M
Massimo Marengo
Researcher at Iowa State University
Publications - 233
Citations - 14103
Massimo Marengo is an academic researcher from Iowa State University. The author has contributed to research in topics: Stars & Spitzer Space Telescope. The author has an hindex of 52, co-authored 228 publications receiving 13242 citations. Previous affiliations of Massimo Marengo include University of Arizona & International School for Advanced Studies.
Papers
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Journal ArticleDOI
A Spitzer IRAC Imaging Survey for T Dwarf Companions Around M, L, and T Dwarfs: Observations, Results, and Monte Carlo Population Analyses
Joseph C. Carson,Massimo Marengo,Brian M. Patten,Kevin Luhman,Sarah Sonnett,Joseph L. Hora,M. T. Schuster,M. T. Schuster,P. R. Allen,Giovanni G. Fazio,John R. Stauffer,Carolin Schnupp +11 more
TL;DR: In this paper, a two-epoch survey achieved typical detection sensitivities to substellar companions of [4.5 μm] ≤ 17.2mag for angular separations between about 7'' and 165''.
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Resolving the Dusty Circumstellar Structure of the Enigmatic Symbiotic Star CH Cygni with the MMT Adaptive Optics System
Beth Biller,Laird M. Close,Aigen Li,Massimo Marengo,John H. Bieging,Phil Hinz,William F. Hoffmann,Guido Brusa,Doug Miller +8 more
TL;DR: In this article, the symbiotic star CH Cyg and two PSF calibration stars were imaged using the unique 6.5 m MMT deformable secondary adaptive optics system.
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A thin shell of ionized gas as the explanation for infrared excess among classical Cepheids
V. Hocdé,Nicolas Nardetto,Eric Lagadec,G. Niccolini,A. Domiciano de Souza,Antoine Mérand,Pierre Kervella,Alexandre Gallenne,Alexandre Gallenne,Massimo Marengo,B. Trahin,Wolfgang Gieren,Grzegorz Pietrzyński,S. Borgniet,L. Breuval,Behnam Javanmardi +15 more
TL;DR: In this paper, the spectral energy distribution (SED) of five Cepheids: RS Pup (P = 41.46d), ζ Gem, η Aql, V Cen, and SU Cyg was analyzed using the SPIPS algorithm.
The Dust and Gas Around Beta Pictoris
Christine Chen,Aigen Li,C. J. Bohac,K. H. Kim,Dan M. Watson,J. van Cleve,James R. Houck,K. Stapelfeldt,Michael Werner,George H. Rieke,Kate Y. L. Su,Massimo Marengo,D. E. Backman,Chas Beichman,Giovanni G. Fazio +14 more
TL;DR: In this paper, the authors obtained Spitzer IRS 5.5 - 35 micron spectroscopy of the debris disk around beta Pictoris and detected the crystalline silicate emission bands at 28 micron and 33.5 micron.
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