Kate Gudrun Isaak
European Space Research and Technology Centre
159 Papers
1.3K Citations
Kate Gudrun Isaak is an academic researcher from European Space Research and Technology Centre. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 48, co-authored 110 publications. Previous affiliations of Kate Gudrun Isaak include European Space Agency & Cardiff University.
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Papers
In-flight calibration of the Herschel-SPIRE instrument
B. M. Swinyard,Peter A. R. Ade,Jean-Paul Baluteau,Herve Aussel,M. J. Barlow,George J. Bendo,Dominique Benielli,James J. Bock,Drew Brisbin,A. Conley,L. Conversi,A. Dowell,Darren Dowell,Marc Ferlet,T. Fulton,Jason Glenn,Adrian M. Glauser,Adrian M. Glauser,Douglas Griffin,Matthew Joseph Griffin,S. Guest,P. Imhof,Kate Gudrun Isaak,S. C. Jones,K. J. King,S. J. Leeks,L. R. Levenson,T. L. Lim,Nanyao Y. Lu,Gibion Makiwa,David A. Naylor,Hien Nguyen,Seb Oliver,Pasquale Panuzzo,Andreas Papageorgiou,C. P. Pearson,C. P. Pearson,Michael Pohlen,Edward Polehampton,Edward Polehampton,D. Pouliquen,Dimitra Rigopoulou,Dimitra Rigopoulou,S. Ronayette,Helene Roussel,A. Rykala,Giorgio Savini,Bernhard Schulz,Arnold A. Schwartz,David L. Shupe,Bruce Sibthorpe,S. D. Sidher,Anthony J. Smith,Locke D. Spencer,Markos Trichas,H. Triou,Ivan Valtchanov,Roger Wesson,Adam Woodcraft,C. K. Xu,Michael Zemcov,L. Zhang +61 more
TL;DR: In this article, the authors present the photometric, spectroscopic and spatial accuracy of the SPIRE system using a combination of the emission from the Herschel telescope itself and the modelled continuum emission from solar system objects and other astronomical targets.
The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift
D. Brisbin,Martin Harwit,Bruno Altieri,A. Amblard,V. Arumugam,Herve Aussel,T. Babbedge,Andrew Blain,James J. Bock,James J. Bock,Alessandro Boselli,V. Buat,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,Antonio Cava,Pierre Chanial,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Eli Dwek,Stephen Anthony Eales,David Elbaz,M. Fox,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,Matthew Joseph Griffin,Mark Halpern,Evanthia Hatziminaoglou,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,L. R. Levenson,L. R. Levenson,Carol J. Lonsdale,Nanyao Y. Lu,Suzanne C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,Glenn Morrison,Hien Nguyen,Hien Nguyen,B. O'Halloran,Seb Oliver,Alain Omont,Frazer N. Owen,Maurilio Pannella,P. Panuzzo,Andreas Papageorgiou,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,D. Rizzo,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Nick Seymour,David L. Shupe,A. J. Smith,Jamie Stevens,Veronica Strazzullo,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,L. Vigroux,Lian-Tao Wang,Robyn L. Ward,Gillian S. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +83 more
- 21 Nov 2010
TL;DR: In this article, the authors report observations of the IR/SMM emission from the Lockman North field and the Great Observatories Origins Deep Survey Field-North (GOSF-North).
HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements
Asantha Cooray,Asantha Cooray,A. Amblard,Lian-Tao Wang,V. Arumugam,Robbie Richard Auld,Herve Aussel,Tom Babbedge,Andrew Blain,J. J. Bock,J. J. Bock,Alessandro Boselli,V. Buat,Denis Burgarella,N. Castro-Rodriguez,Antonio Cava,Pierre Chanial,David L. Clements,A. Conley,L. Conversi,C. D. Dowell,C. D. Dowell,Eli Dwek,Stephen Anthony Eales,D. Elbaz,Duncan Farrah,M. Fox,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,Matthew Joseph Griffin,Mark Halpern,Evanthia Hatziminaoglou,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Ali Ahmad Khostovan,Guilaine Lagache,L. R. Levenson,L. R. Levenson,Nanyao Y. Lu,Suzanne C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,G. Marsden,K. Mitchell-Wynne,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,S. J. Oliver,Alain Omont,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,Chris Pearson,I. Perez Fournon,Michael Pohlen,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,D. Rizzo,Isaac Roseboom,Michael Rowan-Robinson,Benjamin L. Schulz,Douglas Scott,Paolo Serra,Nick Seymour,David L. Shupe,A. J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,L. Vigroux,Robyn L. Ward,Gillian S. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +86 more
TL;DR: In this paper, the authors measured the angular correlation function, w(theta), from 0.5 to 30 arcminutes of detected sources in two wide fields of the Herschel Multi-tiered Extragalactic Survey (HerMES).
Detailed cool star flare morphology with CHEOPS and TESS
G. Bruno,Isabella Pagano,Gaetano Scandariato,H. G. Floren,Alexis Brandeker,G. Olofsson,P. Maxted,Andrea Fortier,S. Sousa,Sophia Sulis,Valérie Van Grootel,Z. Garai,Á. Boldog,L. Kriskovics,M. G. Szabó,D. Gandolfi,Y. Alibert,R Alonso,T. Bárczy,D. Barrado Navascues,S. C. C. Barros,W. Baumjohann,M. Beck,Thomas Boeck,W. Benz,N. Billot,Luca Borsato,C. Broeg,A. Collier Cameron,Sz. Csizmadia,P. E. Cubillos,M. B. Davies,Magali Deleuil,A. Deline,Laetitia Delrez,Olivier Demangeon,Brice-Olivier Demory,David Ehrenreich,Alex Erikson,J. Farinato,Luciano Fossati,M. Fridlund,M. Gillon,M. Güdel,M. N. Günther,A. Heitzmann,Ch. Helling,Sergio Hoyer,Kate Gudrun Isaak,L. Kiss,K. W. F. Lam,J. Laskar,A. Lecavelier des Etangs,Monika Lendl,D. Magrin,C. Mordasini,Valerio Nascimbeni,Roland Ottensamer,E. Pallé,Gao Peter,G. Piotto,D. Pollacco,D. Queloz,Roberto Ragazzoni,Nicola Rando,F. Ratti,Heike Rauer,I. Ribas,M. Sarajlic,Damien Ségransan,A. E. Simon,V. Singh,A.M.S. Smith,M. Stalport,Nicolas Thomas,S. Udry,B. Ulmer,J. Venturini,E. Villaver,N. A. Walton,T. G. Wilson +80 more
- 24 Mar 2024
TL;DR: High-cadence observations of stellar flares with CHEOPS and TESS reveal complex flare morphology and provide constraints on flare parameter distributions.
The central region of spiral galaxies as seen by Herschel - M 81, M 99, and M 100
Marc Sauvage,N. Sacchi,George J. Bendo,Alessandro Boselli,Michael Pohlen,Christine D. Wilson,Robbie Richard Auld,Maarten Baes,M. J. Barlow,J. J. Bock,M. Bradford,V. Buat,N. Castro-Rodriguez,P. Chanial,Stéphane Charlot,Laure Ciesla,David L. Clements,Asantha Cooray,Diane Cormier,Luca Cortese,Jonathan Ivor Davies,Eli Dwek,Stephen Anthony Eales,D. Elbaz,Maud Galametz,Frédéric Galliano,Walter Kieran Gear,Jason Glenn,Haley Louise Gomez,Matthew Joseph Griffin,Sacha Hony,Kate Gudrun Isaak,Kate Gudrun Isaak,Louis Levenson,Nanyao Y. Lu,Suzanne C. Madden,B. O'Halloran,K. Okumura,Seb Oliver,Mat Page,P. Panuzzo,Andreas Papageorgiou,T. J. Parkin,Ismael Perez-Fournon,Naseem Rangwala,E. E. Rigby,Helene Roussel,A. Rykala,Benjamin L. Schulz,Maximilien R. P. Schirm,Matthew Smith,L. Spinoglio,Jamie Stevens,Sundar Srinivasan,M. Symeonidis,Markos Trichas,Mattia Vaccari,L. Vigroux,Herve Wozniak,Gillian S. Wright,Werner W. Zeilinger +60 more
TL;DR: In this article, the authors quantify the luminosity of the central component by both a decomposition of the radial surface brightness profile and a direct extraction in 2D, and find that the relative contribution is variable within the three galaxies in their sample, possibly connected more directly to the presence of a bar than to the morphological type.