activity
20182024
most citedThe SFR-M Correlation Extends to Low Mass at High Redshift

54 citations · 85 across the 7 of their papers we have counts for

collaborators

7 papers

cs.PF2024

Streaming Data in HPC Workflows Using ADIOS

Greg Eisenhauer, Norbert Podhorszki, Ana Gainaru +12

The "IO Wall" problem, in which the gap between computation rate and data access rate grows continuously, poses significant problems to scientific workflows which have traditionall…

cs.DC2021★ 7 cited

Exploring the Role of Machine Learning in Scientific Workflows: Opportunities and Challenges

Azita Nouri, Philip E. Davis, Pradeep Subedi +1

In this survey, we discuss the challenges of executing scientific workflows as well as existing Machine Learning (ML) techniques to alleviate those challenges. We provide the conte…

cs.LG2021★ 1 cited

Scalable Graph Embedding LearningOn A Single GPU

Azita Nouri, Philip E. Davis, Pradeep Subedi +1

Graph embedding techniques have attracted growing interest since they convert the graph data into continuous and low-dimensional space. Effective graph analytic provides users a de…

cs.DC2021★ 21 cited

Transitioning from file-based HPC workflows to streaming data pipelines with openPMD and ADIOS2

Franz Poeschel, Juncheng E, William F. Godoy +11

This paper aims to create a transition path from file-based IO to streaming-based workflows for scientific applications in an HPC environment. By using the openPMP-api, traditional…

cs.DC2020★ 1 cited

Exploring Trade-offs in Dynamic Task Triggering for Loosely Coupled Scientific Workflows

Zhe Wang, Pradeep Subedi, Shaohua Duan +5

In order to achieve near-time insights, scientific workflows tend to be organized in a flexible and dynamic way. Data-driven triggering of tasks has been explored as a way to suppo…

astro-ph.GA2018★ 54 cited

The SFR-M Correlation Extends to Low Mass at High Redshift

Kartheik G. Iyer, Eric Gawiser, Romeel Davé +8

To achieve a fuller understanding of galaxy evolution, SED fitting can be used to recover quantities beyond stellar masses (M) and star formation rates (SFRs). We use Star Form…