J
J. A. Murphy
Researcher at Maynooth University
Publications - 244
Citations - 45569
J. A. Murphy is an academic researcher from Maynooth University. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 87, co-authored 238 publications receiving 42760 citations. Previous affiliations of J. A. Murphy include National University of Ireland.
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Journal ArticleDOI
Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates
Peter A. R. Ade,Nabila Aghanim,M. Arnaud,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,N. Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,F. R. Bouchet,F. Boulanger,Carlo Burigana,R. C. Butler,Erminia Calabrese,A. Catalano,H. C. Chiang,P. R. Christensen,D. L. Clements,L. P. L. Colombo,F. Couchot,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,Jacques Delabrouille,Clive Dickinson,Jose M. Diego,H. Dole,Olivier Doré,M. Douspis,A. Ducout,X. Dupac,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,Fabio Finelli,I. Flores-Cacho,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Galeotta,Silvia Galli,K. Ganga,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,Krzysztof M. Gorski,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,F. K. Hansen,D. L. Harrison,George Helou,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,E. Keihänen,Reijo Keskitalo,Theodore Kisner,J. Knoche,Martin Kunz,Hannu Kurki-Suonio,G. Lagache,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,François Levrier,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Gianmarco Maggio,Davide Maino,Nazzareno Mandolesi,Anna Mangilli,Michele Maris,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Alessandro Melchiorri,A. Mennella,M. Migliaccio,S. Mitra,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Federico Nati,Paolo Natoli,Nicole P. H. Nesvadba,F. Noviello,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,B. Partridge,Fabio Pasian,T. J. Pearson,O. Perdereau,L. Perotto,Valeria Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,M. Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,Graca Rocha,C. Rosset,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,Locke D. Spencer,V. Stolyarov,R. Stompor,R. V. Sudiwala,R. A. Sunyaev,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,M. Turler,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,B. Van Tent,P. Vielva,Fabrizio Villa,Lawrence A. Wade,B. D. Wandelt,Ingunn Kathrine Wehus,Niraj Welikala,D. Yvon,Andrea Zacchei,Andrea Zonca +187 more
TL;DR: In this article, a combination of Planck and IRAS data was used to select the most luminous cold submm sources with spectral energy distributions peaking between 353 and 857GHz at 5' resolution.
Journal ArticleDOI
Planck intermediate results. XLIII. The spectral energy distribution of dust in clusters of galaxies
R. Adam,P. A. R. Ade,Nabila Aghanim,M. Ashdown,Jonathan Aumont,C. Baccigalupi,R. B. Barreiro,Nicola Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,M. Bersanelli,P. Bielewicz,I. F. Bikmaev,Anna Bonaldi,J. R. Bond,J. Borrill,F. R. Bouchet,R. A. Burenin,Carlo Burigana,E. Calabrese,J.-F. Cardoso,A. Catalano,H. C. Chiang,P. R. Christensen,E. M. Churazov,L. P. L. Colombo,C. Combet,B. Comis,F. Couchot,B. P. Crill,A. Curto,F. Cuttaia,L. Danese,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,J. Delabrouille,F.-X. Désert,Jose M. Diego,H. Dole,O. Doré,M. Douspis,A. Ducout,X. Dupac,F. Elsner,Torsten A. Enßlin,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Galeotta,K. Ganga,Ricardo Génova-Santos,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,F. K. Hansen,D. L. Harrison,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,Allan Hornstrup,W. Hovest,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,E. Keihänen,R. Keskitalo,I. M. Khamitov,Theodore Kisner,R. Kneissl,J. Knoche,M. Kunz,Hannu Kurki-Suonio,G. Lagache,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,J. F. Macías-Pérez,Bruno Maffei,Gianmarco Maggio,Nazzareno Mandolesi,Anna Mangilli,Michele Maris,Pierrick Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Alessandro Melchiorri,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel D. Naselsky,Federico Nati,P. Natoli,Hans Ulrik Nørgaard-Nielsen,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,D. Paoletti,Fabio Pasian,O. Perdereau,L. Perotto,V. Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,N. Ponthieu,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,G. Rocha,C. Rosset,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,B. Rusholme,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,V. Stolyarov,R. Stompor,R. V. Sudiwala,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,Luca Valenziano,J. Valiviita,F. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,I. K. Wehus,D. Yvon,A. Zacchei,A. Zonca +178 more
TL;DR: In this paper, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.
Journal ArticleDOI
Small Angular Scale Measurements of the CMB Temperature Power Spectrum from QUaD
R. B. Friedman,P. A. R. Ade,J. J. Bock,M. Bowden,Michael L. Brown,G. Cahill,P. G. Castro,Sarah E. Church,T. Culverhouse,K. Ganga,Walter Kieran Gear,S. Gupta,J. Hinderks,John M Kovac,Andrew E. Lange,E. M. Leitch,S. Melhuish,Y. Memari,J. A. Murphy,Angelo Orlando,C. O' Sullivan,Lucio Piccirillo,C. Pryke,N. Rajguru,Ben Rusholme,R. Schwarz,Andy Taylor,K. L. Thompson,A. H. Turner,E. Y. S. Wu,Michael Zemcov +30 more
TL;DR: In this paper, the authors estimate the contribution of residual (unmasked) radio point sources using a model calibrated to their own bright source observations, and a full simulation of the source finding and masking procedure.
Journal ArticleDOI
Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck
Peter A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,J. Aumont,C. Baccigalupi,A. J. Banday,R. B. Barreiro,Nicola Bartolo,E. Battaner,Richard A. Battye,K. Benabed,George J. Bendo,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,Anna Bonaldi,Laura Bonavera,J. R. Bond,J. Borrill,F. R. Bouchet,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,A. Catalano,A. Chamballu,R.-R. Chary,Xin Chen,H. C. Chiang,P. R. Christensen,D. L. Clements,L. P. L. Colombo,C. Combet,F. Couchot,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,J. Delabrouille,Clive Dickinson,Jose M. Diego,H. Dole,S. Donzelli,O. Doré,M. Douspis,A. Ducout,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,K. Ganga,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,K. M. Górski,A. Gregorio,Alessandro Gruppuso,F. K. Hansen,D. Hanson,D. L. Harrison,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,Frank P. Israel,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,R. Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,M. Kunz,Hannu Kurki-Suonio,G. Lagache,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,S. C. Madden,Bruno Maffei,Davide Maino,Nazzareno Mandolesi,Michele Maris,Pierrick Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Pasquale Mazzotta,L. Mendes,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,P. Natoli,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,R. Paladini,D. Paoletti,Bruce Partridge,Fabio Pasian,T. J. Pearson,Michael W. Peel,O. Perdereau,F. Perrotta,V. Pettorino,F. Piacentini,M. Piat,Elena Pierpaoli,D. Pietrobon,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,L. Popa,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Martin Reinecke,Mathieu Remazeilles,C. Renault,S. Ricciardi,I. Ristorcelli,G. Rocha,C. Rosset,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,Giorgio Savini,Douglas Scott,Locke D. Spencer,V. Stolyarov,R. V. Sudiwala,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,G. Umana,Luca Valenziano,J. Valiviita,B. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,B. D. Wandelt,Robert A. Watson,Ingunn Kathrine Wehus,D. Yvon,A. Zacchei,A. Zonca +203 more
TL;DR: In this paper, the authors examined the morphology of the Andromeda galaxy's outermost spiral arms and investigated the dust heating mechanism across M31, finding that dust dominating the longer wavelength emission is heated by the diffuse stellar population.
Journal ArticleDOI
Planck Intermediate Results. XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes in the Canary Islands Observatories
P. A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,Jonathan Aumont,C. Baccigalupi,A. J. Banday,R. B. Barreiro,R. Barrena,Nicola Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,J.-P. Bernard,M. Bersanelli,P. Bielewicz,I. F. Bikmaev,Hans Böhringer,Anna Bonaldi,Laura Bonavera,J. R. Bond,J. Borrill,F. R. Bouchet,R. A. Burenin,Carlo Burigana,E. Calabrese,Jean-François Cardoso,A. Catalano,A. Chamballu,R.-R. Chary,H. C. Chiang,G. Chon,P. R. Christensen,D. L. Clements,L. P. L. Colombo,C. Combet,B. Comis,B. P. Crill,A. Curto,F. Cuttaia,Håkon Dahle,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,J. Delabrouille,Jose M. Diego,H. Dole,S. Donzelli,O. Doré,M. Douspis,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,A. Ferragamo,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Fromenteau,S. Galeotta,Silvia Galli,K. Ganga,Ricardo Génova-Santos,M. Giard,E. Gjerløw,J. González-Nuevo,K. M. Górski,A. Gruppuso,F. K. Hansen,D. L. Harrison,A. Hempel,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,T. R. Jaffe,E. Keihänen,R. Keskitalo,I. M. Khamitov,Theodore Kisner,J. Knoche,M. Kunz,Hannu Kurki-Suonio,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,J. Leon-Tavares,François Levrier,H. Lietzen,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Davide Maino,Nazzareno Mandolesi,Michele Maris,Pierrick Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Peregrine McGehee,Alessandro Melchiorri,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel D. Naselsky,Federico Nati,P. Natoli,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,D. Paoletti,Fabio Pasian,O. Perdereau,V. Pettorino,F. Piacentini,M. Piat,Elena Pierpaoli,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,G. Rocha,C. Rosset,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,B. Rusholme,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,V. Stolyarov,Alina Streblyanska,R. V. Sudiwala,R. A. Sunyaev,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,D. Tramonte,M. Tristram,M. Tucci,Luca Valenziano,J. Valiviita,B. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,B. D. Wandelt,Ingunn Kathrine Wehus,D. Yvon,A. Zacchei,A. Zonca +188 more
TL;DR: The results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with telescopes at the Canary Islands observatories as part of the general optical follow-up programme undertaken by the Planck collaboration are discussed in this paper.