Mario G. and Sengate, Onkabetse and Shaw, J. Richard and Sievers, Jonathan L. and Smirnov, Oleg M. and Smith, Kendrick M. and Sob, Ulrich Armel Mbou and Srianand, Raghunathan and Stronkhorst, Pieter and Sunder, Dhaneshwar D. and Tartakovsky, Simon and Taylor, Russ and Timbie, Peter and Tolley, Emma E. and Townsend, Junaid and Tyndall, Will and Ungerer, Cornelius and van Dyk, Jacques and van Vuuren, Gary and Vanderlinde, Keith and Viant, Thierry and Walters, Anthony and Wang, Jingying and Weltman, Amanda and Woudt, Patrick and Wulf, Dallas and Zavyalov, Anatoly and Zhang, Zheng},
  biburl = {https://www.bibsonomy.org/bibtex/2ac503763926579b8b2e8050fe45dfd82/gpkulkarni},
  description = {The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview},
  interhash = {fe7bd2a0ac1a22a9a16365b2b27b99bf},
  intrahash = {ac503763926579b8b2e8050fe45dfd82},
  keywords = {library},
  note = {cite arxiv:2109.13755Comment: 23 pages, 6 figures. Submitted to the Journal of Astronomical  Telescopes, Instruments, and Systems (JATIS), SKA Observatory special section},
  timestamp = {2021-09-29T18:03:45.000+0200},
  title = {The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element
  Array Status and Overview},
  url = {http://arxiv.org/abs/2109.13755},
  year = 2021
}

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The statistical power of such a survey is sufficient to produce $∼$7 percent constraints on the dark energy equation of state parameter when combined with measurements from the Planck satellite. Additionally, HIRAX will provide a highly competitive platform for radio transient and HI absorber science while enabling a multitude of cross-correlation studies. 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Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview","interhash":"fe7bd2a0ac1a22a9a16365b2b27b99bf","intrahash":"ac503763926579b8b2e8050fe45dfd82","keywords":"library","note":"cite arxiv:2109.13755Comment: 23 pages, 6 figures. Submitted to the Journal of Astronomical Telescopes, Instruments, and Systems (JATIS), SKA Observatory special section","timestamp":"2021-09-29T18:03:45.000+0200","title":"The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview","url":"http://arxiv.org/abs/2109.13755","year":"2021","bibtex":"@misc{crichton2021hydrogen,\n abstract = {The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a radio\r\ninterferometer array currently in development, with an initial 256-element\r\narray to be deployed at the South African Radio Astronomy Observatory (SARAO)\r\nSquare Kilometer Array (SKA) site in South Africa. Each of the 6~m, $f/0.23$\r\ndishes will be instrumented with dual-polarisation feeds operating over a\r\nfrequency range of 400-800 MHz. Through intensity mapping of the 21 cm emission\r\nline of neutral hydrogen, HIRAX will provide a cosmological survey of the\r\ndistribution of large-scale structure over the redshift range of $0.775 < z <\r\n2.55$ over $\\sim$15,000 square degrees of the southern sky. The statistical\r\npower of such a survey is sufficient to produce $\\sim$7 percent constraints on\r\nthe dark energy equation of state parameter when combined with measurements\r\nfrom the Planck satellite. Additionally, HIRAX will provide a highly\r\ncompetitive platform for radio transient and HI absorber science while enabling\r\na multitude of cross-correlation studies. In these proceedings, we describe the\r\nscience goals of the experiment, overview of the design and status of the\r\nsub-components of the telescope system, and describe the expected performance\r\nof the initial 256-element array as well as the planned future expansion to the\r\nfinal, 1024-element array.},\n added-at = {2021-09-29T18:03:45.000+0200},\n author = {Crichton, Devin and Aich, Moumita and Amara, Adam and Bandura, Kevin and Bassett, Bruce A. and Bengaly, Carlos and Berner, Pascale and Bhatporia, Shruti and Bucher, Martin and Chang, Tzu-Ching and Chiang, H. Cynthia and Cliche, Jean-Francois and Crichton, Carolyn and Dave, Romeel and de Villiers, Dirk I. L. and Dobbs, Matt A. and Ewall-Wice, Aaron M. and Eyono, Scott and Finlay, Christopher and Gaddam, Sindhu and Ganga, Ken and Gayley, Kevin G. and Gerodias, Kit and Gibbon, Tim and Gumba, Austin and Gupta, Neeraj and Harris, Maile and Heilgendorf, Heiko and Hilton, Matt and Hincks, Adam D. and Hitz, Pascal and Jalilvand, Mona and Julie, Roufurd and Kader, Zahra and Kania, Joseph and Karagiannis, Dionysios and Karastergiou, Aris and Kesebonye, Kabelo and Kittiwisit, Piyanat and Kneib, Jean-Paul and Knowles, Kenda and Kuhn, Emily R. and Kunz, Martin and Maartens, Roy and MacKay, Vincent and MacPherson, Stuart and Monstein, Christian and Moodley, Kavilan and Mugundhan, V. and Naidoo, Warren and Naidu, Arun and Newburgh, Laura B. and Nistane, Viraj and Di Nitto, Amanda and Ölçek, Deniz and Pan, Xinyu and Paul, Sourabh and Peterson, Jeffrey B. and Pieters, Elizabeth and Pieterse, Carla and Pillay, Aritha and Polish, Anna R. and Randrianjanahary, Liantsoa and Refregier, Alexandre and Renard, Andre and Retana-Montenegro, Edwin and Rout, Ian H. and Russeeawon, Cyndie and Sadr, Alireza Vafaei and Saliwanchik, Benjamin R. B. and Sampath, Ajith and Sanghavi, Pranav and Santos, Mario G. and Sengate, Onkabetse and Shaw, J. Richard and Sievers, Jonathan L. and Smirnov, Oleg M. and Smith, Kendrick M. and Sob, Ulrich Armel Mbou and Srianand, Raghunathan and Stronkhorst, Pieter and Sunder, Dhaneshwar D. and Tartakovsky, Simon and Taylor, Russ and Timbie, Peter and Tolley, Emma E. and Townsend, Junaid and Tyndall, Will and Ungerer, Cornelius and van Dyk, Jacques and van Vuuren, Gary and Vanderlinde, Keith and Viant, Thierry and Walters, Anthony and Wang, Jingying and Weltman, Amanda and Woudt, Patrick and Wulf, Dallas and Zavyalov, Anatoly and Zhang, Zheng},\n biburl = {https://www.bibsonomy.org/bibtex/2ac503763926579b8b2e8050fe45dfd82/gpkulkarni},\n description = {The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview},\n interhash = {fe7bd2a0ac1a22a9a16365b2b27b99bf},\n intrahash = {ac503763926579b8b2e8050fe45dfd82},\n keywords = {library},\n note = {cite arxiv:2109.13755Comment: 23 pages, 6 figures. 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