Microwave spectro-polarimetry of matter and radiation across space and time

Jacques Delabrouille; Maximilian H. Abitbol; Nabila Aghanim; Yacine Ali-Haïmoud; David Alonso; Marcelo Alvarez; Anthony J. Banday; James G. Bartlett; Jochem Baselmans; Kaustuv Basu; Nicholas Battaglia; José Ramón Bermejo Climent; José L. Bernal; Matthieu Béthermin; Boris Bolliet; Matteo Bonato; François R. Bouchet; Patrick C. Breysse; Carlo Burigana; Zhen Yi Cai; Jens Chluba; Eugene Churazov; Helmut Dannerbauer; Paolo De Bernardis; Gianfranco De Zotti; Eleonora Di Valentino; Emanuela Dimastrogiovanni; Akira Endo; Jens Erler; Simone Ferraro; Fabio Finelli; Dale Fixsen; Shaul Hanany; Luke Hart; Carlos Hernández-Monteagudo; J. Colin Hill; Selim C. Hotinli; Kenichi Karatsu; Kirit Karkare; Garrett K. Keating; Ildar Khabibullin; Alan Kogut; Kazunori Kohri; Ely D. Kovetz; Guilaine Lagache; Julien Lesgourgues; Mathew Madhavacheril; Bruno Maffei; Nazzareno Mandolesi; Carlos Martins; Silvia Masi; John Mather; Jean Baptiste Melin; Azadeh Moradinezhad Dizgah; Tony Mroczkowski; Suvodip Mukherjee; Daisuke Nagai; Mattia Negrello; Nathalie Palanque-Delabrouille; Daniela Paoletti; Subodh P. Patil; Francesco Piacentini; Srinivasan Raghunathan; Andrea Ravenni; Mathieu Remazeilles; Vincent Revéret; Louis Rodriguez; Aditya Rotti; Jose Alberto Rubiño Martin; Jack Sayers; Douglas Scott; Joseph Silk; Marta Silva; Tarun Souradeep; Naonori Sugiyama; Rashid Sunyaev; Eric R. Switzer; Andrea Tartari; Tiziana Trombetti; Íñigo Zubeldia

doi:10.1007/s10686-021-09721-z

Microwave spectro-polarimetry of matter and radiation across space and time

Jacques Delabrouille, Maximilian H. Abitbol, Nabila Aghanim, Yacine Ali-Haïmoud, David Alonso, Marcelo Alvarez, Anthony J. Banday, James G. Bartlett, Jochem Baselmans, Kaustuv Basu, Nicholas Battaglia, José Ramón Bermejo Climent, José L. Bernal, Matthieu Béthermin, Boris Bolliet, Matteo Bonato, François R. Bouchet, Patrick C. Breysse, Carlo Burigana, Zhen Yi CaiJens Chluba, Eugene Churazov, Helmut Dannerbauer, Paolo De Bernardis, Gianfranco De Zotti, Eleonora Di Valentino, Emanuela Dimastrogiovanni, Akira Endo, Jens Erler, Simone Ferraro, Fabio Finelli, Dale Fixsen, Shaul Hanany, Luke Hart, Carlos Hernández-Monteagudo, J. Colin Hill, Selim C. Hotinli, Kenichi Karatsu, Kirit Karkare, Garrett K. Keating, Ildar Khabibullin, Alan Kogut, Kazunori Kohri, Ely D. Kovetz, Guilaine Lagache, Julien Lesgourgues, Mathew Madhavacheril, Bruno Maffei, Nazzareno Mandolesi, Carlos Martins, Silvia Masi, John Mather, Jean Baptiste Melin, Azadeh Moradinezhad Dizgah, Tony Mroczkowski, Suvodip Mukherjee, Daisuke Nagai, Mattia Negrello, Nathalie Palanque-Delabrouille, Daniela Paoletti, Subodh P. Patil, Francesco Piacentini, Srinivasan Raghunathan, Andrea Ravenni, Mathieu Remazeilles, Vincent Revéret, Louis Rodriguez, Aditya Rotti, Jose Alberto Rubiño Martin, Jack Sayers, Douglas Scott, Joseph Silk, Marta Silva, Tarun Souradeep, Naonori Sugiyama, Rashid Sunyaev, Eric R. Switzer, Andrea Tartari, Tiziana Trombetti, Íñigo Zubeldia

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

15 Scopus citations

Abstract

This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-dimensional distribution of hot gas, velocity flows, early metals, dust, and mass distribution in the entire Hubble volume, exploit CMB temperature and polarisation anisotropies down to fundamental limits, and track energy injection and absorption into the radiation background across cosmic times by measuring spectral distortions of the CMB blackbody emission. In addition to its exceptional capability for cosmology and fundamental physics, such a survey would provide an unprecedented view of microwave emissions at sub-arcminute to few-arcminute angular resolution in hundreds of frequency channels, a data set that would be of immense legacy value for many branches of astrophysics. We propose that this survey be carried out with a large space mission featuring a broad-band polarised imager and a moderate resolution spectro-imager at the focus of a 3.5 m aperture telescope actively cooled to about 8K, complemented with absolutely-calibrated Fourier Transform Spectrometer modules observing at degree-scale angular resolution in the 10–2000 GHz frequency range. We propose two observing modes: a survey mode to map the entire sky as well as a few selected wide fields, and an observatory mode for deeper observations of regions of specific interest.

Original language	English (US)
Pages (from-to)	1471-1514
Number of pages	44
Journal	Experimental Astronomy
Volume	51
Issue number	3
DOIs	https://doi.org/10.1007/s10686-021-09721-z
State	Published - Jun 2021

Bibliographical note

Publisher Copyright:
© 2021, The Author(s).

Keywords

Cosmology
Early Universe
Galaxies
Galaxy clusters

Access

10.1007/s10686-021-09721-z

OpenUrl availability

Full text

Cite this

Delabrouille, J., Abitbol, M. H., Aghanim, N., Ali-Haïmoud, Y., Alonso, D., Alvarez, M., Banday, A. J., Bartlett, J. G., Baselmans, J., Basu, K., Battaglia, N., Climent, J. R. B., Bernal, J. L., Béthermin, M., Bolliet, B., Bonato, M., Bouchet, F. R., Breysse, P. C., Burigana, C., ... Zubeldia, Í. (2021). Microwave spectro-polarimetry of matter and radiation across space and time. Experimental Astronomy, 51(3), 1471-1514. https://doi.org/10.1007/s10686-021-09721-z

Delabrouille, J, Abitbol, MH, Aghanim, N, Ali-Haïmoud, Y, Alonso, D, Alvarez, M, Banday, AJ, Bartlett, JG, Baselmans, J, Basu, K, Battaglia, N, Climent, JRB, Bernal, JL, Béthermin, M, Bolliet, B, Bonato, M, Bouchet, FR, Breysse, PC, Burigana, C, Cai, ZY, Chluba, J, Churazov, E, Dannerbauer, H, De Bernardis, P, De Zotti, G, Di Valentino, E, Dimastrogiovanni, E, Endo, A, Erler, J, Ferraro, S, Finelli, F, Fixsen, D, Hanany, S, Hart, L, Hernández-Monteagudo, C, Hill, JC, Hotinli, SC, Karatsu, K, Karkare, K, Keating, GK, Khabibullin, I, Kogut, A, Kohri, K, Kovetz, ED, Lagache, G, Lesgourgues, J, Madhavacheril, M, Maffei, B, Mandolesi, N, Martins, C, Masi, S, Mather, J, Melin, JB, Dizgah, AM, Mroczkowski, T, Mukherjee, S, Nagai, D, Negrello, M, Palanque-Delabrouille, N, Paoletti, D, Patil, SP, Piacentini, F, Raghunathan, S, Ravenni, A, Remazeilles, M, Revéret, V, Rodriguez, L, Rotti, A, Martin, JAR, Sayers, J, Scott, D, Silk, J, Silva, M, Souradeep, T, Sugiyama, N, Sunyaev, R, Switzer, ER, Tartari, A, Trombetti, T & Zubeldia, Í 2021, 'Microwave spectro-polarimetry of matter and radiation across space and time', Experimental Astronomy, vol. 51, no. 3, pp. 1471-1514. https://doi.org/10.1007/s10686-021-09721-z

@article{4eda8a69ea3f4975a9ff933aa4d924df,

title = "Microwave spectro-polarimetry of matter and radiation across space and time",

abstract = "This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-dimensional distribution of hot gas, velocity flows, early metals, dust, and mass distribution in the entire Hubble volume, exploit CMB temperature and polarisation anisotropies down to fundamental limits, and track energy injection and absorption into the radiation background across cosmic times by measuring spectral distortions of the CMB blackbody emission. In addition to its exceptional capability for cosmology and fundamental physics, such a survey would provide an unprecedented view of microwave emissions at sub-arcminute to few-arcminute angular resolution in hundreds of frequency channels, a data set that would be of immense legacy value for many branches of astrophysics. We propose that this survey be carried out with a large space mission featuring a broad-band polarised imager and a moderate resolution spectro-imager at the focus of a 3.5 m aperture telescope actively cooled to about 8K, complemented with absolutely-calibrated Fourier Transform Spectrometer modules observing at degree-scale angular resolution in the 10–2000 GHz frequency range. We propose two observing modes: a survey mode to map the entire sky as well as a few selected wide fields, and an observatory mode for deeper observations of regions of specific interest.",

keywords = "Cosmology, Early Universe, Galaxies, Galaxy clusters",

author = "Jacques Delabrouille and Abitbol, {Maximilian H.} and Nabila Aghanim and Yacine Ali-Ha{\"i}moud and David Alonso and Marcelo Alvarez and Banday, {Anthony J.} and Bartlett, {James G.} and Jochem Baselmans and Kaustuv Basu and Nicholas Battaglia and Climent, {Jos{\'e} Ram{\'o}n Bermejo} and Bernal, {Jos{\'e} L.} and Matthieu B{\'e}thermin and Boris Bolliet and Matteo Bonato and Bouchet, {Fran{\c c}ois R.} and Breysse, {Patrick C.} and Carlo Burigana and Cai, {Zhen Yi} and Jens Chluba and Eugene Churazov and Helmut Dannerbauer and {De Bernardis}, Paolo and {De Zotti}, Gianfranco and {Di Valentino}, Eleonora and Emanuela Dimastrogiovanni and Akira Endo and Jens Erler and Simone Ferraro and Fabio Finelli and Dale Fixsen and Shaul Hanany and Luke Hart and Carlos Hern{\'a}ndez-Monteagudo and Hill, {J. Colin} and Hotinli, {Selim C.} and Kenichi Karatsu and Kirit Karkare and Keating, {Garrett K.} and Ildar Khabibullin and Alan Kogut and Kazunori Kohri and Kovetz, {Ely D.} and Guilaine Lagache and Julien Lesgourgues and Mathew Madhavacheril and Bruno Maffei and Nazzareno Mandolesi and Carlos Martins and Silvia Masi and John Mather and Melin, {Jean Baptiste} and Dizgah, {Azadeh Moradinezhad} and Tony Mroczkowski and Suvodip Mukherjee and Daisuke Nagai and Mattia Negrello and Nathalie Palanque-Delabrouille and Daniela Paoletti and Patil, {Subodh P.} and Francesco Piacentini and Srinivasan Raghunathan and Andrea Ravenni and Mathieu Remazeilles and Vincent Rev{\'e}ret and Louis Rodriguez and Aditya Rotti and Martin, {Jose Alberto Rubi{\~n}o} and Jack Sayers and Douglas Scott and Joseph Silk and Marta Silva and Tarun Souradeep and Naonori Sugiyama and Rashid Sunyaev and Switzer, {Eric R.} and Andrea Tartari and Tiziana Trombetti and {\'I}{\~n}igo Zubeldia",

note = "Publisher Copyright: {\textcopyright} 2021, The Author(s).",

year = "2021",

month = jun,

doi = "10.1007/s10686-021-09721-z",

language = "English (US)",

volume = "51",

pages = "1471--1514",

journal = "Experimental Astronomy",

issn = "0922-6435",

publisher = "Springer Netherlands",

number = "3",

}

TY - JOUR

T1 - Microwave spectro-polarimetry of matter and radiation across space and time

AU - Delabrouille, Jacques

AU - Abitbol, Maximilian H.

AU - Aghanim, Nabila

AU - Ali-Haïmoud, Yacine

AU - Alonso, David

AU - Alvarez, Marcelo

AU - Banday, Anthony J.

AU - Bartlett, James G.

AU - Baselmans, Jochem

AU - Basu, Kaustuv

AU - Battaglia, Nicholas

AU - Climent, José Ramón Bermejo

AU - Bernal, José L.

AU - Béthermin, Matthieu

AU - Bolliet, Boris

AU - Bonato, Matteo

AU - Bouchet, François R.

AU - Breysse, Patrick C.

AU - Burigana, Carlo

AU - Cai, Zhen Yi

AU - Chluba, Jens

AU - Churazov, Eugene

AU - Dannerbauer, Helmut

AU - De Bernardis, Paolo

AU - De Zotti, Gianfranco

AU - Di Valentino, Eleonora

AU - Dimastrogiovanni, Emanuela

AU - Endo, Akira

AU - Erler, Jens

AU - Ferraro, Simone

AU - Finelli, Fabio

AU - Fixsen, Dale

AU - Hanany, Shaul

AU - Hart, Luke

AU - Hernández-Monteagudo, Carlos

AU - Hill, J. Colin

AU - Hotinli, Selim C.

AU - Karatsu, Kenichi

AU - Karkare, Kirit

AU - Keating, Garrett K.

AU - Khabibullin, Ildar

AU - Kogut, Alan

AU - Kohri, Kazunori

AU - Kovetz, Ely D.

AU - Lagache, Guilaine

AU - Lesgourgues, Julien

AU - Madhavacheril, Mathew

AU - Maffei, Bruno

AU - Mandolesi, Nazzareno

AU - Martins, Carlos

AU - Masi, Silvia

AU - Mather, John

AU - Melin, Jean Baptiste

AU - Dizgah, Azadeh Moradinezhad

AU - Mroczkowski, Tony

AU - Mukherjee, Suvodip

AU - Nagai, Daisuke

AU - Negrello, Mattia

AU - Palanque-Delabrouille, Nathalie

AU - Paoletti, Daniela

AU - Patil, Subodh P.

AU - Piacentini, Francesco

AU - Raghunathan, Srinivasan

AU - Ravenni, Andrea

AU - Remazeilles, Mathieu

AU - Revéret, Vincent

AU - Rodriguez, Louis

AU - Rotti, Aditya

AU - Martin, Jose Alberto Rubiño

AU - Sayers, Jack

AU - Scott, Douglas

AU - Silk, Joseph

AU - Silva, Marta

AU - Souradeep, Tarun

AU - Sugiyama, Naonori

AU - Sunyaev, Rashid

AU - Switzer, Eric R.

AU - Tartari, Andrea

AU - Trombetti, Tiziana

AU - Zubeldia, Íñigo

PY - 2021/6

Y1 - 2021/6

N2 - This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-dimensional distribution of hot gas, velocity flows, early metals, dust, and mass distribution in the entire Hubble volume, exploit CMB temperature and polarisation anisotropies down to fundamental limits, and track energy injection and absorption into the radiation background across cosmic times by measuring spectral distortions of the CMB blackbody emission. In addition to its exceptional capability for cosmology and fundamental physics, such a survey would provide an unprecedented view of microwave emissions at sub-arcminute to few-arcminute angular resolution in hundreds of frequency channels, a data set that would be of immense legacy value for many branches of astrophysics. We propose that this survey be carried out with a large space mission featuring a broad-band polarised imager and a moderate resolution spectro-imager at the focus of a 3.5 m aperture telescope actively cooled to about 8K, complemented with absolutely-calibrated Fourier Transform Spectrometer modules observing at degree-scale angular resolution in the 10–2000 GHz frequency range. We propose two observing modes: a survey mode to map the entire sky as well as a few selected wide fields, and an observatory mode for deeper observations of regions of specific interest.

AB - This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-dimensional distribution of hot gas, velocity flows, early metals, dust, and mass distribution in the entire Hubble volume, exploit CMB temperature and polarisation anisotropies down to fundamental limits, and track energy injection and absorption into the radiation background across cosmic times by measuring spectral distortions of the CMB blackbody emission. In addition to its exceptional capability for cosmology and fundamental physics, such a survey would provide an unprecedented view of microwave emissions at sub-arcminute to few-arcminute angular resolution in hundreds of frequency channels, a data set that would be of immense legacy value for many branches of astrophysics. We propose that this survey be carried out with a large space mission featuring a broad-band polarised imager and a moderate resolution spectro-imager at the focus of a 3.5 m aperture telescope actively cooled to about 8K, complemented with absolutely-calibrated Fourier Transform Spectrometer modules observing at degree-scale angular resolution in the 10–2000 GHz frequency range. We propose two observing modes: a survey mode to map the entire sky as well as a few selected wide fields, and an observatory mode for deeper observations of regions of specific interest.

KW - Cosmology

KW - Early Universe

KW - Galaxies

KW - Galaxy clusters

UR - http://www.scopus.com/inward/record.url?scp=85109346936&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85109346936&partnerID=8YFLogxK

U2 - 10.1007/s10686-021-09721-z

DO - 10.1007/s10686-021-09721-z

M3 - Article

AN - SCOPUS:85109346936

SN - 0922-6435

VL - 51

SP - 1471

EP - 1514

JO - Experimental Astronomy

JF - Experimental Astronomy

IS - 3

ER -

Microwave spectro-polarimetry of matter and radiation across space and time

Abstract

Bibliographical note

Keywords

Access

OpenUrl availability

Other files and links

Fingerprint

Cite this