J
Jingwen Wu
Researcher at Chinese Academy of Sciences
Publications - 129
Citations - 5656
Jingwen Wu is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 35, co-authored 109 publications receiving 5139 citations. Previous affiliations of Jingwen Wu include University of Texas at Austin & CFA Institute.
Papers
More filters
Journal ArticleDOI
Mid-Infrared Selection of Active Galactic Nuclei with the Wide-Field Infrared Survey Explorer. II. Properties of WISE-Selected Active Galactic Nuclei in the NDWFS Boötes Field
Roberto J. Assef,Daniel Stern,Christopher S. Kochanek,Andrew Blain,Mark Brodwin,Michael J. I. Brown,Emilio Donoso,Peter Eisenhardt,Buell T. Jannuzi,Thomas H. Jarrett,Thomas H. Jarrett,S. A. Stanford,S. A. Stanford,C. W. Tsai,Jingwen Wu,Lin Yan +15 more
TL;DR: In this paper, the authors presented a study of WISE selection of AGN in the 2 deg 2 COSMOS field, finding that a simple criterion W1-W2�0.8 provides a highly reliable and complete AGN sample for W2<15.05, where the W1 and W2 passbands are centered at 3.4µm and 4.6µmm, respectively.
Journal ArticleDOI
Connecting Dense Gas Tracers of Star Formation in our Galaxy to High-z Star Formation
TL;DR: This paper showed that the global star formation rate, as indicated by the infrared luminosity, has a tight and almost linear correlation with the amount of dense gas as traced by the luminosity of HCN.
Journal ArticleDOI
Mid-Infrared Selection of Active Galactic Nuclei with the Wide-Field Infrared Survey Explorer. II. Properties of WISE-Selected Active Galactic Nuclei in the NDWFS Bo\"otes Field
Roberto J. Assef,Daniel Stern,Christopher S. Kochanek,Andrew Blain,Mark Brodwin,Michael J. I. Brown,Emilio Donoso,Peter Eisenhardt,Buell T. Jannuzi,Thomas H. Jarrett,S. Adam Stanford,Chao-Wei Tsai,Jingwen Wu,Lin Yan +13 more
TL;DR: In this article, a modified color-magnitude cut was proposed to combine the W1-W2 color and the W2 magnitude to provide highly reliable or highly complete AGN samples for fainter WISE sources.
Journal ArticleDOI
The Properties of Massive, Dense Clumps: Mapping Surveys of HCN and CS
TL;DR: In this paper, the authors have mapped over 50 massive, dense clumps with four dense gas tracers: HCN J = 1-0 and 3-2; and CS J = 2-1 and 7-6 transitions.
Journal ArticleDOI
Simultaneous Planck, Swift, and Fermi observations of X-ray and γ-ray selected blazars
Paolo Giommi,G. Polenta,G. Polenta,Anne Lähteenmäki,Anne Lähteenmäki,D. J. Thompson,M. Capalbi,S. Cutini,Dario Gasparrini,J. González-Nuevo,Jonathan León-Tavares,M. López-Caniego,Mn Mazziotta,C. Monte,C. Monte,M. Perri,S. Rainò,S. Rainò,G. Tosti,G. Tosti,Andrea Tramacere,F. Verrecchia,Hugh D. Aller,M. F. Aller,E. Angelakis,Denis Bastieri,Denis Bastieri,Andrei Berdyugin,Anna Bonaldi,Laura Bonavera,Laura Bonavera,Carlo Burigana,David N. Burrows,S. Buson,E. Cavazzuti,G. Chincarini,Sergio Colafrancesco,L. Costamante,F. Cuttaia,Filippo D'Ammando,G. de Zotti,G. de Zotti,M. Frailis,Lars Fuhrmann,S. Galeotta,F. Gargano,N. Gehrels,Nicola Giglietto,Nicola Giglietto,Francesco Giordano,Marcello Giroletti,E. Keihänen,O. King,Thomas P. Krichbaum,Anthony Lasenby,N. Lavonen,Charles R. Lawrence,C. Leto,Elina Lindfors,Nazzareno Mandolesi,Marcella Massardi,Walter Max-Moerbeck,Peter F. Michelson,M. G. Mingaliev,Paolo Natoli,Paolo Natoli,Paolo Natoli,I. Nestoras,E. Nieppola,E. Nieppola,Kari Nilsson,B. Partridge,Vasiliki Pavlidou,T. J. Pearson,Pietro Procopio,Jörg P. Rachen,Anthony C. S. Readhead,R. Reeves,A. Reimer,R. Reinthal,S. Ricciardi,Joseph L. Richards,D. Riquelme,Jari Saarinen,Anna Sajina,M. Sandri,P. Savolainen,A. Sievers,A. Sillanpää,Yu. V. Sotnikova,Mark Stevenson,G. Tagliaferri,L. O. Takalo,Joni Tammi,D. Tavagnacco,Luca Terenzi,L. Toffolatti,Merja Tornikoski,Corrado Trigilio,M. Turunen,G. Umana,H. Ungerechts,F. Villa,Jingwen Wu,Andrea Zacchei,J. A. Zensus,Xu Zhou +106 more
TL;DR: In this paper, simultaneous Planck, Swift, Fermi, and ground-based data for 105 blazars belonging to three samples with flux limits in the soft X-ray, hard Xray, and gamma-ray bands, with additional 5 GHz flux-density limits to ensure a good probability of a Planck detection.