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William T. Reach
Researcher at Universities Space Research Association
Publications - 545
Citations - 95523
William T. Reach is an academic researcher from Universities Space Research Association. The author has contributed to research in topics: Galaxy & Interstellar medium. The author has an hindex of 131, co-authored 535 publications receiving 90496 citations. Previous affiliations of William T. Reach include California Institute of Technology & Space Telescope Science Institute.
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Journal ArticleDOI
Planck early results. XXIII. The first all-sky survey of Galactic cold clumps
Peter A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,Amedeo Balbi,A. J. Banday,A. J. Banday,R. B. Barreiro,James G. Bartlett,James G. Bartlett,E. Battaner,Karim Benabed,Alain Benoit,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,R. Bhatia,J. J. Bock,Anna Bonaldi,J. R. Bond,Julian Borrill,Julian Borrill,F. R. Bouchet,F. Boulanger,M. Bucher,Carlo Burigana,Paolo Cabella,Christopher Cantalupo,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,L. Cayón,Anthony Challinor,A. Chamballu,R.-R. Chary,Lung-Yih Chiang,P. R. Christensen,David L. Clements,Stéphane Colombi,F. Couchot,A. Coulais,B. P. Crill,F. Cuttaia,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,G. de Gasperis,A. de Rosa,G. de Zotti,G. de Zotti,Jacques Delabrouille,J.-M. Delouis,F.-X. Désert,Clive Dickinson,Kazuhito Dobashi,S. Donzelli,S. Donzelli,Olivier Doré,U. Dörl,Marian Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,E. Falgarone,Fabio Finelli,Olivier Forni,M. Frailis,E. Franceschi,S. Galeotta,Ken Ganga,Ken Ganga,M. Giard,G. Giardino,Y. Giraud-Héraud,J. González-Nuevo,K. M. Górski,K. M. Górski,Serge Gratton,A. Gregorio,Alessandro Gruppuso,F. K. Hansen,D. L. Harrison,George Helou,Sophie Henrot-Versille,D. Herranz,S. R. Hildebrandt,S. R. Hildebrandt,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,W. Hovest,Roger J. Hoyland,Kevin M. Huffenberger,Andrew H. Jaffe,Gilles Joncas,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Reijo Keskitalo,Theodore Kisner,R. Kneissl,R. Kneissl,Lloyd Knox,Hannu Kurki-Suonio,Guilaine Lagache,J.-M. Lamarre,Anthony Lasenby,René J. Laureijs,Charles R. Lawrence,S. Leach,Rodrigo Leonardi,Rodrigo Leonardi,C. Leroy,C. Leroy,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,C. J. MacTavish,Bruno Maffei,Nazzareno Mandolesi,Robert G. Mann,Michele Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Gábor Marton,Silvia Masi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,P. M. McGehee,Alessandro Melchiorri,L. Mendes,A. Mennella,A. Mennella,Subhasish Mitra,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,Dipak Munshi,Anna Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,S. Osborne,F. Pajot,Roberta Paladini,Fabio Pasian,G. Patanchon,T. J. Pearson,V.-M. Pelkonen,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,M. Piat,Stéphane Plaszczynski,Etienne Pointecouteau,G. Polenta,G. Polenta,N. Ponthieu,T. Poutanen,T. Poutanen,T. Poutanen,G. Prézeau,Simon Prunet,Jean-Loup Puget,William T. Reach,Rafael Rebolo,Rafael Rebolo,Martin Reinecke,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,Graca Rocha,C. Rosset,Michael Rowan-Robinson,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,Giorgio Savini,Douglas Scott,M. D. Seiffert,George F. Smoot,George F. Smoot,George F. Smoot,Jean-Luc Starck,Jean-Luc Starck,F. Stivoli,V. Stolyarov,Rashmikant V. Sudiwala,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tomasi,J. P. Torre,V. Toth,Matthieu Tristram,Jussi Tuovinen,G. Umana,Luca Valenziano,P. Vielva,F. Villa,Nicola Vittorio,Lawrence A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Nathalie Ysard,D. Yvon,A. Zacchei,Sarolta Zahorecz,Andrea Zonca +234 more
TL;DR: The first version of the C3PO (Early Cold Core Catalogue of Planck Objects) is presented in this article, in terms of their spatial distribution, temperature, distance, mass, and morphology.
Journal ArticleDOI
The Dust Cloud around the White Dwarf G29-38
William T. Reach,Marc J. Kuchner,Ted von Hippel,Adam Burrows,Fergal Mullally,Mukremin Kilic,Donald E Winget +6 more
TL;DR: In this paper, the spectral energy distribution (SED) of the white dwarf G29-38 has a continuum peak around 4.5 μm and a 9-11 μm emission feature 1.25 times brighter than the continuum.
Journal ArticleDOI
Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE). IV. Dust Properties in the Interstellar Medium
Jean Philippe Bernard,William T. Reach,Deborah Paradis,Margaret Meixner,Roberta Paladini,Akiko Kawamura,Toshikazu Onishi,U. Vijh,Karl D. Gordon,Remy Indebetouw,Joseph L. Hora,Barbara A. Whitney,Robert Blum,Marilyn R. Meade,Brian Babler,Ed Churchwell,Charles W. Engelbracht,B. Q. For,Karl Misselt,Claus Leitherer,Martin Cohen,Francois Boulanger,Jay A. Frogel,Yasuo Fukui,Jay Gallagher,Varoujan Gorjian,Jason Harris,Douglas M. Kelly,William B. Latter,Suzanne C. Madden,Ciska Markwick-Kemper,Akira Mizuno,Norikazu Mizuno,Jeremy Mould,Antonella Nota,M. S. Oey,Knut Olsen,Nino Panagia,Pablo G. Pérez-González,Hiroshi Shibai,Shuji Sato,Linda J. Smith,Lister Staveley-Smith,Alexander G. G. M. Tielens,Toshiya Ueta,Schuyler D. Van Dyk,Kevin Volk,Michael W. Werner,Dennis Zaritsky +48 more
TL;DR: In this paper, a preliminary analysis of the extended infrared (IR) emission by dust in the interstellar medium (ISM) of the Large Magellanic Cloud (LMC) is presented.
Journal ArticleDOI
Planck 2013 results. XIII. Galactic CO emission
Peter A. R. Ade,Nabila Aghanim,M. I. R. Alves,C. Armitage-Caplan,Monique Arnaud,M. Ashdown,Fernando Atrio-Barandela,J. Aumont,C. Baccigaluppi,A. J. Banday,R. B. Barreiro,James G. Bartlett,E. Battaner,K. Benabed,Alain Benoit,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,Jérôme Bobin,James J. Bock,Anna Bonaldi,J. R. Bond,Julian Borrill,François R. Bouchet,F. Boulanger,M. Bridges,M. Bucher,Carlo Burigana,R. C. Butler,Jean-François Cardoso,A. Catalano,A. Chamballu,Ranga-Ram Chary,Xun Chen,Lung-Yih Chiang,H. C. Chiang,P. R. Christensen,Sarah E. Church,David L. Clements,S. Colombi,L. P. L. Colombo,C. Combet,F. Couchot,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,Luigi Danese,R. D. Davies,P. de Bernardis,A. de Rosa,G. de Zotti,Jacques Delabrouille,J.-M. Delouis,Jessica Dempsey,F.-X. Désert,Clive Dickinson,Jose M. Diego,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,X. Dupac,George Efstathiou,T. A. Enblin,H. K. Eriksen,E. Falgarone,Fabio Finelli,Olivier Forni,M. Frailis,E. Franceschi,Yasuo Fukui,S. Galeotta,K. Ganga,M. Giard,Y. Giraud-Héraud,J. González-Nuevo,Krzysztof M. Gorski,Serge Gratton,A. Gregorio,Alessandro Gruppuso,Toshihiro Handa,F. K. Hansen,Duncan Hanson,D. L. Harrison,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,P. Hily-Blant,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,T. R. Jaffe,Andrew H. Jaffe,J. Jewell,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Theodore Kisner,J. Knoche,Lloyd Knox,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,R. J. Laureijs,Charles R. Lawrence,R. Leonardi,J. León-Tavares,J. Lesgourgues,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,N. Mandolesi,M. Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,Peregrine McGehee,Alessandro Melchiorri,L. Mendes,A. Mennella,M. Migliaccio,Subhabrata Mitra,M.-A. Miville-Deschênes,A. Moneti,L. Montier,Toby J. T. Moore,Gianluca Morgante,Jun-Ichi Morino,Daniel J. Mortlock,Dipak Munshi,Taku Nakajima,Pavel Naselsky,Federico Nati,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,Takio Okuda,S. Osborne,Carol Anne Oxborrow,F. Paci,L. Pagano,F. Pajot,R. Paladini,Daniela Paoletti,F. Pasian,G. Patanchon,O. Perdereau,L. Perotto,F. Perrotta,F. Piacentini,M. Piat,E. Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,G. Polenta,N. Ponthieu,L. Popa,T. Poutanen,G. W. Pratt,G. Preezeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,William T. Reach,Rafael Rebolo,M. Reinecke,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,M. Rowan-Robinson,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,Giorgio Savini,Douglas Scott,Michael Seiffert,E. P. S. Shellard,Locke D. Spencer,Jean-Luc Starck,V. Stolyarov,R. Stompor,R. Sudiwala,R. A. Sunyaev,F. Sureau,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,D. Tavagnacco,Luca Terenzi,H. Thomas,L. Toffolatti,M. Tomasi,Kazufumi Torii,M. Tristram,M. Tucci,J. Tuovinen,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,B. Van Tent,P. Vielva,Fabrizio Villa,Nicola Vittorio,L. A. Wade,Benjamin D. Wandelt,Ingunn Kathrine Wehus,H. Yamamoto T. Yoda,D. Yvon,Andrea Zacchei,Andrea Zonca +239 more
TL;DR: In this article, the velocity-integrated CO emission maps for the (1-0), (2-1), and (3-2) rotational transitions with low foreground contamination but moderate signal-to-noise ratio were extracted from Planck HFI data.
Journal ArticleDOI
Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance
Peter A. R. Ade,Nabila Aghanim,R. Ansari,M. Arnaud,M. Ashdown,J. Aumont,A. J. Banday,A. J. Banday,A. J. Banday,Matthias Bartelmann,Matthias Bartelmann,James G. Bartlett,James G. Bartlett,E. Battaner,Karim Benabed,Alain Benoit,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,R. Bhatia,J. J. Bock,J. R. Bond,Julian Borrill,Julian Borrill,F. R. Bouchet,F. Boulanger,Tom Bradshaw,E. Bréelle,M. Bucher,Philippe Camus,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,Anthony Challinor,A. Chamballu,J. Charra,M. Charra,R.-R. Chary,C. Chiang,Sarah E. Church,David L. Clements,Stéphane Colombi,F. Couchot,A. Coulais,C. Cressiot,B. P. Crill,Martin Crook,P. de Bernardis,Jacques Delabrouille,J.-M. Delouis,F.-X. Désert,Klaus Dolag,Herve Dole,Olivier Doré,Marian Douspis,George Efstathiou,P. Eng,C. Filliard,Olivier Forni,Olivier Forni,Pablo Fosalba,J. J. Fourmond,Ken Ganga,Ken Ganga,M. Giard,M. Giard,D. Girard,Y. Giraud-Héraud,R. Gispert,K. M. Górski,K. M. Górski,Serge Gratton,Matthew Joseph Griffin,G. Guyot,J. Haissinski,D. L. Harrison,George Helou,Sophie Henrot-Versille,C. Hernández-Monteagudo,S. R. Hildebrandt,S. R. Hildebrandt,S. R. Hildebrandt,Richard Hills,E. Hivon,Michael P. Hobson,W. A. Holmes,Kevin M. Huffenberger,Andrew H. Jaffe,W. C. Jones,Jean Kaplan,R. Kneissl,R. Kneissl,Lloyd Knox,Guilaine Lagache,J.-M. Lamarre,P. Lami,Andrew E. Lange,Anthony Lasenby,A. Lavabre,Charles R. Lawrence,B. Leriche,C. Leroy,C. Leroy,C. Leroy,Y. Longval,J. F. Macías-Pérez,Thierry Maciaszek,C. J. MacTavish,Bruno Maffei,Nazzareno Mandolesi,Robert G. Mann,B. Mansoux,Silvia Masi,Tomotake Matsumura,P. M. McGehee,Jean-Baptiste Melin,C. Mercier,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Daniel J. Mortlock,Anna Murphy,Federico Nati,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,C. North,F. Noviello,Dmitry Novikov,S. Osborne,Christopher G. Paine,F. Pajot,G. Patanchon,T. Peacocke,T. J. Pearson,O. Perdereau,L. Perotto,F. Piacentini,M. Piat,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,R. Pons,R. Pons,N. Ponthieu,G. Prézeau,Simon Prunet,Jean-Loup Puget,William T. Reach,C. Renault,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,Michael Rowan-Robinson,Ben Rusholme,D. Santos,Giorgio Savini,B. M. Schaefer,P. Shellard,Locke D. Spencer,Jean-Luc Starck,Jean-Luc Starck,P. Stassi,V. Stolyarov,Radek Stompor,Rashmikant V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,J.-F. Sygnet,J. A. Tauber,Clemens Thum,J. P. Torre,F. Touze,Matthieu Tristram,F. van Leeuwen,L. Vibert,D. Vibert,Lawrence A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Simon D. M. White,Helmut Wiesemeyer,Adam Woodcraft,V. Yurchenko,D. Yvon,A. Zacchei +191 more
TL;DR: 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 wide bands at an angular resolution of 10' (100 GHz), 7' (143 GHz), and 5' (217 GHz) as mentioned in this paper.