Professor Andrew H Jaffe

Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bonaldi A, Bonavera L, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Butler RC, Cappellini B, Cardoso J-F, Catalano A, Chamballu A, Chen X, Chiang L-Y, Christensen PR, Church S, Colombi S, Colombo LPL, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Gaier TC, Galeotta S, Ganga K, Giard M, Giardino G, Giraud-Heraud Y, Gjerlow E, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jewell J, Jones WC, Juvela M, Kangaslahti P, Keihanen E, Keskitalo R, Kisner TS, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leach S, Leahy JP, Leonard R, Lesgourgues J, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Maino D, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Novikov D, Novikov I, O'Dwyer IJ, Osborne S, Paci F, Pagano L, Paladini R, Paoletti D, Partridge B, Pasian F, Patanchon G, Pearson D, Peel M, Perdereau O, Perotto L, Perrotta F, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanen T, Pratt GW, Prezeet al., 2014, <i>Planck</i> 2013 results. V. LFI calibration, ASTRONOMY & ASTROPHYSICS, Vol: 571, ISSN: 0004-6361

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• Citations: 60

Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Butler RC, Cardoso J-F, Catalano A, Chamballu A, Chiang L-Y, Christensen PR, Church S, Colombi S, Colombo LPL, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Gaier TC, Galeotta S, Ganga K, Giard M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jewell J, Jones WC, Juvela M, Kangaslahti P, Keihanen E, Keskitalo R, Kiiveri K, Kisner TS, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leahy JP, Leonardi R, Lesgourgues J, Liguori M, Lilje PB, Linden-Vornle M, Lindholm V, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Maino D, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Novikov D, Novikov I, O'Dwyer IJ, Osborne S, Paci F, Pagano L, Paoletti D, Partridge B, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Pierpaoli E, Pietrobon D, Plaszczynski S, Platania P, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanen T, Pratt GW, Prezeau G, Prunet S, Puget J-L, Rachen JP, Rebolo R, Reinecke M Ret al., 2014, <i>Planck</i> 2013 results. IV. Low Frequency Instrument beams and window functions, ASTRONOMY & ASTROPHYSICS, Vol: 571, ISSN: 0004-6361

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• Citations: 49

Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bonaldi A, Bonavera L, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Butler RC, Cardoso J-F, Catalano A, Chamballu A, Chiang L-Y, Cristensen PR, Church S, Olombi SC, Colombo LPL, Crill BP, Cruz M, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rose A, de Zotti G, Delabrouillei J, Dick J, Dickinson C, Diego JM, Dole H, Donzeli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Gaier TC, Galeotta S, Ganga K, Giard M, Giraud-Heraud Y, Gjerlow E, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jewell J, Jones WC, Juvela M, Kaneaslahti P, Keihanen E, Keskitalo R, Kuveri K, Kisner TS, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leahy JP, Leonardi R, Lesgourgues J, Liguori M, Lilje PB, Linden-Vornle M, Lindholm V, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Maino D, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Mieliaccio M, Mitra S, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Novikov D, Novikov I, O'Dwyer IJ, Osborne S, Paci F, Pagano L, Paladini R, Paoletti D, Partridge B, Pasian F, Patanchon G, Pearson D, Peel M, Perdereau O, Perotto L, Perrotta F, Pierpaoli E, Pietrobon D, Plaszczynski S, Platania P, Pointecouteau E, Polenta G, Ponthieu N, Popa I, Poutanen T, Pratt GWet al., 2014, <i>Planck</i> 2013 results. III. LFI systematic uncertainties, ASTRONOMY & ASTROPHYSICS, Vol: 571, ISSN: 0004-6361

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• Citations: 46

Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bonaldi A, Bonavera L, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Butler RC, Cappellini B, Cardoso J-F, Catalano A, Chamballu A, Chen X, Chiang L-Y, Christensen PR, Church S, Colombi S, Colombo LPL, Crill BP, Cruz M, Curto A, Cattaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Falvella MC, Finelli F, Forni O, Frailis M, Franceschi E, Gaier TC, Galeotta S, Ganga K, Giard M, Giardino G, Giraud-Heraud Y, Gjerlow E, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jewel J, Jones WC, Juvela M, Kangaslahti P, Keihanen E, Keskitalo R, Kiiveri K, Kisner TS, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lattanzi M, Laureijs RJ, Lawrence CR, Leach S, Leahy JP, Leonardi R, Lesgourgues J, Liguori M, Lilje PB, Linden-Vornle M, Lindholm V, Lopez-Caniego M, Lubin PM, Macias-Perez JE, Maggio G, Maino D, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Moneti A, Montier L, Morgantes G, Morisset N, Mortlock D, Moss A, Munshi D, Naseisky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Novikov D, Novikov I, O'Dwyer IJ, Osborne S, Paci F, Pagano L, Paladini R, Paoletti D, Partridge B, Pasian F, Patanchon G, Peel M, Perdereau O, Perotto L, Perrotta F, Pierpaoli E, Pietrobon D, Plaszczynski S, Plataniet al., 2014, <i>Planck</i> 2013 results. II. Low Frequency Instrument data processing, ASTRONOMY & ASTROPHYSICS, Vol: 571, ISSN: 0004-6361

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• Citations: 57

Abergel A, Ade PAR, Aghanim N, Alves MIR, Aniano G, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bridges M, Bucher M, Burigana C, Butler RC, Cardoso J-F, Catalano A, Chamballu A, Chary R-R, Chiang HC, Chiang L-Y, Christensen PR, Church S, Clemens M, Clements DL, Colombi S, Colombo LPL, Combet C, Couchot F, Coulais A, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Draine BT, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Falgarone E, Finelli F, Forni O, Frailis M, Fraisse AA, Franceschi E, Galeotta S, Ganga K, Ghosh T, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Grenier IA, Gruppuso A, Guillet V, Hansen FK, Hanson D, Harrison DL, Helou G, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jewell J, Joncas G, Jones WC, Juvela M, Keihaenen E, Keskitalo R, Kisner TS, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Laehteenmaeki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leonardi R, Leon-Tavares J, Lesgourgues J, Levrier F, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego 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, Matthai F, Mazzotta P, McGehee P, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Oxborrowet al., 2014, <i>Planck</i> 2013 results. XI. All-sky model of thermal dust emission, ASTRONOMY & ASTROPHYSICS, Vol: 571, ISSN: 0004-6361

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• Citations: 469

Ade PAR, Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bethermin M, Bielewicz P, Blagrave K, Bobin J, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bridges M, Bucher M, Burigana C, Butler RC, Cardoso J-F, Catalano A, Challinor A, Chamballu A, Chen X, Chiang HC, Chiang L-Y, Christensen PR, Church S, Clements DL, Colombi S, Colombo LPL, Couchot F, Coulais A, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Ghosh T, Giard M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Helou G, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jones WC, Juvela M, Kalberla P, Keihanen E, Kerp J, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lacasa F, Lagache G, Lahteenmaki A, Lamarre J-M, Langer M, Lasenby A, Laureijs RJ, Lawrence CR, Leonardi R, Leon-Tavares J, Lesgourgues J, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego 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, Matthai F, Mazzotta P, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Oxborrow CA, Paci F, Pagano L, Pajot F, Paladini R, Paoletti D, Partridge B, Pasian F, Patanet al., 2014, <i>Planck</i> 2013 results. XXX. Cosmic infrared background measurements and implications for star formation, ASTRONOMY & ASTROPHYSICS, Vol: 571, ISSN: 0004-6361

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• Citations: 148

Ade PAR, Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Cardoso J-F, Catalano A, Challinor A, Chamballu A, Chiang HC, Chiang L-Y, Christensen PR, Church S, Clements DL, Colombi S, Colombo LPL, Couchot F, Coulais A, Crill P, Curto A, Cuttaia F, Danese L, Davies RD, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Gana K, Giard M, Girard D, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leonardi R, Leroy C, Lesgourgues J, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, McGehee P, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Miniussi A, Mitra A, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Mottet S, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Oxborrow CA, Paci F, Pagano L, Pajot F, Paoletti D, Pasian F, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanen T, Pratt GW, Prezeau Get al., 2014, Planck 2013 results. X. HFI energetic particle effects: characterization, removal, and simulation, Astronomy & Astrophysics, Vol: 571, ISSN: 1432-0746

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Ade PAR, Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Bartlett JG, Bartolo N, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bonaldi A, Bonavera L, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Butler RC, Cardoso J-F, Catalano A, Challinor A, Chamballu A, Chiang HC, Chiang L-Y, Christensen PR, Church S, Clements DL, Colombi S, Colombo LPL, Couchot F, Coulais A, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Ducout A, Dunkley J, Dupac X, Efstathiou G, Elsner F, Ensslin TA, Eriksen HK, Fergusson J, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Giard M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Heavens A, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lacasa F, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leahy JP, Leonardi R, Lesgourgues J, Lewis A, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Maffei B, Maino D, Mandolesi N, Mangilli A, Marinucci D, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Murphy JA, Naselsky P, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Oxborrowl CA, Paci F, Pagano L, Pajot F, Paoletti D, Pasian F, Patanchon G, Peiris HV, Perdet al., 2014, Planck 2013 results. XXIV. Constraints on primordial non-Gaussianity, Astronomy & Astrophysics, Vol: 571, ISSN: 1432-0746

The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG). Using three optimal bispectrum estimators, separable template-fitting (KSW), binned, and modal, we obtain consistent values for the primordial local, equilateral, and orthogonal bispectrum amplitudes, quoting as our final result fNLlocal = 2.7 ± 5.8, fNLequil = -42 ± 75, and fNLorth = -25 ± 39 (68% CL statistical). Non-Gaussianity is detected in the data; using skew-Cℓ statistics we find a nonzero bispectrum from residual point sources, and the integrated-Sachs-Wolfe-lensing bispectrum at a level expected in the ΛCDM scenario. The results are based on comprehensive cross-validation of these estimators on Gaussian and non-Gaussian simulations, are stable across component separation techniques, pass an extensive suite of tests, and are confirmed by skew-Cℓ, wavelet bispectrum and Minkowski functional estimators. Beyond estimates of individual shape amplitudes, we present model-independent, three-dimensional reconstructions of the Planck CMB bispectrum and thus derive constraints on early-Universe scenarios that generate primordial NG, including general single-field models of inflation, excited initial states (non-Bunch-Davies vacua), and directionally-dependent vector models. We provide an initial survey of scale-dependent feature and resonance models. These results bound both general single-field and multi-field model parameter ranges, such as the speed of sound, cs ≥ 0.02 (95% CL), in an effective field theory parametrization, and the curvaton decay fraction rD ≥ 0.15 (95% CL). The Planck data significantly limit the viable parameter space of the ekpyrotic/cyclic scenarios. The amplitude of the four-point function in the local model τNL< 2800 (95% CL). Taken together, these constraints represent the highest precision tests to date of physical mechanisms for the origin of cosmic structure.

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Ade PAR, Aghanim N, Alves MIR, Armitage-Caplan C, Amaud M, Ashdown M, Atrio-Barandela F, Aumont J, Ausse H, Baccigalupi C, Banday AJ, Barreiro RB, Barrenass R, Bartelmann M, Bartlett JG, Bartolo N, Basak S, Battaner E, Battye R, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bertincourt B, Bethermin M, Bielewicz P, Bikmaev I, Blanchard A, Bobin J, Bock JJ, Boehringer H, Bonaldi A, Bonavera L, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bourdin H, Bowyer JW, Bridges M, Brown ML, Bucher M, Burenin R, Burigana C, Butler RC, Calabrese E, Cappellini B, Cardoso J-F, Carr R, Carvalho P, Casale M, Castexl G, Catalano A, Challinor A, Chamballu A, Chary R-R, Chen X, Chiang HC, Chiang L-Y, Chon G, Christensen PR, Churazov E, Church S, Clemens M, Clements DL, Colombi S, Colombo LPL, Combet C, Comis B, Couchot E, Coulais A, Crill BP, Cruz M, Curto A, Cuttaia F, Da Silva A, Dahle H, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Dechelette T, Delabrouille J, Delouis J-M, Democles J, Desert F-X, Dick J, Dickinson C, Diego JM, Dolag K, Dole H, Donzelli S, Dore O, Douspis M, Ducout A, Dunkley J, Dupac X, Efstathiou G, Elsner F, Ensslin TA, Eriksen HK, Fabre O, Falgarone E, Falvella MC, Fantaye Y, Fergusson J, Filliard C, Finelli F, Flores-Cacho I, Foley S, Forni O, Fosalba P, Frailis M, Fraisse AA, Franceschi E, Freschi M, Fromenteau S, Frommert M, Gaier TC, Galeotta S, Gallegos J, Galli S, Gandolfo B, Ganga K, Gauthier C, Genova-Santos RT, Ghosh T, Giard M, Giardino G, Gilfanov M, Girard D, Giraud-Heraud Y, Gjerlow E, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Gudmundsson JE, Haissinski J, Hamann J, Hansen FK, Hansen M, Hanson D, Harrison DL, Heavens A, Helou G, Hempel A, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Ho S, Hobson M, Holmes WA, Hornstrup A, Hou Z, Hovest W, Huey G, Huffenberger KM, Hurier G, Ilic S, Jaffe AH, Jaffe TR, Jasches J, Jewell J, Jones WC, Juvela M, Kalberla P, Kaet al., 2014, Planck 2013 results. I. Overview of products and scientific results, Astronomy & Astrophysics, Vol: 571, ISSN: 1432-0746

The European Space Agency’s Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5 months of Planck data, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the cosmic microwave background (CMB) and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the Sunyaev-Zeldovich effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter ΛCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25σ. Planck finds no evidence for non-Gaussianity in the CMB. Planck’s results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluc

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Ade PAR, Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Bartlett JG, Bartolo N, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Butler RC, Calabrese E, Cardoso J-F, Catalano A, Challinor A, Chamballu A, Chiang HC, Chiang L-Y, Christensen PR, Church S, Clements DL, Colombi S, Colombo LPL, Couchot F, Coulais A, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dunkley J, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Gauthier C, Giard M, Giardino G, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hamann J, Hansen FK, Hanson D, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jones WC, Juvela M, Keihaenen E, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Laehteenmaeki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leach S, Leahy JP, Leonardi R, Lesgourgues J, Lewis A, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego 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, Matthai F, Mazzotta P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, O'Dwyer IJ, Osborne S, Oxborrow CA, Paci F, Pagano L, Pajot F, Paladini R, Pandolfi S, Paoletti D, Paret al., 2014, Planck 2013 results. XXII. Constraints on inflation, Astronomy and Astrophysics, Vol: 571, Pages: 1-43, ISSN: 1432-0746

We analyse the implications of the Planck data for cosmic inflation. The Planck nominal mission temperature anisotropy measurements, combinedwith the WMAP large-angle polarization, constrain the scalar spectral index to be ns = 0.9603 ± 0.0073, ruling out exact scale invariance atover 5σ. Planck establishes an upper bound on the tensor-to-scalar ratio of r < 0.11 (95% CL). The Planck data thus shrink the space of allowedstandard inflationary models, preferring potentials with V00 < 0. Exponential potential models, the simplest hybrid inflationary models, andmonomial potential models of degree n ≥ 2 do not provide a good fit to the data. Planck does not find statistically significant running of thescalar spectral index, obtaining dns/dln k = −0.0134 ± 0.0090. We verify these conclusions through a numerical analysis, which makes no slowrollapproximation, and carry out a Bayesian parameter estimation and model-selection analysis for a number of inflationary models includingmonomial, natural, and hilltop potentials. For each model, we present the Planck constraints on the parameters of the potential and exploreseveral possibilities for the post-inflationary entropy generation epoch, thus obtaining nontrivial data-driven constraints. We also present a directreconstruction of the observable range of the inflaton potential. Unless a quartic term is allowed in the potential, we find results consistent withsecond-order slow-roll predictions. We also investigate whether the primordial power spectrum contains any features. We find that models with aparameterized oscillatory feature improve the fit by ∆χ2eff ≈ 10; however, Bayesian evidence does not prefer these models. We constrain severalsingle-field inflation models with generalized Lagrangians by combining power spectrum data with Planck bounds on fNL. Planck constrains withunprecedented accuracy the amplitude and possible correlation (with the adiabatic mode) of non-decaying iso

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Ade PAR, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bond JR, Borrill J, Bouchet FR, Burigana C, Cardoso J-F, Catalano A, Challinor A, Chamballu A, Chiang HC, Christensen PR, Clements DL, Colombi S, Colombo LPL, Couchot F, Coulais A, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Desert F-X, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Fraisse AA, Franceschi E, Galeotta S, Ganga K, Giard M, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Gudmundsson JE, Hansen FK, Hanson D, Harrison DL, Henrot-Versille S, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jones WC, Keihaenen E, Keskitalo R, Knoche J, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Leonardi R, Leon-Tavares J, Lesgourgues J, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Maino D, Mandolesi N, Maris M, Martin PG, Martinez-Gonzalez E, Masi S, Matarrese S, Mazzotta P, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Oxborrow CA, Pagano L, Pajot F, Paoletti D, Partridge B, Pasian F, Patanchon G, Pearson D, Pearson TJ, Perdereau O, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Pratt GW, Prunet S, Puget J-L, Rachen JP, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Ristorcelli I, Rocha G, Roudier G, Rubino-Martin JA, Rusholme B, Sandri M, Scott D, Stolyarov V, Sudiwala R, Sutton D, Suur-Uski A-S, Sygnet J-F, Tauber JA, Tereet al., 2014, Planck 2013 results. XXXI. Consistency of the Planck data, Astronomy & Astrophysics, Vol: 571, ISSN: 1432-0746

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Ade PAR, Akiba Y, Anthony AE, Arnold K, Atlas M, Barron D, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs M, Elleflot T, Errard J, Fabbian G, Feng C, Flanigan D, Gilbert A, Grainger W, Halverson NW, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Hori Y, Howard J, Hyland P, Inoue Y, Jaehnig GC, Jaffe AH, Keating B, Kermish Z, Keskitalo R, Kisner T, Le Jeune M, Lee AT, Leitch EM, Linder E, Lungu M, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Moyerman S, Myers MJ, Navaroli M, Nishino H, Orlando A, Paar H, Peloton J, Poletti D, Quealy E, Rebeiz G, Reichardt CL, Richards PL, Ross C, Schanning I, Schenck DE, Sherwin BD, Shimizu A, Shimmin C, Shimon M, Siritanasak P, Smecher G, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Takakura S, Tomaru T, Wilson B, Yadav A, Zahn Oet al., 2014, A measurement of the cosmic microwave background b-mode polarization power spectrum at sub-degree scales with POLARBEAR, Astrophysical Journal, Vol: 794, ISSN: 0004-637X

We report a measurement of the B-mode polarization power spectrum in the cosmic microwave background (CMB) using the POLARBEAR experiment in Chile. The faint B-mode polarization signature carries information about the universe's entire history of gravitational structure formation, and the cosmic inflation that may have occurred in the very early universe. Our measurement covers the angular multipole range 500 < ℓ < 2100 and is based on observations of an effective sky area of 25 $\deg ^2$ with 3farcm5 resolution at 150 GHz. On these angular scales, gravitational lensing of the CMB by intervening structure in the universe is expected to be the dominant source of B-mode polarization. Including both systematic and statistical uncertainties, the hypothesis of no B-mode polarization power from gravitational lensing is rejected at 97.2% confidence. The band powers are consistent with the standard cosmological model. Fitting a single lensing amplitude parameter ABB to the measured band powers, $A_{BB} = 1.12 \pm 0.61 ({\rm stat}) ^{+0.04}_{-0.12}({\rm sys}) \pm 0.07 ({\rm multi})$, where ABB = 1 is the fiducial WMAP-9 ΛCDM value. In this expression, "stat" refers to the statistical uncertainty, "sys" to the systematic uncertainty associated with possible biases from the instrument and astrophysical foregrounds, and "multi" to the calibration uncertainties that have a multiplicative effect on the measured amplitude ABB.

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Barron D, Ade P, Anthony A, Arnold K, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs M, Edwards J, Errard J, Fabbian G, Flanigan D, Fuller G, Ghribi A, Grainger W, Halverson N, Hasegawa M, Hattori K, Hazumi M, Holzapfel W, Howard J, Hyland P, Jaehnig G, Jaffe A, Keating B, Kermish Z, Keskitalo R, Kisner T, Lee AT, Le Jeune M, Linder E, Lungu M, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Moyerman S, Myers M, Nishino H, Paar H, Peloton J, Quealy E, Rebeiz G, Reichardt CL, 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, Yadav A, Zahn Oet al., 2014, The POLARBEAR Cosmic Microwave Background Polarization Experiment, JOURNAL OF LOW TEMPERATURE PHYSICS, Vol: 176, Pages: 726-732, ISSN: 0022-2291

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Kitching TD, Heavens AF, Alsing J, Erben T, Heymans C, Hildebrandt H, Hoekstra H, Jaffe A, Kiessling A, Mellier Y, Miller L, van Waerbeke L, Benjamin J, Coupon J, Fu L, Hudson MJ, Kilbinger M, Kuijken K, Rowe BTP, Schrabback T, Semboloni E, Velander Met al., 2014, 3D cosmic shear: cosmology from CFHTLenS, Monthly Notices of the Royal Astronomical Society, Vol: 442, Pages: 1326-1349, ISSN: 0035-8711

This paper presents the first application of 3D cosmic shear to a wide-field weak lensing survey. 3D cosmic shear is a technique that analyses weak lensing in three dimensions using a spherical harmonic approach, and does not bin data in the redshift direction. This is applied to CFHTLenS, a 154 square degree imaging survey with a median redshift of 0.7 and an effective number density of 11 galaxies per square arcminute usable for weak lensing. To account for survey masks we apply a 3D pseudo-Cℓ approach on weak lensing data, and to avoid uncertainties in the highly non-linear regime, we separately analyse radial wavenumbers k ≤ 1.5 and 5.0 h Mpc−1, and angular wavenumbers ℓ ≈ 400–5000. We show how one can recover 2D and tomographic power spectra from the full 3D cosmic shear power spectra and present a measurement of the 2D cosmic shear power spectrum, and measurements of a set of 2-bin and 6-bin cosmic shear tomographic power spectra; in doing so we find that using the 3D power in the calculation of such 2D and tomographic power spectra from data naturally accounts for a minimum scale in the matter power spectrum. We use 3D cosmic shear to constrain cosmologies with parameters ΩM, ΩB, σ8, h , ns, w0 and wa. For a non-evolving dark energy equation of state, and assuming a flat cosmology, lensing combined with Wilkinson Microwave Anisotropy Probe 7 results in h = 0.78 ± 0.12, ΩM = 0.252 ± 0.079, σ8 = 0.88 ± 0.23 and w = −1.16 ± 0.38 using only scales k ≤ 1.5  h Mpc−1. We also present results of lensing combined with first year Planck results, where we find no tension with the results from this analysis, but we also find no significant improvement over the Planck results alone. We find evidence of a suppression of power compared to Lambda cold dark matter (LCDM) on small scales 1.5 < k ≤ 5.0 h Mpc−1 in the l

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Ade PAR, Akiba Y, Anthony AE, Arnold K, Atlas M, Barron D, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs M, Elleflot T, Errard J, Fabbian G, Feng C, Flanigan D, Gilbert A, Grainger W, Halverson NW, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Hori Y, Howard J, Hyland P, Inoue Y, Jaehnig GC, Jaffe A, Keating B, Kermish Z, Keskitalo R, Kisner T, Le Jeune M, Lee AT, Linder E, Leitch EM, Lungu M, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Moyerman S, Myers MJ, Navaroli M, Nishino H, Paar H, Peloton J, Quealy E, Rebeiz G, Reichardt CL, Richards PL, Ross C, Schanning I, Schenck DE, Sherwin B, Shimizu A, Shimmin C, Shimon M, Siritanasak P, Smecher G, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Takakura S, Tomaru T, Wilson B, Yadav A, Zahn Oet al., 2014, Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum with the POLARBEAR Experiment, PHYSICAL REVIEW LETTERS, Vol: 113, ISSN: 0031-9007

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• Citations: 117

Abergel A, Ade PAR, Aghanim N, Alves MIR, Aniano G, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Bartett JG, Battaner E, Benabed K, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bonaldi A, Bond JR, Bouchet FR, Boulanger F, Burigana C, Cardoso J-F, Catalano A, Chamballu A, Chiang HC, Christensen PR, Clements DL, Colombi S, Colombo LPL, Couchot F, Crill BP, Cuttaia F, Danese L, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Desert F-X, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Falgarone E, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Ghosh T, Giard M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Guillet V, Hansen FK, Harrison D, Helou G, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Joncas G, Jones A, Jones WC, Juvela M, Kalberla P, Kaihanen E, Kerp J, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Leonardi R, Levrier F, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego 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, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Noviello F, Novikov D, Novikov I, Oxborrow CA, Pagano L, Pajot F, Paoletti D, Pasian F, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Pratt GW, Prunet S, Puget J-L, Rachen JP, Reach WT, Rebolo R, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Riller T, Ristorcelli I, Rocha G, Rosset C, Roudier G Ret al., 2014, Planck intermediate results XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies, ASTRONOMY & ASTROPHYSICS, Vol: 566, ISSN: 0004-6361

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• Citations: 81

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bonaldi A, Bond JR, Bouchet FR, Burigana C, Cardoso J-F, Catalano A, Chamballu A, Chiang HC, Christensen PR, Clements DL, Colombi S, Colombo LPL, Couchot F, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Galli S, Ganga K, Giard M, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison DL, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Leonardi R, Liddle A, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Maffei B, Maino D, Mandolesi N, Maris M, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Mazzotta P, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Noviello F, Novikov D, Novikov I, Oxborrow CA, Pagano L, Pajot F, Paoletti D, Pasian F, Perdereau O, Perotto L, Perrotta F, Pettorino V, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Popa L, Pratt GW, Puget J-L, Rachen JP, Rebolo R, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Riller T, Ristorcelli I, Rocha G, Rosset C, Roudier G, d'Orfeuil BR, Rubino-Martin JA, Rusholme B, Sandri M, Savelainen M, Savini G, Spencer LD, Spinelli M, Starck J-L, Sureau F, Sutton D, Suur-Uski A-S, Sygnet J-F, Tauber JA, Terenzet al., 2014, <i>Planck</i> intermediate results XVI. Profile likelihoods for cosmological parameters, ASTRONOMY & ASTROPHYSICS, Vol: 566, ISSN: 0004-6361

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• Citations: 69

Ade PAR, Akiba Y, Anthony AE, Arnold K, Atlas M, Barron D, Boettger D, Borrill J, Borys C, Chapman S, Chinone Y, Dobbs M, Elleflot T, Errard J, Fabbian G, Feng C, Flanigan D, Gilbert A, Grainger W, Halverson NW, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Hori Y, Howard J, Hyland P, Inoue Y, Jaehnig GC, Jaffe A, Keating B, Kermish Z, Keskitalo R, Kisner T, Le Jeune M, Lee AT, Leitch EM, Linder E, Lungu M, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Moyerman S, Myers MJ, Navaroli M, Nishino H, Paar H, Peloton J, Poletti D, Quealy E, Rebeiz G, Reichardt CL, Richards PL, Ross C, Rotermund K, Schanning I, Schenck DE, Sherwin BD, Shimizu A, Shimmin C, Shimon M, Siritanasak P, Smecher G, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Takakura S, Tikhomirov A, Tomaru T, Wilson B, Yadav A, Zahn Oet al., 2014, Evidence for Gravitational Lensing of the Cosmic Microwave Background Polarization from Cross-Correlation with the Cosmic Infrared Background, PHYSICAL REVIEW LETTERS, Vol: 112, ISSN: 0031-9007

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• Citations: 71

Ade PAR, Aghanim N, Alves MIR, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Bartlett JG, Battaner E, Benabed K, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bucher M, Burigana C, Butler RC, Cardoso J-F, Catalano A, Chamballu A, Chiang HC, Chiang L-Y, Christensen PR, Clements DL, Colombi S, Colombo LPL, Couchot F, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Dickinson C, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Ensslin TA, Eriksen HK, Falgarone E, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Ganga K, Ghosh T, Giard M, Giardino G, Gonzalez-Nuevo J, Gorski KM, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Holmes WA, Hornstrup A, Hovest W, Jaffe AH, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leonardi R, Levrier F, Liguori M, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Macias-Perez JF, Maffei B, Maino D, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Matarrese S, Mazzotta P, Melchiorri A, Mendes L, Mennella A, Migliaccio M, 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, Oxborrow CA, Pagano L, Pajot F, Paladini R, Paoletti D, Pasian F, Patanchon G, Peel M, Perdereau O, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Pratt GW, Prunet S, Puget J-L, Rachen JP, Reach WT, Rebolo R, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Riller T, Ristorcelli I, Rocha G, Rosset C, Rubino-Martin JA, Rusholme B, Sandri M, Savini G, Scott D, Spet al., 2014, <i>Planck</i> intermediate results. XIV. Dust emission at millimetre wavelengths in the Galactic plane, ASTRONOMY & ASTROPHYSICS, Vol: 564, ISSN: 0004-6361

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• Citations: 35

Nishino H, Ade P, Akiba Y, Anthony A, Arnold K, Barron D, Boettger D, Borrill J, Chapmann S, Chinone Y, Dobbs MA, Errard J, Fabbian G, Feng C, Flanigan D, Fuller G, Ghribi A, Grainger W, Halverson N, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Howard J, Hyland P, Inoue Y, Jaffe A, Jaehnig G, Kaneko Y, Katayama N, Keating B, Kermish Z, Kimura N, Kisner T, Lee AT, Le Jeune M, Linder E, Lungu M, Matsuda F, Matsumura T, Miller NJ, Morii H, Moyerman S, Myers MJ, O’Brient R, Okamura T, Paar H, Peloton J, 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, Suzuki J, Tanaka K, Tomaru T, Tucker C, Yadav A, Zahn Oet al., 2014, POLARBEAR CMB Polarization Experiment, Proceedings of the 12th Asia Pacific Physics Conference (APPC12), Publisher: Journal of the Physical Society of Japan

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André P, Baccigalupi C, Banday A, Barbosa D, Barreiro B, Bartlett J, Bartolo N, Battistelli E, Battye R, Bendo G, Benoît A, Bernard JP, Bersanelli M, Béthermin M, Bielewicz P, Bonaldi A, Bouchet F, Boulanger F, Brand J, Bucher M, Burigana C, Cai ZY, Camus P, Casas F, Casasola V, Castex G, Challinor A, Chluba J, Chon G, Colafrancesco S, Comis B, Cuttaia F, Dalessandro G, Silva AD, Davis R, Avillez MD, Bernardis PD, Petris MD, Rosa AD, Zotti GD, Delabrouille J, Désert FX, Dickinson C, Diego JM, Dunkley J, Enßlin T, Errard J, Falgarone E, Ferreira P, Ferrière K, Finelli F, Fletcher A, Fosalba P, Fuller G, Galli S, Ganga K, García-Bellido J, Ghribi A, Giard M, Giraud-Héraud Y, Gonzalez-Nuevo J, Grainge K, Gruppuso A, Hall A, Hamilton JC, Haverkorn M, Hernandez-Monteagudo C, Herranz D, Jackson M, Jaffe A, Khatri R, Kunz M, Lamagna L, Lattanzi M, Leahy P, Lesgourgues J, Liguori M, Liuzzo E, Lopez-Caniego M, Macias-Perez J, Maffei B, Maino D, Mangilli A, Martinez-Gonzalez E, Martins CJAP, Masi S, Massardi M, Matarrese S, Melchiorri A, Melin JB, Mennella A, Mignano A, Miville-Deschênes MA, Monfardini A, Murphy A, Naselsky P, Nati F, Natoli P, Negrello M, Noviello Fet al., 2014, PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An extended white paper, Journal of Cosmology and Astroparticle Physics, Vol: 2014

PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high resolution, high sensitivity, full-sky observations of the sky emission at wavelengths ranging from millimeter-wave to the far-infrared. PRISM's main objective is to explore the distant universe, probing cosmic history from very early times until now as well as the structures, distribution of matter, and velocity flows throughout our Hubble volume. PRISM will survey the full sky in a large number of frequency bands in both intensity and polarization and will measure the absolute spectrum of sky emission more than three orders of magnitude better than COBE FIRAS. The data obtained will allow us to precisely measure the absolute sky brightness and polarization of all the components of the sky emission in the observed frequency range, separating the primordial and extragalactic components cleanly from the galactic and zodiacal light emissions. The aim of this Extended White Paper is to provide a more detailed overview of the highlights of the new science that will be made possible by PRISM, which include: (1) the ultimate galaxy cluster survey using the Sunyaev-Zeldovich (SZ) effect, detecting approximately 106 clusters extending to large redshift, including a characterization of the gas temperature of the brightest ones (through the relativistic corrections to the classic SZ template) as well as a peculiar velocity survey using the kinetic SZ effect that comprises our entire Hubble volume; (2) a detailed characterization of the properties and evolution of dusty galaxies, where the most of the star formation in the universe took place, the faintest population of which constitute the diffuse CIB (Cosmic Infrared Background); (3) a characterization of the B modes from primordial gravity waves generated during inflation and from

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• Citations: 216

Peloton J, Ade PAR, Akiba Y, Anthony AE, Arnold K, Atlas M, Barron D, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs M, Elleflot T, Errard J, Fabbian G, Feng C, Flanigan D, Gilbert A, Grainger W, Halverson NW, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Hori Y, Howard J, Hyland P, Inoue Y, Jaehnig GC, Jaffe AH, Keating B, Kermish Z, Keskitalo R, Kisner T, Le Jeune M, Lee AT, Leitch EM, Linder E, Lungu M, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Moyerman S, Myers MJ, Navaroli M, Nishino H, Paar H, Poletti D, Quealy E, Rebeiz G, Reichardt CL, Richards PL, Ross C, Schanning I, Schenck DE, Sherwin BD, Shimizu A, Shimmin C, Shimon M, Siritanasak P, Smecher G, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Takakura S, Tomaru T, Wilson B, Yadav A, Zahn Oet al., 2014, Polarbear experiment: Data analysis of the first season, Pages: 363-364

Polarbear is a ground-based cosmic microwave background (CMB) polarization experiment located on the Atacama Desert in Chile. The experiment has recently reported its first science results based on the analysis of the first data set collected during 2013 observational campaign. In this proceeding, I focus on the data analysis pipelines, which lead to the production of these results. I describe the data analysis challenge faced by the collaboration, highlighting some steps of the analysis from time-ordered data processing and map mapking to the power spectra estimation.

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Didier J, Aboobaker AM, Ade P, Aubin F, Baccigalupi C, Bandura K, Bao C, Borrill J, Chandra B, Chapman D, Dobbs M, Grain J, Grainger W, Hanany S, Helson K, Hillbrand S, Hilton G, Hubmayr H, Irwin K, Johnson B, Jaffe A, Jones T, Kisner T, Klein J, Korotkov A, Lee A, Levinson L, Limon M, Macdermid K, Miller A, Milligan M, Pascale E, Puglisi G, Raach K, Reichborn-Kjennerud B, Reintsema C, Sagiv I, Smecher G, Stompor R, Tristram M, Tucker G, Westbrook B, Zilic Ket al., 2014, EBEX, the E and B experiment, Pages: 41-44

The E and B experiment (EBEX) is a balloon-borne telescope designed to measure the polarization of the cosmic microwave background radiation as well as that from Galactic dust. The instrument is equipped with a 1.5 meter aperture Gregorian-Dragone telescope, providing an 8' beam at three frequency bands centered on 150, 250 and 410 GHz. Polarimetry is achieved by rotating an achromatic half-wave plate on a superconducting magnetic bearing. In January 2013, EBEX completed 11 days of observations in a flight over Antarctica covering 6000 square degrees of the sky. This marks the first time that arrays with about 1000 transition-edge sensor bolometers have made science observations on a balloon-borne platform. These proceedings describe the EBEX instrument, the science flight and the status of the data analysis.

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• Citations: 1

Fabbian G, Ade PAR, Akiba Y, Anthony AE, Arnold K, Atlas M, Barron D, Boettger D, Borrill J, Chapman S, Chinone Y, Dobbs M, Elleflot T, Errard J, Feng C, Flanigan D, Gilbert A, Grainger W, Halverson NW, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Hori Y, Howard J, Hyland P, Inoue Y, Jaehnig GC, Jaffe AH, Keating B, Kermish Z, Keskitalo R, Kisner T, Le Jeune M, Lee AT, Leitch EM, Linder E, Lungu M, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Moyerman S, Myers MJ, Navaroli M, Nishino H, Paar H, Peloton J, Poletti D, Quealy E, Rebeiz G, Reichardt CL, Richards PL, Ross C, Schanning I, Schenck DE, Sherwin BD, Shimizu A, Shimmin C, Shimon M, Siritanasak P, Smecher G, Spieler H, Stebor N, Steinbach B, Stompor R, Suzuki A, Takakura S, Tomaru T, Wilson B, Yadav A, Zahn Oet al., 2014, The POLARBEAR experiment: Results from the first observational campaign and prospects, Pages: 45-52

The POLARBEAR experiment is one of the few ongoing ground-based Cosmic Microwave Background (CMB) polarization experiment. The experiment is located in the Atacama desert in northern Chile and is designed to target both large and small scales anisotropies thanks to the combination of high angular resolution and large sky-fraction accessible from its mid-latitude site. We review the results of the analysis activity conducted on the data collected during the first observational campaign. These include the first measurement of B-modes of polarization on sub-degree angular scales together with the first reconstruction of the projected matter distribution between us and the epoch of recombination (lensing potential) using CMB polarization data alone. The measurement of the lensing potential was validated through cross-correlation of the matter distribution measured by the Herschel satellite. Finally, we discuss the upcoming experimental upgrades of the experiment.

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MacDermid K, Aboobaker AM, Ade P, Aubin F, Baccigalupi C, Bandura K, Bao C, Borrill J, Chapman D, Didier J, Dobbs M, Grain J, Grainger W, Hanany S, Helson K, Hillbrand S, Hilton G, Hubmayr H, Irwin K, Johnson B, Jaffe A, Jones T, Kisner T, Klein J, Korotkov A, Lee A, Levinson L, Limon M, Miller A, Milligan M, Pascale E, Raach K, Reichborn-Kjennerud B, Reintsema C, Sagiv I, Smecher G, Stompor R, Tristram M, Tucker G, Westbrook B, Zilic Ket al., 2014, The performance of the bolometer array and readout system during the 2012/2013 flight of the e and B experiment (EBEX), ISSN: 0277-786X

EBEX is a balloon-borne telescope designed to measure the polarization of the cosmic microwave background radiation. During its eleven day science flight in the Austral Summer of 2012, it operated 955 spider-web transition edge sensor (TES) bolometers separated into bands at 150, 250 and 410 GHz. This is the first time that an array of TES bolometers has been used on a balloon platform to conduct science observations. Polarization sensitivity was provided by a wire grid and continuously rotating half-wave plate. The balloon implementation of the bolometer array and readout electronics presented unique development requirements. Here we present an outline of the readout system, the remote tuning of the bolometers and Superconducting QUantum Interference Device (SQUID) amplifiers, and preliminary current noise of the bolometer array and readout system.

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• Citations: 15

Ade PAR, Aghanim N, Arnaud M, Ashdown M, Aumont J, Baccigalupi C, Balbi A, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bikmaev I, Bobin J, Bock JJ, Bonaldi A, Bond JR, Borrill J, Bouchet FR, Burigana C, Butler RC, Cabella P, Cardoso J-F, Catalano A, Chamballu A, Chiang L-Y, Chon G, Christensen PR, Clements DL, Colombi S, Colombo LPL, Crill BP, Cuttaia F, Da Silva A, Dahle H, Davies RD, 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, Ensslin TA, Finelli F, Flores-Cacho I, Forni O, Frailis M, Frommert M, Galeotta S, Ganga K, Genova-Santos RT, Giard M, Giardino G, Gonzalez-Nuevo J, Gregorio A, Gruppuso A, Hansen FK, Harrison D, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Holmes WA, Hovest W, Huffenberger KM, Hurier G, Jaffe TR, Jaffe AH, Jasche J, Jones WC, Juvela M, Keihanen E, Keskitalo R, Khamitov I, Kisner TS, Knoche J, Kunz M, Kurki-Suonio H, Lagache G, Lahteenmaki A, Lamarre J-M, Lasenby A, Lawrence CR, Le Jeune M, Leonardi R, Lilje PB, Linden-Vornle M, Lopez-Caniego M, Macias-Perez JF, Maino D, Mak DSY, Mandolesi N, Maris M, Marleau F, Martinez-Gonzalez E, Masi S, Matarrese S, Mazzotta P, Melchiorri A, Melin J-B, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschenes M-A, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Pagano L, Paoletti D, Perdereau O, 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, Puisieux S, Rachen JP, Rebolo R, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Roman M, Rubino-Martin JA, Rusholme B, Sandri M, Savini G, Scott D, Spencer L, Sunyaev R, Sutton D, Suur-Uski A-S, Sygnet J-F, Tauber JA, Terenzi L, Toffoet al., 2014, <i>Planck</i> intermediate results XIII. Constraints on peculiar velocities, ASTRONOMY & ASTROPHYSICS, Vol: 561, ISSN: 0004-6361

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• Citations: 69

Arnold K, Stebor N, Ade PAR, Akiba Y, Anthony AE, Atlas M, Barron D, Bender A, Boettger D, Borrill J, Chapman S, Chinone Y, Cukierman A, Dobbs M, Elleflot T, Errard J, Fabbian G, Feng C, Gilbert A, Goeckner-Wald N, Halverson NW, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Hori Y, Inoue Y, Jaehnig GC, Jaffe AH, Katayama N, Keating B, Kermish Z, Keskitalo R, Kisner T, Le Jeune M, Lee AT, Leitch EM, Linder E, Matsuda F, Matsumura T, Meng X, Miller NJ, Morii H, Myers MJ, Navaroli M, Nishino H, Okamura T, Paar H, Peloton J, Poletti D, Raum C, Rebeiz G, Reichardt CL, Richards PL, Ross C, Rotermund KM, Schenck DE, Sherwin BD, Shirley I, Sholl M, Siritanasak P, Smecher G, Steinbach B, Stompor R, Suzuki A, Suzuki J, Takada S, Takakura S, Tomaru T, Wilson B, Yadav A, Zahn Oet al., 2014, The Simons Array: expanding POLARBEAR to three multi-chroic telescopes, Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, Publisher: SPIE-INT SOC OPTICAL ENGINEERING, ISSN: 0277-786X

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• Citations: 29

Inoue Y, Stebor N, Ade PAR, Akiba Y, Arnold K, Anthony AE, Atlas M, Barron D, Bender A, Boettger D, Borrill J, Chapman S, Chinone Y, Cukierman A, Dobbs M, Elleflot T, Errard J, Fabbian G, Feng C, Gilbert A, Halverson NW, Hasegawa M, Hattori K, Hazumi M, Holzapfel WL, Hori Y, Jaehnig GC, Jaffe AH, Katayama N, Keating B, Kermish Z, Keskitalo R, Kisner T, Le Jeune M, Lee AT, Leitc EM, Linder E, Matsuda F, Matsumura T, Meng X, Morii H, Myers MJ, Navaroli M, Nishino H, Okamura T, Paar H, Peloton J, Poletti D, Rebeiz G, Reichard CL, Richards PL, Ross C, Schenck DE, Sherwin BD, Siritanasak P, Smecher G, Sholl M, Steinbach B, Stompor R, Suzuki A, Suzukim J, Takada S, Takakura S, Tomaru T, Wilson B, Yadav A, Yamaguchi H, Zahn Oet al., 2014, Thermal and optical characterization for POLARBEAR-2 optical cryostat, Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, Publisher: SPIE-INT SOC OPTICAL ENGINEERING, ISSN: 0277-786X

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• Citations: 3

Jaffe A, 2013, Physics: The time lord and fellow travellers, Nature, Vol: 502, Pages: 620-622, ISSN: 0028-0836

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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 (vol 550, A131, 2013), ASTRONOMY & ASTROPHYSICS, Vol: 558, ISSN: 0004-6361

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• Citations: 19