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Mark A. Kramer

Researcher at Boston University

Publications -  103
Citations -  7952

Mark A. Kramer is an academic researcher from Boston University. The author has contributed to research in topics: Epilepsy & Ictal. The author has an hindex of 39, co-authored 103 publications receiving 6539 citations. Previous affiliations of Mark A. Kramer include University of California, Berkeley & Oberlin College.

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Dynamic cross-frequency couplings of local field potential oscillations in rat striatum and hippocampus during performance of a T-maze task

TL;DR: Cross-frequency coupling of multiple neuronal rhythms could be a general mechanism used by the brain to perform network-level dynamical computations underlying voluntary behavior, particularly during decision-making behavioral epochs.
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Epilepsy as a Disorder of Cortical Network Organization

TL;DR: This review examines some aspects of cortical network organization that distinguish epileptic cortex from normal brain as well as the dynamics of network activity before and during seizures, focusing primarily on focal seizures.
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Age-Related Changes in 1/f Neural Electrophysiological Noise.

TL;DR: It is found, in two separate human studies, that 1/f electrophysiological noise increases with aging, and it is observed that this age-related 1/ f noise statistically mediates age- related working memory decline.
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Rhizosphere processes are quantitatively important components of terrestrial carbon and nutrient cycles.

TL;DR: It is shown that root-accelerated mineralization and priming can account for up to one-third of the total C and N mineralized in temperate forest soils and that rhizosphere processes are a widespread, quantitatively important driver of SOM decomposition and nutrient release at the ecosystem scale.
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Search for co outflows toward a sample of 69 high-mass protostellar candidates. II. Outflow properties

TL;DR: In this paper, the authors present a study of molecular outflows toward a sample of 69 luminous IRAS point sources, associated with dense molecular gas and having far-infrared luminosities ranging from 102 to 105 L☉, indicating these objects as regions likely forming high-mass stars.