papers

Publications (11)

cs.LG2023

Fully Elman Neural Network: A Novel Deep Recurrent Neural Network Optimized by an Improved Harris Hawks Algorithm for Classification of Pulmonary Arterial Wedge Pressure

Masoud Fetanat, Michael Stevens, Pankaj Jain +3

Heart failure (HF) is one of the most prevalent life-threatening cardiovascular diseases in which 6.5 million people are suffering in the USA and more than 23 million worldwide. Me…

astro-ph.CO2010

A Physical Model for z~2 Dust Obscured Galaxies

Desika Narayanan, Arjun Dey, Christopher Hayward +8

We present a physical model for the origin of z~2 Dust-Obscured Galaxies (DOGs), a class of high-redshift ULIRGs selected at 24 micron which are particularly optically faint (24/R>…

astro-ph.CO2011

The Kennicutt-Schmidt Star Formation Relation at z~2

Desika Narayanan, Thomas J. Cox, Christopher Hayward +1

Recent observations of excited CO emission lines from z~2 disc galaxies have shed light on the Kennicutt-Schmidt relation at high-z via observed SFR-CO (J=2-1) and (J=3-2) relation…

eess.SY2019

A Physiological Control System for an Implantable Heart Pump that Accommodates for Interpatient and Intrapatient Variations

Masoud Fetanat, Michael Stevens, Christopher Hayward +1

Left ventricular assist devices (LVADs) can provide mechanical support for a failing heart as bridge to transplant and destination therapy. Physiological control systems for LVADs…

astro-ph.GA2021

Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement

Daniel Anglés-Alcázar, Eliot Quataert, Philip Hopkins +7

We present cosmological hydrodynamic simulations of a quasar-mass halo ( at z=2) that for the first time resolve gas transport down…

astro-ph.GA2019

Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment

Shea Garrison-Kimmel, Andrew Wetzel, Phillip F. Hopkins +13

We study star formation histories (SFHs) of dwarf galaxies (stellar mass ) from FIRE-2 cosmological zoom-in simulations. We compare dwarf…