Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI Response

Emanuele Castorina; Simon Foreman; Dionysios Karagiannis; Adrian Liu; Kiyoshi W. Masui; Pieter D. Meerburg; Laura B. Newburgh; Paul O'Connor; Andrej Obuljen; Hamsa Padmanabhan; J. Richard Shaw; Anže Slosar; Paul Stankus; Peter T. Timbie; Benjamin Wallisch; Martin White

doi:10.48550/arXiv.2002.05072

Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI Response

Emanuele Castorina, Simon Foreman, Dionysios Karagiannis, Adrian Liu, Kiyoshi W. Masui, Pieter D. Meerburg, Laura B. Newburgh, Paul O'Connor, Andrej Obuljen, Hamsa Padmanabhan, J. Richard Shaw, Anže Slosar, Paul Stankus, Peter T. Timbie, Benjamin Wallisch, Martin White

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The Packed Ultra-wideband Mapping Array (PUMA) is a proposed low-resolution transit interferometric radio telescope operating over the frequency range 200 - 1100MHz. Its rich science portfolio will include measuring structure in the universe from redshift z = 0.3 to 6 using 21cm intensity mapping, detecting one million fast radio bursts, and monitoring thousands of pulsars. It will allow PUMA to advance science in three different areas of physics (the physics of dark energy, the physics of cosmic inflation and time-domain astrophysics). This document is a response to a request for information (RFI) by the Panel on Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Decadal Survey on Astronomy and Astrophysics 2020. We present the science case of PUMA, the development path and major risks to the project.

Originele taal-2	English
DOI's	https://doi.org/10.48550/arXiv.2002.05072
Status	Submitted - 12-feb.-2020

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@techreport{1307f852b7c14d0ebb2066ba3bc50b97,

title = "Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI Response",

abstract = " The Packed Ultra-wideband Mapping Array (PUMA) is a proposed low-resolution transit interferometric radio telescope operating over the frequency range 200 - 1100MHz. Its rich science portfolio will include measuring structure in the universe from redshift z = 0.3 to 6 using 21cm intensity mapping, detecting one million fast radio bursts, and monitoring thousands of pulsars. It will allow PUMA to advance science in three different areas of physics (the physics of dark energy, the physics of cosmic inflation and time-domain astrophysics). This document is a response to a request for information (RFI) by the Panel on Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Decadal Survey on Astronomy and Astrophysics 2020. We present the science case of PUMA, the development path and major risks to the project. ",

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

author = "Emanuele Castorina and Simon Foreman and Dionysios Karagiannis and Adrian Liu and Masui, {Kiyoshi W.} and Meerburg, {Pieter D.} and Newburgh, {Laura B.} and Paul O'Connor and Andrej Obuljen and Hamsa Padmanabhan and Shaw, {J. Richard} and An{\v z}e Slosar and Paul Stankus and Timbie, {Peter T.} and Benjamin Wallisch and Martin White",

note = "46 pages, 16 figures, 7 tables; response to the request for information (RFI) by the Panel on Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Astro2020 Decadal Survey regarding PUMA APC submission (arXiv:1907.12559); v2: updated with correct bbl file",

year = "2020",

month = feb,

day = "12",

doi = "10.48550/arXiv.2002.05072",

language = "English",

type = "WorkingPaper",

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T1 - Packed Ultra-wideband Mapping Array (PUMA)

T2 - Astro2020 RFI Response

AU - Castorina, Emanuele

AU - Foreman, Simon

AU - Karagiannis, Dionysios

AU - Liu, Adrian

AU - Masui, Kiyoshi W.

AU - Meerburg, Pieter D.

AU - Newburgh, Laura B.

AU - O'Connor, Paul

AU - Obuljen, Andrej

AU - Padmanabhan, Hamsa

AU - Shaw, J. Richard

AU - Slosar, Anže

AU - Stankus, Paul

AU - Timbie, Peter T.

AU - Wallisch, Benjamin

AU - White, Martin

N1 - 46 pages, 16 figures, 7 tables; response to the request for information (RFI) by the Panel on Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Astro2020 Decadal Survey regarding PUMA APC submission (arXiv:1907.12559); v2: updated with correct bbl file

PY - 2020/2/12

Y1 - 2020/2/12

N2 - The Packed Ultra-wideband Mapping Array (PUMA) is a proposed low-resolution transit interferometric radio telescope operating over the frequency range 200 - 1100MHz. Its rich science portfolio will include measuring structure in the universe from redshift z = 0.3 to 6 using 21cm intensity mapping, detecting one million fast radio bursts, and monitoring thousands of pulsars. It will allow PUMA to advance science in three different areas of physics (the physics of dark energy, the physics of cosmic inflation and time-domain astrophysics). This document is a response to a request for information (RFI) by the Panel on Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Decadal Survey on Astronomy and Astrophysics 2020. We present the science case of PUMA, the development path and major risks to the project.

AB - The Packed Ultra-wideband Mapping Array (PUMA) is a proposed low-resolution transit interferometric radio telescope operating over the frequency range 200 - 1100MHz. Its rich science portfolio will include measuring structure in the universe from redshift z = 0.3 to 6 using 21cm intensity mapping, detecting one million fast radio bursts, and monitoring thousands of pulsars. It will allow PUMA to advance science in three different areas of physics (the physics of dark energy, the physics of cosmic inflation and time-domain astrophysics). This document is a response to a request for information (RFI) by the Panel on Radio, Millimeter, and Submillimeter Observations from the Ground (RMS) of the Decadal Survey on Astronomy and Astrophysics 2020. We present the science case of PUMA, the development path and major risks to the project.

KW - astro-ph.IM

KW - astro-ph.CO

KW - astro-ph.HE

U2 - 10.48550/arXiv.2002.05072

DO - 10.48550/arXiv.2002.05072

M3 - Preprint

BT - Packed Ultra-wideband Mapping Array (PUMA)

ER -

Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI Response

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