Instrument Overview of Taurus: A Balloon-borne CMB and Dust Polarization Experiment

Autor: May, Jared L., Adler, Alexandre E., Austermann, Jason E., Benton, Steven J., Bihary, Rick, Durkin, Malcolm, Duff, Shannon M., Filippini, Jeffrey P., Fraisse, Aurelien A., Gascard, Thomas J. L. J., Gibbs, Sho M., Gourapura, Suren, Gudmundsson, Jon E., Hartley, John W., Hubmayr, Johannes, Jones, William C., Li, Steven, Nagy, Johanna M., Okun, Kate, Padilla, Ivan L., Romualdez, L. Javier, Tartakovsky, Simon, Vissers, Michael R.

Taurus is a balloon-borne cosmic microwave background (CMB) experiment optimized to map the E-mode polarization and Galactic foregrounds at the largest angular scales ($\ell$ $\lt$ 30) and improve measurements of the optical depth to reionization ($\

Externí odkaz: http://arxiv.org/abs/2407.01438

The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview

Autor: Crichton, Devin, Aich, Moumita, Amara, Adam, Bandura, Kevin, Bassett, Bruce A., Bengaly, Carlos, Berner, Pascale, Bhatporia, Shruti, Bucher, Martin, Chang, Tzu-Ching, Chiang, H. Cynthia, Cliche, Jean-Francois, Crichton, Carolyn, Dave, Romeel, de Villiers, Dirk I. L., Dobbs, Matt A., Ewall-Wice, Aaron M., Eyono, Scott, Finlay, Christopher, Gaddam, Sindhu, Ganga, Ken, Gayley, Kevin G., Gerodias, Kit, Gibbon, Tim, Gumba, Austin, Gupta, Neeraj, Harris, Maile, Heilgendorf, Heiko, Hilton, Matt, Hincks, Adam D., Hitz, Pascal, Jalilvand, Mona, Julie, Roufurd, Kader, Zahra, Kania, Joseph, Karagiannis, Dionysios, Karastergiou, Aris, Kesebonye, Kabelo, Kittiwisit, Piyanat, Kneib, Jean-Paul, Knowles, Kenda, Kuhn, Emily R., Kunz, Martin, Maartens, Roy, MacKay, Vincent, MacPherson, Stuart, Monstein, Christian, Moodley, Kavilan, Mugundhan, V., Naidoo, Warren, Naidu, Arun, Newburgh, Laura B., Nistane, Viraj, Di Nitto, Amanda, Ölçek, Deniz, Pan, Xinyu, Paul, Sourabh, Peterson, Jeffrey B., Pieters, Elizabeth, Pieterse, Carla, Pillay, Aritha, Polish, Anna R., Randrianjanahary, Liantsoa, Refregier, Alexandre, Renard, Andre, Retana-Montenegro, Edwin, Rout, Ian H., Russeeawon, Cyndie, Sadr, Alireza Vafaei, Saliwanchik, Benjamin R. B., Sampath, Ajith, Sanghavi, Pranav, Santos, Mario G., Sengate, Onkabetse, Shaw, J. Richard, Sievers, Jonathan L., Smirnov, Oleg M., Smith, Kendrick M., Sob, Ulrich Armel Mbou, Srianand, Raghunathan, Stronkhorst, Pieter, Sunder, Dhaneshwar D., Tartakovsky, Simon, Taylor, Russ, Timbie, Peter, Tolley, Emma E., Townsend, Junaid, Tyndall, Will, Ungerer, Cornelius, van Dyk, Jacques, van Vuuren, Gary, Vanderlinde, Keith, Viant, Thierry, Walters, Anthony, Wang, Jingying, Weltman, Amanda, Woudt, Patrick, Wulf, Dallas, Zavyalov, Anatoly, Zhang, Zheng

Publikováno v: J. of Astronomical Telescopes, Instruments, and Systems, 8(1), 011019 (2022)

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 Arra

Externí odkaz: http://arxiv.org/abs/2109.13755

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.

Hydrogen Intensity and Real-Time Analysis Experiment: 256-element array status and overview

Autor: Crichton, Devin, Aich, Moumita, Amara, Adam, Bandura, Kevin, Bassett, Bruce A., Bengaly, Carlos, Berner, Pascale, Bhatporia, Shruti, Bucher, Martin, Chang, Tzu-Ching, Chiang, H. Cynthia, Cliche, Jean-Francois, Crichton, Carolyn, Dave, Romeel, De Villiers, Dirk I. L., Dobbs, Matt, Ewall-Wice, Aaron M., Eyono, Scott, Finlay, Christopher, Gaddam, Sindhu, Ganga, Ken, Gayley, Kevin G., Gerodias, Kit, Gibbon, Tim B., Gumba, Austine, Gupta, Neeraj, Harris, Maile, Heilgendorff, Heiko, Hilton, Matt, Hincks, Adam D., Hitz, Pascal, Jalilvand, Mona, Julie, Roufurd P. M., Kader, Zahra, Kania, Joseph, Karagiannis, Dionysios, Karastergiou, Aris, Kesebonye, Kabelo, Kittiwisit, Piyanat, Kneib, Jean-Paul, Knowles, Kenda, Kuhn, Emily R., Kunz, Martin, Maartens, Roy, MacKay, Vincent, MacPherson, Stuart, Monstein, Christian, Moodley, Kavilan, Mugundhan, V., Naidoo, Warren, Naidu, Arun, Newburgh, Laura B., Nistane, Viraj, Di Nitto, Amanda, Ölçek, Deniz, Pan, Xinyu, Paul, Sourabh, Peterson, Jeffrey B., Pieters, Elizabeth, Pieterse, Carla, Pillay, Aritha, Polish, Anna R., Randrianjanahary, Liantsoa, Refregier, Alexandre, Renard, Andre, Retana-Montenegro, Edwin, Rout, Ian H., Russeeawon, Cyndie, Sadr, Alireza Vafaei, Saliwanchik, Benjamin R. B., Sampath, Ajith, Sanghavi, Pranav, Santos, Mario G., Sengate, Onkabetse, Shaw, J. Richard, Sievers, Jonathan L., Smirnov, Oleg M., Smith, Kendrick M., Sob, Ulrich Armel Mbou, Srianand, Raghunathan, Stronkhorst, Pieter, Sunder, Dhaneshwar D., Tartakovsky, Simon, Taylor, Russ, Timbie, Peter, Tolley, Emma E., Townsend, Junaid, Tyndall, Will, Ungerer, Cornelius, van Dyk, Jacques, van Vuuren, Gary, Vanderlinde, Keith, Viant, Thierry, Walters, Anthony, Wang, Jingying, Weltman, Amanda, Woudt, Patrick, Wulf, Dallas, Zavyalov, Anatoly, Zhang, Zheng

Publikováno v: Journal of Astronomical Telescopes, Instruments, and Systems; November 2021, Vol. 8 Issue: 1 p011019-011019, 1p