C
Carol J. Lonsdale
Researcher at National Radio Astronomy Observatory
Publications - 185
Citations - 20937
Carol J. Lonsdale is an academic researcher from National Radio Astronomy Observatory. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 63, co-authored 182 publications receiving 18841 citations. Previous affiliations of Carol J. Lonsdale include California Institute of Technology & Jet Propulsion Laboratory.
Papers
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Journal ArticleDOI
The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
S. Berta,Carol J. Lonsdale,Carol J. Lonsdale,Maria del Carmen Polletta,Maria del Carmen Polletta,Richard S. Savage,Alberto Franceschini,H. Buttery,Andrea Cimatti,J. E. Dias,Chiara Feruglio,Fabrizio Fiore,Enrico V. Held,F. La Franca,Roberto Maiolino,Alessandro Marconi,I. Matute,Seb Oliver,E. Ricciardelli,Stefano Rubele,N. Sacchi,David L. Shupe,Jason Surace +22 more
TL;DR: In this paper, the authors performed a systematic study of high-redshift massive galaxies, in order to determine the shape of the very-massive tail of the stellar mass function and determine the epoch of their assembly.
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IR and UV Galaxies at z = 0.6: Evolution of Dust Attenuation and Stellar Mass as Revealed by SWIRE and GALEX
C. Kevin Xu,David L. Shupe,Veronique Buat,Michael Rowan-Robinson,T. Babbedge,Jorge Iglesias-Páramo,Tsutomu T. Takeuchi,Tom A. Barlow,Tim Conrow,Fan Fang,Karl Forster,Peter G. Friedman,E. Gonzales-Solares,Carol J. Lonsdale,D. Christopher Martin,Patrick Morrissey,Susan G. Neff,David Schiminovich,Mark Seibert,Todd Small,Gene Smith,Jason Surace,Ted K. Wyder +22 more
TL;DR: In this paper, the authors studied dust attenuation and stellar mass of z = 0.6 star-forming galaxies using new SWIRE observations in IR and GALEX observations in UV.
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Spitzer Photometry of WISE-Selected Brown Dwarf and Hyper-Luminous Infrared Galaxy Candidates
Roger L. Griffith,J. Davy Kirkpatrick,Peter R. Eisenhardt,Christopher R. Gelino,Michael C. Cushing,Dominic J. Benford,Andrew Blain,Carrie Bridge,Martin Cohen,Roc M. Cutri,Emilio Donoso,Thomas Jarrett,Carol J. Lonsdale,Gregory N. Mace,A. K. Mainzer,Kenneth A. Marsh,Deborah Padgett,Sara Petty,Michael E. Ressler,Michael F. Skrutskie,S. A. Stanford,Daniel Stern,Chao-Wei Tsai,Edward L. Wright,Jingwen Wu,Lin Yan +25 more
TL;DR: In this article, the authors present a catalog of Spitzer photometry for all astrophysical sources identified in these fields and use this catalog to identify 7 fainter (4.5 $\mu$m 17.0 mag) brown dwarf candidates, which are possibly wide-field companions to the original WISE sources.
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VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2<z<2.1 selected from Spitzer IRAC 3.6 micron and 4.5 micron photometry
S. de la Torre,O. Le Fevre,Stephane Arnouts,Luigi Guzzo,Duncan Farrah,A. Iovino,Carol J. Lonsdale,B. Meneux,S. J. Oliver,A. Pollo,I. Waddington,D. Bottini,Fan Fang,B. Garilli,V. Le Brun,D. Maccagni,J. P. Picat,Roberto Scaramella,Marco Scodeggio,David L. Shupe,Jason Surace,L. Tresse,G. Vettolani,A. Zanichelli,C. Adami,S. Bardelli,M. Bolzonella,A. Cappi,Stéphane Charlot,Paolo Ciliegi,T. Contini,Sylvie Foucaud,P. Franzetti,I. Gavignaud,O. Ilbert,F. Lamareille,H. J. McCracken,Bruno Marano,Christian Marinoni,Alain Mazure,R. Merighi,S. Paltani,R. Pello,Lucia Pozzetti,Mario Radovich,G. Zamorani,E. Zucca,M. Bondi,Angela Bongiorno,Jarle Brinchmann,O. Cucciati,Yannick Mellier,Paola Merluzzi,S. Temporin,D. Vergani,C. J. Walcher +55 more
TL;DR: In this article, the authors used the projected two-point correlation function wp(rp) to study the three dimensional clustering properties of galaxies detected at 3.6 and 4.5 microns with IRAC.
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Overdensities of SMGs around WISE-selected, ultraluminous, high-redshift AGNs
Suzy Jones,Andrew Blain,Roberto J. Assef,Peter Eisenhardt,Carol J. Lonsdale,James J. Condon,Duncan Farrah,Chao-Wei Tsai,Carrie Bridge,Jingwen Wu,Edward L. Wright,Thomas H. Jarrett +11 more
TL;DR: In this article, the authors investigate extremely luminous dusty galaxies in the environments around Wide-field Infrared Survey Explorer (WISE)-selected hot dust-obscured galaxies (Hot DOGs) and WISE/radio-selected active galactic nuclei (AGNs) at average redshifts of z = 2.7 and 1.7, respectively.