E
Edward J. Wollack
Researcher at Goddard Space Flight Center
Publications - 794
Citations - 109859
Edward J. Wollack is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: Cosmic microwave background & Atacama Cosmology Telescope. The author has an hindex of 104, co-authored 732 publications receiving 102070 citations. Previous affiliations of Edward J. Wollack include Raytheon & West Chester University of Pennsylvania.
Papers
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Journal ArticleDOI
A high-resolution map of the cosmic microwave background around the north celestial pole
Max Tegmark,Angelica de Oliveira-Costa,Angelica de Oliveira-Costa,M. J. Devlin,C. Barth Netterfield,Lyman A. Page,Edward J. Wollack +6 more
TL;DR: In this paper, a Wiener filtered map of the Cosmic Microwave Background (CMB) fluctuations in a disk with 15 degree diameter, centered at the North Celestial Pole, is presented.
Journal ArticleDOI
Auxiliary components for kilopixel transition edge sensor arrays
Ari-David Brown,David T. Chuss,Vilem Mikula,Ross Henry,Edward J. Wollack,Yue Zhao,Gene C. Hilton,James A. Chervenak +7 more
TL;DR: In this article, the Atacama Cosmology Telescope (ACT) was used to probe the cosmic microwave background at 145, 215, and 280 GHz using a transition edge sensor bolometer.
Journal Article
A Degree-Scale Measurement of the Anisotropy in the Cosmic Microwave Background
TL;DR: In this paper, the authors reported the detection of anisotropy in the microwave sky at 3O GHz and at l deg angular scales, assuming a Gaussian auto-correlation function with a coherence angle of 1.2 deg.
Proceedings ArticleDOI
Aerogel scattering filters for cosmic microwave background observations
Thomas Essinger-Hileman,Charles L. Bennett,Lance Corbett,Haiquan Guo,Tobias A. Marriage,Mary Ann B. Meador,Karwan Rostem,Edward J. Wollack +7 more
TL;DR: In this article, the authors present the design and performance of broadband and tunable infrared-blocking filters for millimeter and sub-millimeter astronomy composed of small scattering particles embedded in an aerogel substrate.
Journal ArticleDOI
Venus Observations at 40 and 90 GHz with CLASS
Sumit Dahal,Sumit Dahal,Michael K. Brewer,John W. Appel,Aamir Ali,Aamir Ali,Charles L. Bennett,Ricardo Bustos,Manwei Chan,David T. Chuss,Joseph Cleary,Jullianna Couto,Rahul Datta,Kevin L. Denis,Joseph Eimer,Francisco Espinoza,Thomas Essinger-Hileman,Thomas Essinger-Hileman,Dominik Gothe,Kathleen Harrington,Kathleen Harrington,Jeffrey Iuliano,John Karakla,Tobias A. Marriage,Sasha Novack,Carolina Núñez,Ivan L. Padilla,Lucas Parker,Lucas Parker,Matthew Petroff,Rodrigo Reeves,Gary Rhoades,Karwan Rostem,Deniz Augusto Nunes Valle,Duncan J. Watts,Duncan J. Watts,Janet L. Weiland,Edward J. Wollack,Zhilei Xu,Zhilei Xu +39 more
TL;DR: In this article, the Cosmology Large Angular Scale Surveyor (LASS) was used to measure the disk-averaged absolute Venus brightness temperature to be 432.3 K and 355.6 K in the Q and W frequency bands.