Imperial College London

Professor Andrew H Jaffe

Faculty of Natural SciencesDepartment of Physics

Professor of Astrophysics and Cosmology
 
 
 
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Contact

 

+44 (0)20 7594 7526a.jaffe Website

 
 
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Assistant

 

Miss Louise Hayward +44 (0)20 7594 7679

 
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Location

 

1018BBlackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Publication Type
Year
to

368 results found

Ade PAR, Aghanim N, Alves MIR, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Bedini L, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Boulanger F, Burigana C, Butler RC, Cabella P, Cardoso J-F, Chen X, Chiang L-Y, Christensen PR, Clements DL, Colombi S, Colombo LPL, Coulais A, Cuttaia F, Davies RD, Davis RJ, de Bernardis P, de Gasperis G, de Zotti G, Delabrouille J, Dickinson C, Diego JM, Dobler G, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Ensslin TA, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Genova-Santos RT, Ghosh T, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Hernandez-Monteagudo C, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe TR, Jaffe AH, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Knoche J, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Leach S, Leonardi R, Lilje PB, Linden-Vornle M, Lubin PM, Macias-Perez JF, Maffei B, Maino D, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Mazzotta P, Melchiorri A, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Oxborrow CA, Pajot F, Paladini R, Paoletti D, Peel M, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Popa L, Poutanen T, Pratt GW, Prunet S, Puget J-L, Rachen JP, Reach WT, Rebolo R, Reinecke M, Renault C, Ricciardi S, Ristorcelli I, Rocha G, Rosset C, Rubino-Martin JA, Rusholme B, Salerno E, Sandri M, Savini G, Scott D, Spencer L, Stolyarov V, Sudiwala R, Suur-Uski A-S, Sygnet J-F, Tauber JA, Terenzi L, Tibbs CT, Toffolatti L, Tomasi M Tet al., 2013, <i>Planck</i> intermediate results. XII: Diffuse Galactic components in the Gould Belt system, ASTRONOMY & ASTROPHYSICS, Vol: 557, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Barrena R, Bartlett JG, Battaner E, Benabed K, Bernard J-P, Bersanelli M, Bikmaev I, Bock JJ, Boehringer H, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Bourdin H, Burenin R, Burigana C, Butler RC, Cabella P, Chamballu A, Chary R-R, Chiang L-Y, Chon G, Christensen PR, Clements DL, Colafrancesco S, Colombi S, Colombo LPL, Comis B, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Davis RJ, de Bernardis P, de Gasperis G, de Rosa A, de Zotti G, Delabrouille J, Democles J, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Finelli F, Flores-Cacho I, Forni O, Frailis M, Franceschi E, Frommert M, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Hurier G, Jaffe TR, Jaffe AH, Jones WC, Juvela M, Keihanen E, Keskitalo R, Khamitov I, Kisner TS, Kneissl R, Knoche J, Kunz M, Kurki-Suonio H, Laheenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Le Jeune M, Leonardi R, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Luzzi G, Macias-Perez JF, MacTavish CJ, Maffei B, Maino D, Mandolesi N, Maris M, Marleau F, Marshall DJ, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Mazzotta P, Mei S, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Oxborrow CA, Pajot F, Paoletti D, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Pointecouteau E, Polenta G, Popa L, Poutanen T, Pratt GW, Prunet S, Puget J-L, Rachen JP, Rebolo R, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Ristorcelli I, Rocha Get al., 2013, <i>Planck</i> intermediate results XI. The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies, ASTRONOMY & ASTROPHYSICS, Vol: 557, ISSN: 0004-6361

Journal article

Paykari P, Jaffe AH, 2013, Sparsely sampling the sky: a Bayesian experimental design approach, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 433, Pages: 3523-3533, ISSN: 0035-8711

Journal article

Heavens A, Alsing J, Jaffe AH, 2013, Combining size and shape in weak lensing, Monthly Notices of the Royal Astronomical Society: Letters, Vol: 433, Pages: L6-L10, ISSN: 1745-3933

Weak lensing alters the size of images with a similar magnitude to the distortion due to shear. Galaxy size probes the convergence field and shapes the shear field, both of which contain cosmological information. We show the gains expected in the dark energy figure of merit if galaxy size information is used in combination with galaxy shape. In any normal analysis of cosmic shear, galaxy sizes are also studied, so this is extra statistical information that comes for free and is currently unused. There are two main results in this Letter: first, we show that size measurement can be made uncorrelated with ellipticity measurement, thus allowing the full statistical gain from the combination, provided that √area is used as a size indicator; secondly, as a proof of concept, we show that when the relevant modes are noise dominated, as is the norm for lensing surveys, the gains are substantial, with improvements of about 68 per cent in the figure of merit expected when systematic errors are ignored. An approximate treatment of such systematics such as intrinsic alignments and size–magnitude correlations, respectively, suggests that a much better improvement in the dark energy figure of merit of even a factor of ∼4 may be achieved.

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bikmaev I, Boehringer H, Bonaldi A, Bond JR, Borgani S, Borrill J, Bouchet FR, Brown ML, Burigana C, Butler RC, Cabella P, Carvalho P, Catalano A, Cayon L, Chamballu A, Chary R-R, Chiang L-Y, Chon G, Christensen PR, Clements DL, Colafrancesco S, Colombi S, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Davis RJ, de Bernardis P, de Gasperis G, de Zotti G, Delabrouille J, Democles J, Desert F-X, Diego JM, Dolag K, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Ensslin TA, Eriksen HK, Finelli F, Flores-Cacho I, Forni O, Frailis M, Franceschi E, Frommert M, Galeotta S, Ganga K, Genova-Santos RT, Giraud-Heraud Y, Gonzalez-Nuevo J, Gonzalez-Riestra R, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Hempel A, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Hurier G, Jaffe AH, Jagemann T, Jones WC, Juvela M, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lamarre J-M, Lasenby A, Lawrence CR, Le Jeune M, Leach S, Leonardi R, Liddle A, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Luzzi G, Macias-Perez JF, Maino D, Mandolesi N, Mann R, Maris M, Marleau F, Marshall DJ, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Mazzotta P, Mei S, Meinhold PR, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Morgante G, Mortlock D, Munshi D, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Osborne S, Pajot F, Paoletti D, Perdereau O, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Platania P, Pointecouteau E, Polenta G, Popa L, Poutanen T, Pratt GW, Prunet S, Puget J-L, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Rocha G, Rosset C, Rossetti M, Rubino-Martin JA, Rusholme B, Sandri M, Savini G, Scott D, Smooet al., 2013, <i>Planck</i> intermediate results IV. The <i>XMM</i>-<i>Newton</i> validation programme for new <i>Planck</i> galaxy clusters, ASTRONOMY & ASTROPHYSICS, Vol: 550, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bikmaev I, Boehringer H, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Bourdin H, Burenin R, Burigana C, Cabella P, Cardoso J-F, Castex G, Catalano A, Cayon L, Chamballu A, Chiang L-Y, Chon G, Christensen PR, Clements DL, Colafrancesco S, Colombi S, Colombo LPL, Comis B, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Danese L, Davis RJ, de Bernardis P, de Gasperis G, de Zotti G, Delabrouille J, Democles J, Diego JM, Dolag K, Dole H, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Flores-Cacho I, Forni O, Frailis M, Franceschi E, Frommert M, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Gilfanov M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Heinamaki P, Hempel A, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hurier G, Jaffe TR, Jaffe AH, Jagemann T, Jones WC, Juvela M, Keihaenen E, Khamitov I, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Le Jeune M, Leonardi R, Lilje PB, Lopez-Caniego M, Luzzi G, Macias-Perez JF, Maino D, Mandolesi N, Maris M, Marleau F, Marshall DJ, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Mazzotta P, Mei S, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pajot F, Paoletti D, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanen T, Pratt GW, Prunet S, Puget J-L, Rachen JP, Rebolo R, Reinecet al., 2013, <i>Planck</i> intermediate results VI. The dynamical structure of PLCKG214.6+37.0, a <i>Planck</i> discovered triple system of galaxy clusters, ASTRONOMY & ASTROPHYSICS, Vol: 550, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Argueeso F, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bethermin M, Bhatia R, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Burigana C, Cabella P, Cardoso J-F, Catalano A, Cayon L, Chamballu A, Chary R-R, Chen X, Chiang L-Y, Christensen PR, Clements DL, Colafrancesco S, Colombi S, Colombo LPL, Coulais A, Crill BP, Cuttaia F, Danese L, Davis RJ, de Bernardis P, de Gasperis G, de Zotti G, Delabrouille J, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Fosalba P, Frailis M, Franceschi E, Galeotta S, Ganga K, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Jaffe TR, Jaffe AH, Jagemann T, Jones WC, Juvela M, Keihanen E, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurinsky N, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Leonardi R, Lilje PB, Lopez-Caniego M, Macias-Perez JF, Maino D, Mandolesi N, Maris M, Marshall DJ, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Mazzotta P, Melchiorri A, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pajot F, Paladini R, Paoletti D, Partridge B, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanen T, Pratt GW, Prunet S, Puget J-L, Rachen JP, Reach WT, Rebolo R, Reinecke M, Renault C, Ricciardi S, Riller T, Ristorcelli I, Rocha G, Rosset C, Rowan-Robinson M, Rubino-Martin JA, Rusholme B, Sajina A, Sandri M, Savini G, Scott D, Smoot GFet al., 2013, <i>Planck</i> intermediate results VII. Statistical properties of infrared and radio extragalactic sources from the <i>Planck</i> Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz, ASTRONOMY & ASTROPHYSICS, Vol: 550, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bikmaev I, Boehringer H, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Bourdin H, Burenin R, Burigana C, Cabella P, Cardoso J-F, Castex G, Catalano A, Cayon L, Chamballu A, Chary R-R, Chiang L-Y, Chon G, Christensen PR, Clements DL, Colafrancesco S, Colombo LPL, Comis B, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Danese L, Davis RJ, de Bernardis P, de Gasperis G, de Zotti G, Delabrouille J, Democles J, Desert F-X, Diego JM, Dolag K, Dole H, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Flores-Cacho I, Forni O, Frailis M, Franceschi E, Frommert M, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Gilfanov M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Hempel A, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hovest W, Hurier G, Jaffe TR, Jaffe AH, Jagemann T, Jones WC, Juvela M, Khamitov I, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lamarre J-M, Lasenby A, Lawrence CR, Le Jeune M, Leonardi R, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Luzzi G, Macias-Perez JF, Maffei B, Maino D, Mandolesi N, Maris M, Marleau F, Marshall DJ, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, Mei S, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pajot F, Paoletti D, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanen T, Pratt GW, Prunet S, Puget J-L, Rachen JPet al., 2013, <i>Planck</i> intermediate results VIII. Filaments between interacting clusters, ASTRONOMY & ASTROPHYSICS, Vol: 550, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bikmaev I, Bobin J, Boehringer H, Bonaldi A, Bond JR, Borgani S, Borrill J, Bouchet FR, Bourdin H, Brown ML, Burenin R, Burigana C, Cabella P, Cardoso J-F, Carvalho P, Castex G, Catalano A, Cayon L, Chamballu A, Chiang L-Y, Chon G, Christensen PR, Churazov E, Clements DL, Colafrancesco S, Colombi S, Colombo LPL, Comis B, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Danese L, Davis RJ, de Bernardis P, de Gasperis G, de Zotti G, Delabrouille J, Democles J, Desert F-X, Diego JM, Dolag K, Dole H, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Flores-Cacho I, Forni O, Fosalba P, Frailis M, Franceschi E, Frommert M, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Hempel A, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hurier G, Jaffe TR, Jaffe AH, Jagemann T, Jones WC, Juvela M, Keihanen E, Khamitov I, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Le Jeune M, Leonardi R, Liddle A, Lilje PB, Lopez-Caniego M, Luzzi G, Macias-Perez JF, Maino D, Mandolesi N, Maris M, Marleau F, Marshall DJ, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Mazzotta P, Mei S, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pajot F, Paoletti D, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanenet al., 2013, <i>Planck</i> intermediate results V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect, ASTRONOMY & ASTROPHYSICS, Vol: 550, ISSN: 0004-6361

Journal article

Suzuki A, Arnold K, Edwards J, Engargiola G, Ghribi A, Holzapfel W, Lee AT, Meng XF, Myers MJ, O'Brient R, Quealy E, Rebeiz G, Richards P, Rosen D, Siritanasak Pet al., 2012, Multichroic dual-polarization bolometric detectors for studies of the cosmic microwave background, SPIE Proceedings, ISSN: 0277-786X

Journal article

Macaulay E, Feldman HA, Ferreira PG, Jaffe AH, Agarwal S, Hudson MJ, Watkins Ret al., 2012, Power spectrum estimation from peculiar velocity catalogues, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Vol: 425, Pages: 1709-1717, ISSN: 0035-8711

Journal article

Ball WT, Unruh YC, Krivova NA, Solanki S, Wenzler T, Mortlock DJ, Jaffe AHet al., 2012, Reconstruction of total solar irradiance 1974-2009, ASTRONOMY & ASTROPHYSICS, Vol: 541, ISSN: 1432-0746

Journal article

Bao C, Gold B, Baccigalupi C, Didier J, Hanany S, Jaffe A, Johnson BR, Leach S, Matsumura T, Miller A, O'Dea Det al., 2012, THE IMPACT OF THE SPECTRAL RESPONSE OF AN ACHROMATIC HALF-WAVE PLATE ON THE MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND POLARIZATION, ASTROPHYSICAL JOURNAL, Vol: 747, ISSN: 0004-637X

Journal article

Nishino H, Ade P, Anthony A, Arnold K, Barron D, Boettger D, Borril J, Chapman S, Chinone Y, Dobbs MA, Errard J, Fabbian G, Flanigan D, Fuller G, Ghribi A, Grainger W, Halverson N, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Howard J, Hyland P, Jaffe A, Jeune ML, Keating B, Kermish ZD, Kisner T, Lee AT, Linder E, Lungu M, Matsuda F, Matsumura T, Miller N, Morii H, Moyerman S, Myers MJ, Paar H, Reichardt C, Ross C, Schanning I, Shimizu A, Shimmin C, Shimon M, Sholl M, Siritanasak P, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Tomaru T, Tucker C, Quealy E, Richards PL, Zhan Oet al., 2012, The polarbear experiment, Pages: 63-66

Polarbear is a ground-based experiment in the Atacama desert in Chile, designed to measure the polarization of the Cosmic Microwave Background (CMB) radiation. The main science goals of POLARBEAR are to discover B-mode polarization of the CMB due to gravitational waves produced during the epoch of cosmological inflation. Detection of the B-mode polarization pattern in the CMB would provide strong evidence for inflationary cosmological models while the non-detection of B-modes by POLARBEAR would rule out a majority of single-field, slow-roll inflationary models. POLARBEAR will observe 700 square-degrees of the sky at 150 GHz with an array of 1,274 polarized antenna-coupled Transition Edge Sensor (TES) bolometers. POLARBEAR is expected to reach a sensitivity to the tensor-to-scalar ratio r = 0.025 at 95% confidence level, using the data from 2-years of operation. The beam size of 3.5 arcminutes makes it possible to also detect B-mode polarization signals at small-angular scales. These signals originate from weak gravitational lensing and are therefore sensitive to dark energy and the summed masses of neutrinos. POLARBEAR will be able to measure the sum of neutrino masses with a sensitivity of 75 meV, at 68%C.L., when our data are combined with the forthcoming data from Planck HFI. POLARBEAR was deployed in September 2011 and achieved "first-light" four months later, in January 2012. We will report the current status and the future prospects of POLARBEAR.

Conference paper

Sagiv I, Aboobaker AM, Bao C, Hanany S, Jones T, Klein J, Milligan M, Polsgrove DE, Raach K, Zilic K, Korotkov A, Tucker GS, Vinokurov Y, Matsumura T, Ade P, Grainger W, Pascale E, Chapman D, Didier J, Hillbrand S, Reichborn-Kjennerud B, Limon M, Miller A, Jaffe A, Yadav A, Zaldarriaga M, Ponthieu N, Tristram M, Borrill J, Cantalupo C, Kisner T, Aubin F, Dobbs M, Macdermid K, Hilton G, Hubmayr J, Irwin K, Reintsema C, Baccigalupi C, Leach S, Johnson B, Lee A, Tran H, Levinson Let al., 2012, The EBEX cryostat and supporting electronics, 12th Marcel Grossmann Meeting on Recent Dev. in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories - Proc. of the MG 2009 Meeting on General Relativity, Pages: 2166-2176

We describe the cryostat and supporting electronics for the EBEX experiment. EBEX is a balloon-borne polarimeter designed to measure the B-mode polarization of the cosmic microwave background radiation. The instrument includes a 1:5 meter Gregorian-type telescope and 1432 bolometric transition edge sensor detectors operating at 0.3 K. Electronics for monitoring temperatures and controlling cryostat refrigerators is read out over CANbus. A timing system ensures the data from all subsystems is accurately synchronized. EBEX completed an engineering test flight in June 2009 during which the cryogenics and supporting electronics performed according to predictions. The temperatures of the cryostat were stable, and an analysis of a subset of the data finds no scan synchronous signal in the cryostat temperatures. Preparations are underway for an Antarctic flight. Copyright © 2012 by World Scientific Publishing Co. Pte. Ltd.

Journal article

Hasegawa M, Ade PAR, Anthony AE, Arnold K, Barron D, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs MA, Errard J, Fabbian G, Flanigan D, Fuller G, Ghribi A, Grainger W, Halverson N, Hattori K, Hazumi M, Holzapfel WL, Howard J, Hyland P, Jaffe A, Keating B, Kermish Z, Kisner T, Le Jeune M, Lee AT, Linder E, Lungu M, Matsuda F, Matsumura T, Miller NJ, Meng X, Morii H, Moyerman S, Myers MJ, Nishino H, Paar H, Quealy E, Reichardt C, Richards PL, Ross C, Shimizu A, Chimmin C, Shimon M, Sholl M, Siritanasak P, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Tomaru T, Tucker C, Zahn Oet al., 2012, Cosmology and particle physics with POLARBEAR

Cosmic inflation predicts that primordial gravitational waves were created during the inflationary era. Measurements of polarization of the Cosmic Microwave Background (CMB) radiation are known as the best probe to detect the primordial gravitational waves. POLARBEAR is a telescope designed to detect the CMB B-mode with very sensitive polarimeters based on superconductive transition edge sensor (TES) detector technology. Its large primary mirror with a diameter of 3.5m also allows us to constrain or measure the sum of neutrino masses beyond the limit obtained so far. POLARBEAR is located on the Chajnantor plateau in the Atacama desert in northern Chile at an altitude of 5,200m. We received the first light in January 2012 and are taking CMB data at 150 GHz. In this paper we will describe the current status and prospect of POLARBEAR.

Conference paper

Kermish ZD, Ade P, Anthony A, Arnold K, Barron D, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs MA, Errard J, Fabbian G, Flanigan D, Fuller G, Ghribi A, Grainger W, Halverson N, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Howard J, Hyland P, Jaffe A, Keating B, Kisner T, Lee AT, Le Jeune M, Linder E, Lungu M, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Moyerman S, Myers MJ, Nishino H, Paar H, Quealy E, Reichardt CL, Richards PL, Ross C, Shimizu A, Shimon M, Shimmin C, Sholl M, Siritanasak P, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Tomaru T, Tucker C, Zahn Oet al., 2012, The POLARBEAR Experiment, MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VI, Vol: 8452, ISSN: 0277-786X

Journal article

Arnold K, Ade PAR, Anthony AE, Barron D, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs MA, Errard J, Fabbian G, Flanigan D, Fuller G, Ghribi A, Grainger W, Halverson N, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Howard J, Hyland P, Jaffe A, Keating B, Kermish Z, Kisner T, Le Jeune M, Lee AT, Linder E, Lungu M, Matsuda F, Matsumura T, Miller NJ, Meng X, Morii H, Moyerman S, Myers MJ, Nishino H, Paar H, Quealy E, Reichardt C, Richards PL, Ross C, Shimizu A, Shimmin C, Shimon M, Sholl M, Siritanasak P, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Tomaru T, Tucker C, Zahn Oet al., 2012, The bolometric focal plane array of the POLARBEAR CMB experiment, MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VI, Vol: 8452, ISSN: 0277-786X

Journal article

Ade PAR, Aghanim N, Ansari R, Arnaud M, Ashdown M, Aumont J, Banday AJ, Bartelmann M, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bock JJ, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bradshaw T, Breelle E, Bucher M, Camus P, Cardoso J-F, Catalano A, Challinor A, Chamballu A, Charra J, Charra M, Chary R-R, Chiang C, Church S, Clements DL, Colombi S, Couchot F, Coulais A, Cressiot C, Crill BP, Crook M, de Bernardis P, Delabrouille J, Delouis J-M, Desert F-X, Dolag K, Dole H, Dore O, Douspis M, Efstathiou G, Eng P, Filliard C, Forni O, Fosalba P, Fourmond J-J, Ganga K, Giard M, Girard D, Giraud-Heraud Y, Gispert R, Gorski KM, Gratton S, Griffin M, Guyot G, Haissinski J, Harrison D, Helou G, Henrot-Versille S, Hernandez-Monteagudo C, Hildebrandt SR, Hills R, Hivon E, Hobson M, Holmes WA, Huffenberger KM, Jaffe AH, Jones WC, Kaplan J, Kneissl R, Knox L, Lagache G, Lamarre J-M, Lami P, Lange AE, Lasenby A, Lavabre A, Lawrence CR, Leriche B, Leroy C, Longval Y, Macias-Perez JF, Maciaszek T, MacTavish CJ, Maffei B, Mandolesi N, Mann R, Mansoux B, Masi S, Matsumura T, McGehee P, Melin J-B, Mercier C, Miville-Deschenes M-A, Moneti A, Montier L, Mortlock D, Murphy A, Nati F, Netterfield CB, Norgaard-Nielsen HU, North C, Noviello F, Novikov D, Osborne S, Paine C, Pajot F, Patanchon G, Peacocke T, Pearson TJ, Perdereau O, Perotto L, Piacentini F, Piat M, Plaszczynski S, Pointecouteau E, Pons R, Ponthieu N, Prezeau G, Prunet S, Puget J-L, Reach WT, Renault C, Ristorcelli I, Rocha G, Rosset C, Roudier G, Rowan-Robinson M, Rusholme B, Santos D, Savini G, Schaefer BM, Shellard P, Spencer L, Starck J-L, Stassi P, Stolyarov V, Stompor R, Sudiwala R, Sunyaev R, Sygnet J-F, Tauber JA, Thum C, Torre J-P, Touze F, Tristram M, Van Leeuwen F, Vibert L, Vibert D, Wade LA, Wandelt BD, White SDM, Wiesemeyer H, Woodcraft A, Yurchenko V, Yvon D, Zacchei Aet al., 2011, Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance, Astronomy and Astrophysics, Vol: 536, ISSN: 0004-6361

The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the cosmic microwave background and Galactic foregrounds in six ~30% bands centered at 100, 143, 217, 353, 545, and 857 GHz at an angular resolution of 10′ (100 GHz), 7′ (143 GHz), and 5′ (217 GHz and higher). HFI has been operating flawlessly since launch on 14 May 2009, with the bolometers reaching 100 mK the first week of July. The settings of the readout electronics, including bolometer bias currents, that optimize HFI’s noise performance on orbit are nearly the same as the ones chosen during ground testing. Observations of Mars, Jupiter, and Saturn have confirmed that the optical beams and the time responses of the detection chains are in good agreement with the predictions of physical optics modeling and pre-launch measurements. The Detectors suffer from a high flux of cosmic rays due to historically low levels of solar activity. As a result of the redundancy of Planck’s observation strategy, theremoval of a few percent of data contaminated by glitches does not significantly affect the instrumental sensitivity. The cosmic ray flux represents a significant and variable heat load on the sub-Kelvin stage. Temporal variation and the inhomogeneous distribution of the flux results in thermal fluctuations that are a probable source of low frequency noise. The removal of systematic effects in the time ordered data provides a signal with an average noise equivalent power that is 70% of the goal in the 0.6−2.5 Hz range. This is slightly higher than was achieved during the pre-launch characterization but better than predicted in the early phases of the project. The improvement over the goal is a result of the low level of instrumental background loading achieved by the optical and thermal design of the HFI.

Journal article

Ade PAR, Aghanim N, Ansari R, Arnaud M, Ashdown M, Aumont J, Banday AJ, Bartelmann M, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bock JJ, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bradshaw T, Bucher M, Cardoso J-F, Castex G, Catalano A, Challinor A, Chamballu A, Chary R-R, Chen X, Chiang C, Church S, Clements DL, Colley J-M, Colombi S, Couchot F, Coulais A, Cressiot C, Crill BP, Crook M, de Bernardis P, Delabrouille J, Delouis J-M, Desert F-X, Dolag K, Dole H, Dore O, Douspis M, Dunkley J, Efstathiou G, Filliard C, Forni O, Fosalba P, Ganga K, Giard M, Girard D, Giraud-Heraud Y, Gispert R, Gorski KM, Gratton S, Griffin M, Guyot G, Haissinski J, Harrison D, Helou G, Henrot-Versille S, Hernandez-Monteagudo C, Hildebrandt SR, Hills R, Hivon E, Hobson M, Holmes WA, Huffenberger KM, Jaffe AH, Jones WC, Kaplan J, Kneissl R, Knox L, Kunz M, Lagache G, Lamarre J-M, Lange AE, Lasenby A, Lavabre A, Lawrence CR, Le Jeune M, Leroy C, Lesgourgues J, Macias-Perez JF, MacTavish CJ, Maffei B, Mandolesi N, Mann R, Marleau F, Marshall DJ, Masi S, Matsumura T, McAuley I, McGehee P, Melin J-B, Mercier C, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Mortlock D, Murphy A, Nati F, Netterfield CB, Norgaard-Nielsen HU, North C, Noviello F, Novikov D, Osborne S, Pajot F, Patanchon G, Peacocke T, Pearson TJ, Perdereau O, Perotto L, Piacentini F, Piat M, Plaszczynski S, Pointecouteau E, Ponthieu N, Prezeau G, Prunet S, Puget J-L, Reach WT, Remazeilles M, Renault C, Riazuelo A, Ristorcelli I, Rocha G, Rosset C, Roudier G, Rowan-Robinson M, Rusholme B, Saha R, Santos D, Savini G, Schaefer BM, Shellard P, Spencer L, Starck J-L, Stolyarov V, Stompor R, Sudiwala R, Sunyaev R, Sutton D, Sygnet J-F, Tauber JA, Thum C, Torre J-P, Touze F, Tristram M, Van Leeuwen F, Vibert L, Vibert D, Wade LA, Wandelt BD, White SDM, Wiesemeyer H, Woodcraft A, Yurchenko V, Yvon D, Zacchei Aet al., 2011, Planck early results. VI. The High Frequency Instrument data processing, Astronomy and Astrophysics: a European journal, Vol: 536, ISSN: 0004-6361

We describe the processing of the 336 billion raw data samples from the High Frequency Instrument (HFI) which we performed to produce sixtemperature maps from the first 295 days of Planck-HFI survey data. These maps provide an accurate rendition of the sky emission at 100, 143,217, 353, 545 and 857 GHz with an angular resolution ranging from 9.9 to 4.4. The white noise level is around 1.5 μK degree or less in the 3 mainCMB channels (100–217 GHz). The photometric accuracy is better than 2% at frequencies between 100 and 353 GHz and around 7% at the twohighest frequencies. The maps created by the HFI Data Processing Centre reach our goals in terms of sensitivity, resolution, and photometricaccuracy. They are already sufficiently accurate and well-characterised to allow scientific analyses which are presented in an accompanying seriesof early papers. At this stage, HFI data appears to be of high quality and we expect that with further refinements of the data processing we shouldbe able to achieve, or exceed, the science goals of the Planck project.

Journal article

Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartelmann M, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Brown ML, Bucher M, Burigana C, Cabella P, Cardoso J-F, Catalano A, Cayon L, Challinor A, Chamballu A, Chiang L-Y, Chiang C, Chon G, Christensen PR, Churazov E, Clements DL, Colafrancesco S, Colombi S, Couchot F, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Danese L, Davis RJ, de Bernardis P, de Gasperis G, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Diego JM, Dolag K, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Finelli F, Flores-Cacho I, Forni O, Frailis M, Franceschi E, Fromenteau S, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hovest W, Hoyland RJ, Huffenberger KM, Jaffe AH, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kneissl R, Knox L, Kurki-Suonio H, Lagache G, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leach S, Leonardi R, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, MacTavish CJ, Maffei B, Maino D, Mandolesi N, Mann R, Maris M, Marleau F, Martinez-Gonzalez E, Masi S, Matarrese S, Matthai F, Mazzotta P, Mei S, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy A, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, O'Dwyer IJ, Osborne S, Pajot F, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Poutanen T, Pratt GW, Prezeau G, Prunet S, Puget J-L, Rebolo R, Reinecke M, Renault C, Ricciardiet al., 2011, <i>Planck</i> early results. XII. Cluster Sunyaev-Zeldovich optical scaling relations, ASTRONOMY & ASTROPHYSICS, Vol: 536, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartelmann M, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Bourdin H, Brown ML, Bucher M, Burigana C, Cabella P, Cardoso J-F, Catalano A, Cayon L, Challinor A, Chamballu A, Chiang L-Y, Chiang C, Chon G, Christensen PR, Churazov E, Clements DL, Colafrancesco S, Colombi S, Couchot F, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Danese L, de Bernardis P, de Gasperis G, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Diego JM, Dolag K, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Finelli F, Flores-Cacho I, Forni O, Frailis M, Franceschi E, Fromenteau S, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hovest W, Hoyland RJ, Huffenberger KM, Jaffe AH, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kneissl R, Knox L, Kurki-Suonio H, Lagache G, Lamarre J-M, Lanoux J, Lasenby A, Laureijs RJ, Lawrence CR, Leach S, Leonardi R, Liddle A, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, MacTavish CJ, Maffei B, Maino D, Mandolesi N, Mann R, Maris M, Marleau F, Martinez-Gonzalez E, Masi S, Matarrese S, Matthai F, Mazzotta P, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy A, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pajot F, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Poutanen T, Pratt GW, Prezeau G, Prunet S, Puget J-L, Rachen JP, Rebolo Ret al., 2011, <i>Planck</i> early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations, ASTRONOMY & ASTROPHYSICS, Vol: 536, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bucher M, Burigana C, Cabella P, Cappellini B, Cardoso J-F, Casassus S, Catalano A, Cayon L, Challinor A, Chamballu A, Chary R-R, Chen X, Chiang L-Y, Chiang C, Christensen PR, Clements DL, Colombi S, Couchot F, Coulais A, Crill BP, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Gasperis G, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Dickinson C, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Helou G, Henrot-Versille S, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hovest W, Hoyland RJ, Huffenberger KM, Jaffe TR, Jaffe AH, Jones WC, Juvela M, Keihaenen E, Keskitalo R, Kisner TS, Kneissl R, Knox L, Kurki-Suonio H, Lagache G, Laehteenmaeki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leach S, Leonardi R, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, MacTavish CJ, Maffei B, Maino D, Mandolesi N, Mann R, Maris M, Marshall DJ, Martinez-Gonzalez E, Masi S, Matarrese S, Matthai F, Mazzotta P, McGehee P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy A, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, O'Dwyer IJ, Osborne S, Pajot F, Paladini R, Partridge B, Pasian F, Patanchon G, Pearson TJ, Peel M, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Plaszczynski S, Platania P, Pointecouteau E, Polenta G, Ponthieu N, Poutanen T, Prezeau G, Procopio P, Prunet S, Puget J-L, Reach WTet al., 2011, <i>Planck</i> early results. XX. New light on anomalous microwave emission from spinning dust grains, ASTRONOMY & ASTROPHYSICS, Vol: 536, ISSN: 0004-6361

Journal article

Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartelmann M, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Brown ML, Bucher M, Burigana C, Cabella P, Cardoso J-F, Catalano A, Cayon L, Challinor A, Chamballu A, Chary R-R, Chiang L-Y, Chiang C, Chon G, Christensen PR, Churazov E, Clements DL, Colafrancesco S, Colombi S, Couchot F, Coulais A, Crill BP, Cuttaia F, Da Silva A, Dahle H, Danese L, de Bernardis P, de Gasperis G, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Diego JM, Dolag K, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Finelli F, Flores-Cacho I, Forni O, Frailis M, Franceschi E, Fromenteau S, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hovest W, Hoyland RJ, Huffenberger KM, Jaffe AH, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kneissl R, Knox L, Kurki-Suonio H, Lagache G, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leach S, Leonardi R, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, MacTavish CJ, Maffei B, Maino D, Mandolesi N, Mann R, Maris M, Marleau F, Martinez-Gonzalez E, Masi S, Matarrese S, Matthai F, Mazzotta P, Melchiorri A, Melin J-B, Mendes L, Mennella A, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy A, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pajot F, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Piffaretti R, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Poutanen T, Pratt GW, Prezeau G, Prunet S, Puget J-L, Rebolo R, Reinecke M, Renault C, Ricciardi S, Riller T, Ristet al., 2011, <i>Planck</i> early results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters, ASTRONOMY & ASTROPHYSICS, Vol: 536, ISSN: 0004-6361

Journal article

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Bernard J-P, Bersanelli M, Bhatia R, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bucher M, Burigana C, Cabella P, Cantalupo CM, Cardoso J-F, Catalano A, Cayon L, Challinor A, Chamballu A, Chiang L-Y, Christensen PR, Clements DL, Colombi S, Couchot F, Coulais A, Crill BP, Cuttaia F, Danese L, Davies RD, de Bernardis P, de Gasperis G, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Dickinson C, Doi Y, Donzelli S, Dore O, Doerl U, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Falgarone E, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Helou G, Henrot-Versille S, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hovest W, Hoyland RJ, Huffenberger KM, Ikeda N, Jaffe AH, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kitamura Y, Kneissl R, Knox L, Kurki-Suonio H, Lagache G, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leach S, Leonardi R, Leroy C, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, MacTavish CJ, Maffei B, Malinen J, Mandolesi N, Mann R, Maris M, Marshall DJ, Martin P, Martinez-Gonzalez E, Masi S, Matarrese S, Matthai F, Mazzotta P, McGehee P, Melchiorri A, Mendes L, Mennella A, Meny C, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy A, Naselsky P, Nati F, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pagani L, Pajot F, Paladini R, Pasian F, Patanchon G, Pelkonen V-M, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Poutanen T, Prezeau G, Prunet S, Puget J-L, Reach WT, Rebolo R, Reinecke M, Renault C, Ricciardi S, Riller T, Ristorcelli I, Rocha G, Rosseet al., 2011, <i>Planck</i> early results. XXII. The submillimetre properties of a sample of Galactic cold clumps, ASTRONOMY & ASTROPHYSICS, Vol: 536, ISSN: 0004-6361

Journal article

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