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Nanyao Y. Lu
Researcher at California Institute of Technology
Publications - 90
Citations - 10692
Nanyao Y. Lu is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 44, co-authored 90 publications receiving 10248 citations. Previous affiliations of Nanyao Y. Lu include Jet Propulsion Laboratory.
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Journal ArticleDOI
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
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).
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A Minnesota Automated Plate Scanner Catalog of Galaxies Behind the Virgo Cluster and Toward its Antipode
TL;DR: A catalog of 1268 galxies, essentially complete to B(is less than or equal to)17.0, found by scanning glass copies of several fields of the original Palomar Sky Survey using the Minnesota Automated Plate Scanner in its isodensitometricmode as discussed by the authors.
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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 paper, 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.
Journal ArticleDOI
ALMA Observations of Warm Molecular Gas and Cold Dust in NGC 34
C. K. Xu,Chen Cao,Chen Cao,Nanyao Y. Lu,Yu Gao,P. van der Werf,Aaron S. Evans,Aaron S. Evans,Joseph M. Mazzarella,J. Chu,S. Haan,Tanio Díaz-Santos,Rowin Meijerink,Yinghe Zhao,Yinghe Zhao,P. N. Appleton,Lee Armus,Vassilis Charmandaris,S. D. Lord,Eric J. Murphy,David B. Sanders,Bernhard Schulz,S. Stierwalt,S. Stierwalt +23 more
TL;DR: In this paper, the CO (6-5) line emission was detected on the red-shifted wing of the line profile at the frequency of the (8-7) line, with an integrated flux of 17.7 \pm 2.1 (random) \ pm 2.7 (sysmatic)
Journal ArticleDOI
Radio Properties and Optical Identification of Two Samples of Millijansky Radio Sources at 1.4 GHz
TL;DR: In this paper, the radio, optical and near-IR properties of radio sources in the distant sample were compared with that of more powerful radio sources, and a comparison of primarily non-cluster radio sources from the nearby sample with a companion survey in a pair of rich superclusters at z * 0.1.