L E Bleem
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Explore the profile of L E Bleem including associated specialties, affiliations and a list of published articles.
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Articles
7
Citations
20
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0
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Recent Articles
1.
Raghunathan S, Ade P, Anderson A, Ansarinejad B, Archipley M, Austermann J, et al.
Phys Rev Lett
. 2024 Oct;
133(12):121004.
PMID: 39373410
We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel'dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and Herschel-SPIRE experiments over...
2.
Raghunathan S, Patil S, Baxter E, Benson B, Bleem L, Crawford T, et al.
Phys Rev Lett
. 2019 Nov;
123(18):181301.
PMID: 31763885
We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new...
3.
Hanson D, Hoover S, Crites A, Ade P, Aird K, Austermann J, et al.
Phys Rev Lett
. 2013 Oct;
111(14):141301.
PMID: 24138230
Gravitational lensing of the cosmic microwave background generates a curl pattern in the observed polarization. This "B-mode" signal provides a measure of the projected mass distribution over the entire observable...
4.
Vieira J, Marrone D, Chapman S, De Breuck C, Hezaveh Y, WeiB A, et al.
Nature
. 2013 Mar;
495(7441):344-7.
PMID: 23485967
In the past decade, our understanding of galaxy evolution has been revolutionized by the discovery that luminous, dusty starburst galaxies were 1,000 times more abundant in the early Universe than...
5.
McDonald M, Bayliss M, Benson B, Foley R, Ruel J, Sullivan P, et al.
Nature
. 2012 Aug;
488(7411):349-52.
PMID: 22895340
In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the cluster's lifetime, leading to continuous 'cooling flows' of...
6.
Dobbs M, Lueker M, Aird K, Bender A, Benson B, Bleem L, et al.
Rev Sci Instrum
. 2012 Aug;
83(7):073113.
PMID: 22852677
A technological milestone for experiments employing transition edge sensor bolometers operating at sub-Kelvin temperature is the deployment of detector arrays with 100s-1000s of bolometers. One key technology for such arrays...
7.
Padin S, Staniszewski Z, Keisler R, Joy M, Stark A, Ade P, et al.
Appl Opt
. 2008 Aug;
47(24):4418-28.
PMID: 18716649
The South Pole Telescope is a 10 m diameter, wide-field, offset Gregorian telescope with a 966-pixel, millimeter-wave, bolometer array receiver. The telescope has an unusual optical system with a cold...