activity
20212026
most citedDetection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment

92 citations · 256 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.GA2026

The Low-Mass Baryon Cycle in QUEST Dwarf Galaxies I: Sample definition and first results

Ava Polzin, Hsiao-Wen Chen, Zhijie Qu +3

We introduce the QUEST Dwarfs program, which connects low-mass galaxies' stellar populations, interstellar medium, and circumgalactic medium in a large and coherently analyzed samp…

astro-ph.IM2025

Picture an Astronomer: Best Practices for Retaining Talent in Astrophysics

Ava Polzin, Katherine E. Whitaker, C. Megan Urry +85

Women are consistently underrepresented in astrophysics yet are simultaneously subject to disproportionate attrition at every career stage. This disparity between demonstrated effi…

astro-ph.IM2025★ 4 cited

spike: A tool to drizzle HST, JWST, and Roman PSFs for improved analyses

Ava Polzin

A point spread function (PSF) describes the distribution of light for a pure point source in an astronomical image due to the optics of the instrument. An accurate PSF is key for d…

astro-ph.HE2024★ 2 cited

Dinosaur in a Haystack : X-ray View of the Entrails of SN 2023ixf and the Radio Afterglow of Its Interaction with the Medium Spawned by the Progenitor Star (Paper 1)

A. J. Nayana, Raffaella Margutti, Eli Wiston +24

We present the results from our extensive hard-to-soft X-ray (NuSTAR, Swift-XRT, XMM-Newton, Chandra) and meter-to-mm wave radio (GMRT, VLA, NOEMA) monitoring campaign of the very…

astro-ph.HE2024

Constraints on Relativistic Jets from the Fast X-ray Transient 210423 using Prompt Radio Follow-Up Observations

Dina Ibrahimzade, R. Margutti, J. S. Bright +16

Fast X-ray Transients (FXTs) are a new observational class of phenomena with no clear physical origin. This is at least partially a consequence of limited multi-wavelength follow u…

astro-ph.GA2024★ 8 cited

On the universality of star formation efficiency in galaxies

Ava Polzin, Andrey V. Kravtsov, Vadim A. Semenov +1

We analyze high-resolution hydrodynamics simulations of an isolated disk dwarf galaxy with an explicit model for unresolved turbulence and turbulence-based star formation prescript…

astro-ph.GA2024

Silkscreen: Direct Measurements of Galaxy Distances from Survey Image Cutouts

Tim B. Miller, Imad Pasha, Ava Polzin +1

With upcoming wide field surveys from the ground and space the number of known dwarf galaxies at Mpc is expected to dramatically increase. Insight into their nature a…

astro-ph.GA2024

Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations

Ava Polzin, Laura Newburgh, Priyamvada Natarajan +1

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a drift-scan interferometer designed to map the entire northern sky every 24 hours. The all-sky coverage and sensitivi…

astro-ph.IM2023

Astronomy as a Field: A Guide for Aspiring Astrophysicists

Ava Polzin, Yasmeen Asali, Sanah Bhimani +25

This book was created as part of the SIRIUS B VERGE program to orient students to astrophysics as a broad field. The 2023-2024 VERGE program and the printing of this book is funded…

astro-ph.HE2023

The High Energy X-ray Probe (HEX-P): Sensitive broadband X-ray observations of transient phenomena in the 2030s

Murray Brightman, Raffaella Margutti, Ava Polzin +13

HEX-P will launch at a time when the sky is being routinely scanned for transient gravitational wave, electromagnetic and neutrino phenomena that will require the capabilities of a…

astro-ph.GA2023★ 7 cited

Modeling molecular hydrogen in low metallicity galaxies

Ava Polzin, Andrey V. Kravtsov, Vadim A. Semenov +1

We use a suite of hydrodynamics simulations of the interstellar medium (ISM) within a galactic disk, which include radiative transfer, a non-equilibrium model of molecular hydrogen…

astro-ph.HE2022★ 9 cited

The Luminosity Phase Space of Galactic and Extragalactic X-ray Transients Out to Intermediate Redshifts

Ava Polzin, Raffaella Margutti, Deanne Coppejans +8

We present a detailed compilation and analysis of the X-ray phase space of low- to intermediate-redshift () transients that consolidates observed light curves (and t…

astro-ph.IM2022★ 12 cited

DELIGHT: Deep Learning Identification of Galaxy Hosts of Transients using Multi-resolution Images

Francisco Förster, Alejandra M. Muñoz Arancibia, Ignacio Reyes +25

We present DELIGHT, or Deep Learning Identification of Galaxy Hosts of Transients, a new algorithm designed to automatically and in real-time identify the host galaxies of extragal…

astro-ph.CO2022★ 92 cited

Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment

CHIME Collaboration, Mandana Amiri, Kevin Bandura +30

We present a detection of 21-cm emission from large-scale structure (LSS) between redshift 0.78 and 1.43 made with the Canadian Hydrogen Intensity Mapping Experiment (CHIME). Radio…

astro-ph.IM2022★ 19 cited

Using the Sun to Measure the Primary Beam Response of the Canadian Hydrogen Intensity Mapping Experiment

CHIME Collaboration, Mandana Amiri, Kevin Bandura +27

We present a beam pattern measurement of the Canadian Hydrogen Intensity Mapping Experiment (CHIME) made using the Sun as a calibration source. As CHIME is a pure drift scan instru…

astro-ph.IM2022

An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment

The CHIME Collaboration, Mandana Amiri, Kevin Bandura +40

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a drift scan radio telescope operating across the 400-800 MHz band. CHIME is located at the Dominion Radio Astrophysic…

astro-ph.GA2021★ 13 cited

A Nascent Tidal Dwarf Galaxy Forming within the Northern HI Streamer of M82

Imad Pasha, Deborah Lokhorst, Pieter G. van Dokkum +12

We identify a 600 pc-wide region of active star formation located within a tidal streamer of M82 via emission ( erg s cm), us…

astro-ph.IM2021★ 20 cited

A Method To Characterize the Wide-Angle Point Spread Function of Astronomical Images

Qing Liu, Roberto Abraham, Colleen Gilhuly +14

Uncertainty in the wide-angle Point Spread Function (PSF) at large angles (tens of arcseconds and beyond) is one of the dominant sources of error in a number of important quantitie…

astro-ph.GA2021★ 38 cited

Tidal Distortions in NGC1052-DF2 and NGC1052-DF4: Independent Evidence for a Lack of Dark Matter

Michael A. Keim, Pieter van Dokkum, Shany Danieli +11

Two ultra diffuse galaxies in the same group, NGC1052-DF2 and NGC1052-DF4, have been found to have little or no dark matter and to host unusually luminous globular cluster populati…

astro-ph.GA2021★ 4 cited

Simulating Eclipsing Binary Yields of the Rubin Observatory in the Galactic Field and Star Clusters

Aaron M. Geller, Ava Polzin, Andrew Bowen +1

We present a study of the detection and recovery efficiency of the Rubin Observatory for detached eclipsing binaries (EBs) in the galactic field, globular clusters (GCs) and open c…

astro-ph.GA2021★ 28 cited

A recently quenched isolated dwarf galaxy outside of the Local Group environment

Ava Polzin, Pieter van Dokkum, Shany Danieli +2

We report the serendipitous identification of a low mass (), isolated, likely quenched dwarf galaxy in the "foreground" of the COSMOS-CAN…