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M

M. Brodwin

Researcher at Harvard University

Publications -  59
Citations -  4669

M. Brodwin is an academic researcher from Harvard University. The author has contributed to research in topics: Redshift & Galaxy cluster. The author has an hindex of 38, co-authored 59 publications receiving 4540 citations. Previous affiliations of M. Brodwin include University of Missouri–Kansas City & University of Missouri.

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Number Counts At 3 < lambda < 10 um From the Spitzer Space Telescope

TL;DR: In this article, galaxy counts at wavelengths 3 < lambda < 10 um cover more than 10 magnitudes in source brightness, four orders of magnitude in surface density, and reach an integrated surface density of 10^5 sources/deg^2.
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Cosmological Constraints from Sunyaev-Zel'dovich-Selected Clusters with X-ray Observations in the First 178 Square Degrees of the South Pole Telescope Survey

TL;DR: In this article, the authors used measurements from the South Pole Telescope (SPT) Sunyaev Zel'dovich (SZ) cluster survey in combination with X-ray measurements to constrain cosmological parameters.
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An SZ-selected sample of the most massive galaxy clusters in the 2500-square-degree South Pole Telescope survey

TL;DR: The South Pole Telescope (SPT) is currently surveying 2500 deg^2 of the southern sky to detect massive galaxy clusters out to the epoch of their formation using the Sunyaev-Zel'dovich (SZ) effect as mentioned in this paper.
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Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope

TL;DR: In this article, the authors derived cosmological constraints using a galaxy cluster sample selected from the 2500~deg$^2$ SPT-SZ survey, which is supplemented with optical weak gravitational lensing measurements of 32 clusters with $0.29
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Galaxy Clusters around radio-loud AGN at 1.3 < z < 3.2 as seen by Spitzer

TL;DR: The first results from the Clusters Around Radio-Loud AGN (CARLA) program are reported in this article, where the authors investigate the environments of a large sample of obscured and unobscured luminous radio-loud AGNs at 1.2 -0.1 (AB), which efficiently selects high-redshift (z > 1.3) galaxies of all types.