9 Papers
112 Citations
W. Mo is an academic researcher from Johns Hopkins University. The author has contributed to research in topics: Asteroid & Population. The author has an hindex of 4, co-authored 6 publications.
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Papers
Neowise observations of near-earth objects: preliminary results
Amy Mainzer,Tommy Grav,James M. Bauer,Joseph Masiero,Robert S. McMillan,Roc M. Cutri,Russell G. Walker,Edward L. Wright,Peter Eisenhardt,David J. Tholen,Timothy Spahr,Robert Jedicke,Larry Denneau,E. DeBaun,D. Elsbury,Thomas Gautier,S. Gomillion,E. Hand,W. Mo,J. A. Watkins,A. Wilkins,G. Bryngelson,A. Del Pino Molina,Shantanu Desai,M. Go'mez Camus,Sebastian L. Hidalgo,I. S. Konstantopoulos,Jeffrey A. Larsen,C. Maleszewski,M. A. Malkan,J. C. Mauduit,B. Mullan,Edward W. Olszewski,Janine Pforr,A. Saro,James V. Scotti,Lawrence H. Wasserman +36 more
TL;DR: In this article, the authors carried out a highly uniform survey of the near-Earth object (NEO) population at thermal infrared wavelengths ranging from 3 to 22 μm, allowing them to refine estimates of their numbers, sizes, and albedos.
NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
Amy Mainzer,T. Grav,Joseph R. Masiero,James M. Bauer,E. Hand,David J. Tholen,Robert S. McMillan,T. Spahr,Roc Cutri,Edward L. Wright,J. Watkins,W. Mo,Chet Maleszewski +12 more
TL;DR: In this paper, the authors determined the albedos for nearly 1900 asteroids classified by the Tholen, Bus and Bus-DeMeo taxonomic classification schemes, and found that the S-complex spans a broad range of bright albedo, partially overlapping the low-light C-complex at small sizes.
The Massive and Distant Clusters of WISE Survey. IX. High Radio Activity in a Merging Cluster
Emily Moravec,Anthony H. Gonzalez,Simon Dicker,Stacey Alberts,M. Brodwin,T. Clarke,Thomas Connor,B. Decker,M. Devlin,Peter Eisenhardt,Brian S. Mason,W. Mo,Tony Mroczkowski,Alexandra Pope,C. Romero,Craig L. Sarazin,Jonathan Sievers,S. A. Stanford,D. Stern,Dominika Wylezalek,Fernando Salviatto Zago +20 more
TL;DR: MOO J1506+5137 is a merging cluster with high radio activity. The cluster has a high concentration of massive galaxies and exhibits evidence of an ongoing merger. The radio activity of the cluster is linked to its dynamical state and the merger process.
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NEOWISE Observations of Near-Earth Objects: Preliminary Results
Amy Mainzer,Tommy Grav,James M. Bauer,Joseph Masiero,Robert S. McMillan,Roc M. Cutri,Russell G. Walker,Edward L. Wright,Peter Eisenhardt,David J. Tholen,Timothy Spahr,Robert Jedicke,Larry Denneau,E. DeBaun,D. Elsbury,Thomas Gautier,S. Gomillion,E. Hand,W. Mo,J. A. Watkins,A. Wilkins,G. Bryngelson,A. Del Pino Molina,Shantanu Desai,M. Go'mez Camus,Sebastian L. Hidalgo,I. S. Konstantopoulos,Jeffrey A. Larsen,C. Maleszewski,M. A. Malkan,J. C. Mauduit,B. Mullan,Edward W. Olszewski,Janine Pforr,A. Saro,James V. Scotti,Lawrence H. Wasserman +36 more
TL;DR: In this article, the authors conducted a highly uniform survey of the near-Earth object (NEO) population at thermal infrared wavelengths ranging from 3 to 22$m, allowing them to refine estimates of their numbers, sizes, and albedos.
NEOWISE Studies of Asteroids with Sloan Photometry: Preliminary Results
Amy Mainzer,Joseph R. Masiero,Tommy Grav,James Bauer,David J. Tholen,Robert S. McMillan,Edward L. Wright,Timothy Spahr,Roc M. Cutri,R. Walker,W. Mo,J. A. Watkins,E. Hand,C. Maleszewski +13 more
TL;DR: In this article, the authors combined the NEOWISE and Sloan Digital Sky Survey data to study the albedos of 24,353 asteroids with candidate taxonomic classifications derived using Sloan photometry.