COrE (Cosmic Origins Explorer) A White Paper

COrE Collaboration The; C Armitage-Caplan; M Avillez; D Barbosa; A Banday; N Bartolo; R Battye; J P Bernard; P de Bernardis; S Basak; M Bersanelli; P Bielewicz; A Bonaldi; M Bucher; F Bouchet; F Boulanger; C Burigana; P Camus; A Challinor; S Chongchitnan; D Clements; S Colafrancesco; J Delabrouille; M De Petris; G De Zotti; C Dickinson; J Dunkley; T Ensslin; J Fergusson; P Ferreira; K Ferriere; F Finelli; S Galli; J Garcia-Bellido; C Gauthier; M Haverkorn; M Hindmarsh; A Jaffe; M Kunz; J Lesgourgues; A Liddle; M Liguori; M Lopez-Caniego; B Maffei; P Marchegiani; E Martinez-Gonzalez; S Masi; P Mauskopf; S Matarrese; A Melchiorri; P Mukherjee; F Nati; P Natoli; M Negrello; L Pagano; D Paoletti; T Peacocke; H Peiris; L Perroto; F Piacentini; M Piat; L Piccirillo; G Pisano; N Ponthieu; C Rath; S Ricciardi; J Rubino Martin; M Salatino; P Shellard; R Stompor; L Toffolatti J Urrestilla; B Van Tent; L Verde; B Wandelt; S Withington

COrE (Cosmic Origins Explorer) A White Paper

COrE Collaboration The, C Armitage-Caplan, M Avillez, D Barbosa, A Banday, N Bartolo, R Battye, J P Bernard, P de Bernardis, S Basak, M Bersanelli, P Bielewicz, A Bonaldi, M Bucher, F Bouchet, F Boulanger, C Burigana, P Camus, A Challinor, S ChongchitnanD Clements, S Colafrancesco, J Delabrouille, M De Petris, G De Zotti, C Dickinson, J Dunkley, T Ensslin, J Fergusson, P Ferreira, K Ferriere, F Finelli, S Galli, J Garcia-Bellido, C Gauthier, M Haverkorn, M Hindmarsh, A Jaffe, M Kunz, J Lesgourgues, A Liddle, M Liguori, M Lopez-Caniego, B Maffei, P Marchegiani, E Martinez-Gonzalez, S Masi, P Mauskopf, S Matarrese, A Melchiorri, P Mukherjee, F Nati, P Natoli, M Negrello, L Pagano, D Paoletti, T Peacocke, H Peiris, L Perroto, F Piacentini, M Piat, L Piccirillo, G Pisano, N Ponthieu, C Rath, S Ricciardi, J Rubino Martin, M Salatino, P Shellard, R Stompor, L Toffolatti J Urrestilla, B Van Tent, L Verde, B Wandelt, S Withington

Research output: Book/Report › Book › peer-review

Abstract

COrE (Cosmic Origins Explorer) is a fourth-generation full-sky, microwave-band satellite recently proposed to ESA within Cosmic Vision 2015-2025. COrE will provide maps of the microwave sky in polarization and temperature in 15 frequency bands, ranging from 45 GHz to 795 GHz, with an angular resolution ranging from 23 arcmin (45 GHz) and 1.3 arcmin (795 GHz) and sensitivities roughly 10 to 30 times better than PLANCK (depending on the frequency channel). The COrE mission will lead to breakthrough science in a wide range of areas, ranging from primordial cosmology to galactic and extragalactic science. COrE is designed to detect the primordial gravitational waves generated during the epoch of cosmic inflation at more than $3\sigma $ for $r=(T/S)>=10^{-3}$. It will also measure the CMB gravitational lensing deflection power spectrum to the cosmic variance limit on all linear scales, allowing us to probe absolute neutrino masses better than laboratory experiments and down to plausible values suggested by the neutrino oscillation data. COrE will also search for primordial non-Gaussianity with significant improvements over Planck in its ability to constrain the shape (and amplitude) of non-Gaussianity. In the areas of galactic and extragalactic science, in its highest frequency channels COrE will provide maps of the galactic polarized dust emission allowing us to map the galactic magnetic field in areas of diffuse emission not otherwise accessible to probe the initial conditions for star formation. COrE will also map the galactic synchrotron emission thirty times better than PLANCK. This White Paper reviews the COrE science program, our simulations on foreground subtraction, and the proposed instrumental configuration.

Original language	English
Publisher	No publisher name
Volume	1102
Publication status	Published - 2011

Publication series

Name	ArXiv e-prints

Keywords

Astrophysics - Cosmology and Extragalactic Astrophysics

Access to Document

http://adsabs.harvard.edu/abs/2011arXiv1102.2181T

Cite this

The, CO. C., Armitage-Caplan, C., Avillez, M., Barbosa, D., Banday, A., Bartolo, N., Battye, R., Bernard, J. P., de Bernardis, P., Basak, S., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bucher, M., Bouchet, F., Boulanger, F., Burigana, C., Camus, P., Challinor, A., ... Withington, S. (2011). COrE (Cosmic Origins Explorer) A White Paper. (ArXiv e-prints). No publisher name. http://adsabs.harvard.edu/abs/2011arXiv1102.2181T

@book{fbfe0672c72b4a368e37bd320bc74fe4,

title = "COrE (Cosmic Origins Explorer) A White Paper",

abstract = "COrE (Cosmic Origins Explorer) is a fourth-generation full-sky, microwave-band satellite recently proposed to ESA within Cosmic Vision 2015-2025. COrE will provide maps of the microwave sky in polarization and temperature in 15 frequency bands, ranging from 45 GHz to 795 GHz, with an angular resolution ranging from 23 arcmin (45 GHz) and 1.3 arcmin (795 GHz) and sensitivities roughly 10 to 30 times better than PLANCK (depending on the frequency channel). The COrE mission will lead to breakthrough science in a wide range of areas, ranging from primordial cosmology to galactic and extragalactic science. COrE is designed to detect the primordial gravitational waves generated during the epoch of cosmic inflation at more than $3\sigma $ for $r=(T/S)>=10^{-3}$. It will also measure the CMB gravitational lensing deflection power spectrum to the cosmic variance limit on all linear scales, allowing us to probe absolute neutrino masses better than laboratory experiments and down to plausible values suggested by the neutrino oscillation data. COrE will also search for primordial non-Gaussianity with significant improvements over Planck in its ability to constrain the shape (and amplitude) of non-Gaussianity. In the areas of galactic and extragalactic science, in its highest frequency channels COrE will provide maps of the galactic polarized dust emission allowing us to map the galactic magnetic field in areas of diffuse emission not otherwise accessible to probe the initial conditions for star formation. COrE will also map the galactic synchrotron emission thirty times better than PLANCK. This White Paper reviews the COrE science program, our simulations on foreground subtraction, and the proposed instrumental configuration.",

keywords = "Astrophysics - Cosmology and Extragalactic Astrophysics",

author = "The, {COrE Collaboration} and C Armitage-Caplan and M Avillez and D Barbosa and A Banday and N Bartolo and R Battye and Bernard, {J P} and {de Bernardis}, P and S Basak and M Bersanelli and P Bielewicz and A Bonaldi and M Bucher and F Bouchet and F Boulanger and C Burigana and P Camus and A Challinor and S Chongchitnan and D Clements and S Colafrancesco and J Delabrouille and {De Petris}, M and {De Zotti}, G and C Dickinson and J Dunkley and T Ensslin and J Fergusson and P Ferreira and K Ferriere and F Finelli and S Galli and J Garcia-Bellido and C Gauthier and M Haverkorn and M Hindmarsh and A Jaffe and M Kunz and J Lesgourgues and A Liddle and M Liguori and M Lopez-Caniego and B Maffei and P Marchegiani and E Martinez-Gonzalez and S Masi and P Mauskopf and S Matarrese and A Melchiorri and P Mukherjee and F Nati and P Natoli and M Negrello and L Pagano and D Paoletti and T Peacocke and H Peiris and L Perroto and F Piacentini and M Piat and L Piccirillo and G Pisano and N Ponthieu and C Rath and S Ricciardi and {Rubino Martin}, J and M Salatino and P Shellard and R Stompor and Urrestilla, {L Toffolatti J} and {Van Tent}, B and L Verde and B Wandelt and S Withington",

note = "February 1, 2011 90 pages Latex 15 figures (revised 28 April 2011, references added, minor errors corrected)",

year = "2011",

language = "English",

volume = "1102",

series = "ArXiv e-prints",

publisher = "No publisher name",

}

The, COC, Armitage-Caplan, C, Avillez, M, Barbosa, D, Banday, A, Bartolo, N, Battye, R, Bernard, JP, de Bernardis, P, Basak, S, Bersanelli, M, Bielewicz, P, Bonaldi, A, Bucher, M, Bouchet, F, Boulanger, F, Burigana, C, Camus, P, Challinor, A, Chongchitnan, S, Clements, D, Colafrancesco, S, Delabrouille, J, De Petris, M, De Zotti, G, Dickinson, C, Dunkley, J, Ensslin, T, Fergusson, J, Ferreira, P, Ferriere, K, Finelli, F, Galli, S, Garcia-Bellido, J, Gauthier, C, Haverkorn, M, Hindmarsh, M, Jaffe, A, Kunz, M, Lesgourgues, J, Liddle, A, Liguori, M, Lopez-Caniego, M, Maffei, B, Marchegiani, P, Martinez-Gonzalez, E, Masi, S, Mauskopf, P, Matarrese, S, Melchiorri, A, Mukherjee, P, Nati, F, Natoli, P, Negrello, M, Pagano, L, Paoletti, D, Peacocke, T, Peiris, H, Perroto, L, Piacentini, F, Piat, M, Piccirillo, L, Pisano, G, Ponthieu, N, Rath, C, Ricciardi, S, Rubino Martin, J, Salatino, M, Shellard, P, Stompor, R, Urrestilla, LTJ, Van Tent, B, Verde, L, Wandelt, B & Withington, S 2011, COrE (Cosmic Origins Explorer) A White Paper. ArXiv e-prints, vol. 1102, No publisher name. <http://adsabs.harvard.edu/abs/2011arXiv1102.2181T>

TY - BOOK

T1 - COrE (Cosmic Origins Explorer) A White Paper

AU - The, COrE Collaboration

AU - Armitage-Caplan, C

AU - Avillez, M

AU - Barbosa, D

AU - Banday, A

AU - Bartolo, N

AU - Battye, R

AU - Bernard, J P

AU - de Bernardis, P

AU - Basak, S

AU - Bersanelli, M

AU - Bielewicz, P

AU - Bonaldi, A

AU - Bucher, M

AU - Bouchet, F

AU - Boulanger, F

AU - Burigana, C

AU - Camus, P

AU - Challinor, A

AU - Chongchitnan, S

AU - Clements, D

AU - Colafrancesco, S

AU - Delabrouille, J

AU - De Petris, M

AU - De Zotti, G

AU - Dickinson, C

AU - Dunkley, J

AU - Ensslin, T

AU - Fergusson, J

AU - Ferreira, P

AU - Ferriere, K

AU - Finelli, F

AU - Galli, S

AU - Garcia-Bellido, J

AU - Gauthier, C

AU - Haverkorn, M

AU - Hindmarsh, M

AU - Jaffe, A

AU - Kunz, M

AU - Lesgourgues, J

AU - Liddle, A

AU - Liguori, M

AU - Lopez-Caniego, M

AU - Maffei, B

AU - Marchegiani, P

AU - Martinez-Gonzalez, E

AU - Masi, S

AU - Mauskopf, P

AU - Matarrese, S

AU - Melchiorri, A

AU - Mukherjee, P

AU - Nati, F

AU - Natoli, P

AU - Negrello, M

AU - Pagano, L

AU - Paoletti, D

AU - Peacocke, T

AU - Peiris, H

AU - Perroto, L

AU - Piacentini, F

AU - Piat, M

AU - Piccirillo, L

AU - Pisano, G

AU - Ponthieu, N

AU - Rath, C

AU - Ricciardi, S

AU - Rubino Martin, J

AU - Salatino, M

AU - Shellard, P

AU - Stompor, R

AU - Urrestilla, L Toffolatti J

AU - Van Tent, B

AU - Verde, L

AU - Wandelt, B

AU - Withington, S

N1 - February 1, 2011 90 pages Latex 15 figures (revised 28 April 2011, references added, minor errors corrected)

PY - 2011

Y1 - 2011

N2 - COrE (Cosmic Origins Explorer) is a fourth-generation full-sky, microwave-band satellite recently proposed to ESA within Cosmic Vision 2015-2025. COrE will provide maps of the microwave sky in polarization and temperature in 15 frequency bands, ranging from 45 GHz to 795 GHz, with an angular resolution ranging from 23 arcmin (45 GHz) and 1.3 arcmin (795 GHz) and sensitivities roughly 10 to 30 times better than PLANCK (depending on the frequency channel). The COrE mission will lead to breakthrough science in a wide range of areas, ranging from primordial cosmology to galactic and extragalactic science. COrE is designed to detect the primordial gravitational waves generated during the epoch of cosmic inflation at more than $3\sigma $ for $r=(T/S)>=10^{-3}$. It will also measure the CMB gravitational lensing deflection power spectrum to the cosmic variance limit on all linear scales, allowing us to probe absolute neutrino masses better than laboratory experiments and down to plausible values suggested by the neutrino oscillation data. COrE will also search for primordial non-Gaussianity with significant improvements over Planck in its ability to constrain the shape (and amplitude) of non-Gaussianity. In the areas of galactic and extragalactic science, in its highest frequency channels COrE will provide maps of the galactic polarized dust emission allowing us to map the galactic magnetic field in areas of diffuse emission not otherwise accessible to probe the initial conditions for star formation. COrE will also map the galactic synchrotron emission thirty times better than PLANCK. This White Paper reviews the COrE science program, our simulations on foreground subtraction, and the proposed instrumental configuration.

AB - COrE (Cosmic Origins Explorer) is a fourth-generation full-sky, microwave-band satellite recently proposed to ESA within Cosmic Vision 2015-2025. COrE will provide maps of the microwave sky in polarization and temperature in 15 frequency bands, ranging from 45 GHz to 795 GHz, with an angular resolution ranging from 23 arcmin (45 GHz) and 1.3 arcmin (795 GHz) and sensitivities roughly 10 to 30 times better than PLANCK (depending on the frequency channel). The COrE mission will lead to breakthrough science in a wide range of areas, ranging from primordial cosmology to galactic and extragalactic science. COrE is designed to detect the primordial gravitational waves generated during the epoch of cosmic inflation at more than $3\sigma $ for $r=(T/S)>=10^{-3}$. It will also measure the CMB gravitational lensing deflection power spectrum to the cosmic variance limit on all linear scales, allowing us to probe absolute neutrino masses better than laboratory experiments and down to plausible values suggested by the neutrino oscillation data. COrE will also search for primordial non-Gaussianity with significant improvements over Planck in its ability to constrain the shape (and amplitude) of non-Gaussianity. In the areas of galactic and extragalactic science, in its highest frequency channels COrE will provide maps of the galactic polarized dust emission allowing us to map the galactic magnetic field in areas of diffuse emission not otherwise accessible to probe the initial conditions for star formation. COrE will also map the galactic synchrotron emission thirty times better than PLANCK. This White Paper reviews the COrE science program, our simulations on foreground subtraction, and the proposed instrumental configuration.

KW - Astrophysics - Cosmology and Extragalactic Astrophysics

M3 - Book

VL - 1102

T3 - ArXiv e-prints

BT - COrE (Cosmic Origins Explorer) A White Paper

PB - No publisher name

ER -

COrE (Cosmic Origins Explorer) A White Paper

Abstract

Publication series

Keywords

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