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Amos Yahil
Researcher at Stony Brook University
Publications - 67
Citations - 3416
Amos Yahil is an academic researcher from Stony Brook University. The author has contributed to research in topics: Redshift & Galaxy. The author has an hindex of 28, co-authored 67 publications receiving 3346 citations. Previous affiliations of Amos Yahil include State University of New York System & Siemens.
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A redshift survey of IRAS galaxies. VII - The infrared and redshift data for the 1.936 Jansky sample
TL;DR: In this article, the authors presented the data for a redshift survey of galaxies selected from the database of the Infrared Astronomical Satellite (IRAS), which consists of 5014 objects, of which 2658 are galaxies.
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The IRAS 1.2 Jy Survey: Redshift Data
TL;DR: The data for the complete 1.2 Jy survey (the data presented here in addition to that of Strauss et al. as mentioned in this paper ) can be obtained in a machine-readable form from the National Space Science Data Center and from the anonymous ftp site given above.
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Star-forming galaxies at very high redshifts
TL;DR: In this paper, a catalogue of 1,683 objects with estimated redshifts ranging from z = 0 to z > 6 is presented, interpreted as regions of star formation associated with the progenitors of present-day normal galaxies, at epochs that may reach back 95% of the time to the Big Bang.
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Quantitative Accuracy of Clinical 99mTc SPECT/CT Using Ordered-Subset Expectation Maximization with 3-Dimensional Resolution Recovery, Attenuation, and Scatter Correction
TL;DR: Current commercially available SPECT/CT technology using OSEM-3D reconstruction, scatter correction, and CT-based attenuation correction allows quantification of 99mTc radioactivity concentration in absolute terms within 3.6% in phantoms and 1.1% in patients with a focus on the bladder.
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Clustering in the 1.2-Jy IRAS Galaxy Redshift Survey – II. Redshift distortions and $\xi (r_p, \pi)$
TL;DR: In this paper, the authors examined the effect of redshift space distortions on the galaxy two-point correlation function ξ(r p, π) as a function of separations parallel (r p ) and perpendicular (π) to the line of sight.