papers

Publications (15)

astro-ph.CO2018

Identifying Reionization Sources from 21cm Maps using Convolutional Neural Networks

Sultan Hassan, Adrian Liu, Saul Kohn +1

Active Galactic Nuclei (AGN) and star-forming galaxies are leading candidates for being the luminous sources that reionized our Universe. Next-generation 21cm surveys are promising…

astro-ph.CO2019

Astro2020 Science White Paper: First Stars and Black Holes at Cosmic Dawn with Redshifted 21-cm Observations

Jordan Mirocha, Daniel Jacobs, Josh Dillon +39

The "cosmic dawn" refers to the period of the Universe's history when stars and black holes first formed and began heating and ionizing hydrogen in the intergalactic medium (IGM).…

astro-ph.CO2018

Reionization Models Classifier using 21cm Map Deep Learning

Sultan Hassan, Adrian Liu, Saul Kohn +3

Next-generation 21cm observations will enable imaging of reionization on very large scales. These images will contain more astrophysical and cosmological information than the power…

astro-ph.CO2019

Cosmology with the Highly Redshifted 21cm Line

Adrian Liu, James Aguirre, Yacine Ali-Haimoud +47

In addition to being a probe of Cosmic Dawn and Epoch of Reionization astrophysics, the 21cm line at is also a powerful way to constrain cosmology. Its power derives from sev…

astro-ph.CO2020

The 21 cm-kSZ-kSZ Bispectrum during the Epoch of Reionization

Paul La Plante, Adam Lidz, James Aguirre +1

The high-redshift 21 cm signal from the Epoch of Reionization (EoR) is a promising observational probe of the early universe. Current- and next-generation radio interferometers suc…

astro-ph.CO2017

New Limits on Polarized Power Spectra at 126 and 164 MHz: Relevance to Epoch of Reionization Measurements

David Moore, James E. Aguirre, Saul Kohn +15

Polarized foreground emission is a potential contaminant of attempts to measure the fluctuation power spectrum of highly redshifted 21 cm HI emission from the epoch of reionization…

eess.IV2021

A Pathology Deep Learning System Capable of Triage of Melanoma Specimens Utilizing Dermatopathologist Consensus as Ground Truth

Sivaramakrishnan Sankarapandian, Saul Kohn, Vaughn Spurrier +9

Although melanoma occurs more rarely than several other skin cancers, patients' long term survival rate is extremely low if the diagnosis is missed. Diagnosis is complicated by a h…

astro-ph.IM2019

Optimizing Sparse RFI Prediction using Deep Learning

Joshua Kerrigan, Paul La Plante, Saul Kohn +61

Radio Frequency Interference (RFI) is an ever-present limiting factor among radio telescopes even in the most remote observing locations. When looking to retain the maximum amount…

astro-ph.IM2016

The Astropy Problem

Demitri Muna, Michael Alexander, Alice Allen +151

The Astropy Project (http://astropy.org) is, in its own words, "a community effort to develop a single core package for Astronomy in Python and foster interoperability between Pyth…

astro-ph.IM2019

Improved 21 cm Epoch Of Reionization Power Spectrum Measurements with a Hybrid Foreground Subtraction and Avoidance Technique

Joshua Kerrigan, Jonathan Pober, Zaki Ali +16

Observations of the 21cm Epoch of Reionization (EoR) signal are dominated by Galactic and extragalactic foregrounds. The need for foreground removal has led to the development of t…

astro-ph.CO2016

The Hydrogen Epoch of Reionization Array Dish II: Characterization of Spectral Structure with Electromagnetic Simulations and its science Implications

Aaron Ewall-Wice, Richard Bradley, David DeBoer +25

We use time-domain electromagnetic simulations to determine the spectral characteristics of the Hydrogen Epoch of Reionization Arrays (HERA) antenna. These simulations are part of…

astro-ph.CO2017

Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization

Avery Meiksin, Sadegh Khochfar, Jan-Pieter Paardekooper +2

The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure-driven wind and a superbubble…

astro-ph.CO2022

HERA Phase I Limits on the Cosmic 21-cm Signal: Constraints on Astrophysics and Cosmology During the Epoch of Reionization

The HERA Collaboration, Zara Abdurashidova, James E. Aguirre +81

Recently, the Hydrogen Epoch of Reionization Array (HERA) collaboration has produced the experiment's first upper limits on the power spectrum of 21-cm fluctuations at z~8 and 10.…

astro-ph.CO2019

Astro2020 Science White Paper: Insights Into the Epoch of Reionization with the Highly-Redshifted 21-cm Line

Steven Furlanetto, Chris L. Carilli, Jordan Mirocha +47

The epoch of reionization, when photons from early galaxies ionized the intergalactic medium about a billion years after the Big Bang, is the last major phase transition in the Uni…

astro-ph.CO2019

Astro 2020 Science White Paper: Fundamental Cosmology in the Dark Ages with 21-cm Line Fluctuations

Steven Furlanetto, Judd D. Bowman, Jordan Mirocha +43

The Dark Ages are the period between the last scattering of the cosmic microwave background and the appearance of the first luminous sources, spanning approximately 1100 < z < 30.…