Cmb-hd: Astro2020 RFI Response

Neelima Sehgal; Simone Aiola; Yashar Akrami; Kaustuv moni Basu; Michael Boylan-Kolchin; Sean Bryan; Caitlin M Casey; Sébastien Clesse; Francis-Yan Cyr-Racine; Luca Di Mascolo; Simon Dicker; Thomas Essinger-Hileman; Simone Ferraro; George Fuller; Nicholas Galitzki; Dongwon Han; Matthew Hasselfield; Gil Holder; Bhuvnesh Jain; Bradley R. Johnson; Matthew Johnson; Pamela Klaassen; Amanda MacInnis; Mathew Madhavacheril; Philip Mauskopf; Daan Meerburg; Joel Meyers; Tony Mroczkowski; Suvodip Mukherjee; Moritz Münchmeyer; Sigurd Kirkevold Naess; Daisuke Nagai; Toshiya Namikawa; Laura Newburgh; Nam Nguyen; Michael Niemack; Benjamin D. Oppenheimer; Elena Pierpaoli; Emmanuel Schaan; Blake Sherwin; Anže Slosar; David Spergel; Eric Switzer; Pranjal Trivedi; Yu-Dai Tsai; Alexander van Engelen; Benjamin Wandelt; Edward Wollack

doi:10.48550/arXiv.2002.12714

Cmb-hd: Astro2020 RFI Response

Neelima Sehgal, Simone Aiola, Yashar Akrami, Kaustuv moni Basu, Michael Boylan-Kolchin, Sean Bryan, Caitlin M Casey, Sébastien Clesse, Francis-Yan Cyr-Racine, Luca Di Mascolo, Simon Dicker, Thomas Essinger-Hileman, Simone Ferraro, George Fuller, Nicholas Galitzki, Dongwon Han, Matthew Hasselfield, Gil Holder, Bhuvnesh Jain, Bradley R. JohnsonMatthew Johnson, Pamela Klaassen, Amanda MacInnis, Mathew Madhavacheril, Philip Mauskopf, Daan Meerburg, Joel Meyers, Tony Mroczkowski, Suvodip Mukherjee, Moritz Münchmeyer, Sigurd Kirkevold Naess, Daisuke Nagai, Toshiya Namikawa, Laura Newburgh, Nam Nguyen, Michael Niemack, Benjamin D. Oppenheimer, Elena Pierpaoli, Emmanuel Schaan, Blake Sherwin, Anže Slosar, David Spergel, Eric Switzer, Pranjal Trivedi, Yu-Dai Tsai, Alexander van Engelen, Benjamin Wandelt, Edward Wollack

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CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both fundamental physics of the Universe and astrophysics. This survey would be delivered in 7.5 years of observing 20,000 square degrees, using two new 30-meter-class off-axis cross-Dragone telescopes to be located at Cerro Toco in the Atacama Desert. Each telescope would field 800,000 detectors (200,000 pixels), for a total of 1.6 million detectors.

Originele taal-2	English
DOI's	https://doi.org/10.48550/arXiv.2002.12714
Status	Submitted - 28-feb.-2020
Extern gepubliceerd	Ja

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@techreport{15fa381ac8ce4927af28f741e4671460,

title = "Cmb-hd: Astro2020 RFI Response",

abstract = " CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both fundamental physics of the Universe and astrophysics. This survey would be delivered in 7.5 years of observing 20,000 square degrees, using two new 30-meter-class off-axis cross-Dragone telescopes to be located at Cerro Toco in the Atacama Desert. Each telescope would field 800,000 detectors (200,000 pixels), for a total of 1.6 million detectors. ",

keywords = "astro-ph.CO, astro-ph.IM, hep-ph",

author = "Neelima Sehgal and Simone Aiola and Yashar Akrami and Basu, {Kaustuv moni} and Michael Boylan-Kolchin and Sean Bryan and Casey, {Caitlin M} and S{\'e}bastien Clesse and Francis-Yan Cyr-Racine and Mascolo, {Luca Di} and Simon Dicker and Thomas Essinger-Hileman and Simone Ferraro and George Fuller and Nicholas Galitzki and Dongwon Han and Matthew Hasselfield and Gil Holder and Bhuvnesh Jain and Johnson, {Bradley R.} and Matthew Johnson and Pamela Klaassen and Amanda MacInnis and Mathew Madhavacheril and Philip Mauskopf and Daan Meerburg and Joel Meyers and Tony Mroczkowski and Suvodip Mukherjee and Moritz M{\"u}nchmeyer and Naess, {Sigurd Kirkevold} and Daisuke Nagai and Toshiya Namikawa and Laura Newburgh and Nam Nguyen and Michael Niemack and Oppenheimer, {Benjamin D.} and Elena Pierpaoli and Emmanuel Schaan and Blake Sherwin and An{\v z}e Slosar and David Spergel and Eric Switzer and Pranjal Trivedi and Yu-Dai Tsai and Engelen, {Alexander van} and Benjamin Wandelt and Edward Wollack",

note = "Response to request for information (RFI) by the Panel of Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Astro2020 Decadal Survey regarding the CMB-HD APC (arXiv:1906.10134). Note some text overlap with original APC. Note also detector count and cost have been reduced by 1/3, and observing time increased by 1/3 compared to original APC; science goals expanded",

year = "2020",

month = feb,

day = "28",

doi = "10.48550/arXiv.2002.12714",

language = "English",

type = "WorkingPaper",

}

Sehgal, N, Aiola, S, Akrami, Y, Basu, KM, Boylan-Kolchin, M, Bryan, S, Casey, CM, Clesse, S, Cyr-Racine, F-Y, Mascolo, LD, Dicker, S, Essinger-Hileman, T, Ferraro, S, Fuller, G, Galitzki, N, Han, D, Hasselfield, M, Holder, G, Jain, B, Johnson, BR, Johnson, M, Klaassen, P, MacInnis, A, Madhavacheril, M, Mauskopf, P, Meerburg, D, Meyers, J, Mroczkowski, T, Mukherjee, S, Münchmeyer, M, Naess, SK, Nagai, D, Namikawa, T, Newburgh, L, Nguyen, N, Niemack, M, Oppenheimer, BD, Pierpaoli, E, Schaan, E, Sherwin, B, Slosar, A, Spergel, D, Switzer, E, Trivedi, P, Tsai, Y-D, Engelen, AV, Wandelt, B & Wollack, E 2020 'Cmb-hd: Astro2020 RFI Response'. https://doi.org/10.48550/arXiv.2002.12714

TY - UNPB

T1 - Cmb-hd

T2 - Astro2020 RFI Response

AU - Sehgal, Neelima

AU - Aiola, Simone

AU - Akrami, Yashar

AU - Basu, Kaustuv moni

AU - Boylan-Kolchin, Michael

AU - Bryan, Sean

AU - Casey, Caitlin M

AU - Clesse, Sébastien

AU - Cyr-Racine, Francis-Yan

AU - Mascolo, Luca Di

AU - Dicker, Simon

AU - Essinger-Hileman, Thomas

AU - Ferraro, Simone

AU - Fuller, George

AU - Galitzki, Nicholas

AU - Han, Dongwon

AU - Hasselfield, Matthew

AU - Holder, Gil

AU - Jain, Bhuvnesh

AU - Johnson, Bradley R.

AU - Johnson, Matthew

AU - Klaassen, Pamela

AU - MacInnis, Amanda

AU - Madhavacheril, Mathew

AU - Mauskopf, Philip

AU - Meerburg, Daan

AU - Meyers, Joel

AU - Mroczkowski, Tony

AU - Mukherjee, Suvodip

AU - Münchmeyer, Moritz

AU - Naess, Sigurd Kirkevold

AU - Nagai, Daisuke

AU - Namikawa, Toshiya

AU - Newburgh, Laura

AU - Nguyen, Nam

AU - Niemack, Michael

AU - Oppenheimer, Benjamin D.

AU - Pierpaoli, Elena

AU - Schaan, Emmanuel

AU - Sherwin, Blake

AU - Slosar, Anže

AU - Spergel, David

AU - Switzer, Eric

AU - Trivedi, Pranjal

AU - Tsai, Yu-Dai

AU - Engelen, Alexander van

AU - Wandelt, Benjamin

AU - Wollack, Edward

N1 - Response to request for information (RFI) by the Panel of Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Astro2020 Decadal Survey regarding the CMB-HD APC (arXiv:1906.10134). Note some text overlap with original APC. Note also detector count and cost have been reduced by 1/3, and observing time increased by 1/3 compared to original APC; science goals expanded

PY - 2020/2/28

Y1 - 2020/2/28

N2 - CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both fundamental physics of the Universe and astrophysics. This survey would be delivered in 7.5 years of observing 20,000 square degrees, using two new 30-meter-class off-axis cross-Dragone telescopes to be located at Cerro Toco in the Atacama Desert. Each telescope would field 800,000 detectors (200,000 pixels), for a total of 1.6 million detectors.

AB - CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both fundamental physics of the Universe and astrophysics. This survey would be delivered in 7.5 years of observing 20,000 square degrees, using two new 30-meter-class off-axis cross-Dragone telescopes to be located at Cerro Toco in the Atacama Desert. Each telescope would field 800,000 detectors (200,000 pixels), for a total of 1.6 million detectors.

KW - astro-ph.CO

KW - astro-ph.IM

KW - hep-ph

U2 - 10.48550/arXiv.2002.12714

DO - 10.48550/arXiv.2002.12714

M3 - Preprint

BT - Cmb-hd

ER -

Cmb-hd: Astro2020 RFI Response

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