papers

Publications (22)

astro-ph.CO2026

Feeling Blue: Constructing a Robust SALT3 UV Template and Constraining its Redshift Dependency

Qinan Wang, David O. Jones, Justin D. R. Pierel +13

Upcoming cosmological surveys will obtain numerous rest-frame ultraviolet (UV) observations of Type Ia supernovae (SNe Ia), yet there is concern about how standardizable SNe Ia are…

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

Variability-finding in Rubin Data Preview 1 with LSDB

Konstantin Malanchev, Melissa DeLucchi, Neven Caplar +56

The Vera C. Rubin Observatory recently released Data Preview 1 (DP1) in advance of the upcoming Legacy Survey of Space and Time (LSST), which will enable boundless discoveries in t…

astro-ph.HE2019

Red and Reddened: Ultraviolet through Near-Infrared Observations of Type Ia Supernova 2017erp

Peter J. Brown, Griffin Hosseinzadeh, Saurabh W. Jha +20

We present space-based ultraviolet/optical photometry and spectroscopy with the Swift Ultra-Violet/Optical Telescope and Hubble Space Telescope, respectively, along with ground-bas…

astro-ph.HE2023

A Low-Mass Helium Star Progenitor Model for the Type Ibn SN 2020nxt

Qinan Wang, Anika Goel, Luc Dessart +55

A growing number of supernovae (SNe) are now known to exhibit evidence for significant interaction with a dense, pre-existing, circumstellar medium (CSM). SNe Ibn comprise one such…

astro-ph.HE2022

Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad

Lindsey A. Kwok, Marc Williamson, Saurabh W. Jha +11

Few published ultraviolet (UV) spectra exist for stripped-envelope supernovae, and none to date for broad-lined Type Ic supernovae (SN Ic-bl). These objects have extremely high eje…

astro-ph.CO2016

Exploring uncertainties in dark energy constraints using current observational data with Planck 2015 distance priors

Yun Wang, Mi Dai

We present the distance priors that we have derived from the 2015 Planck data, and use these in combination with the latest observational data from Type Ia Supernovae (SNe Ia) and…

astro-ph.CO2016

Sampling the Probability Distribution of Type Ia Supernova Lightcurve Parameters in Cosmological Analysis

Mi Dai, Yun Wang

In order to obtain robust cosmological constraints from Type Ia supernova (SN Ia) data, we have applied Markov Chain Monte Carlo (MCMC) to SN Ia lightcurve fitting. We develop a me…

astro-ph.IM2026

Hyrax: An Extensible Framework for Rapid ML Experimentation and Unsupervised Discovery in the Era of Rubin, Roman, and Euclid

Aritra Ghosh, Drew Oldag, Michael Tauraso +29

The NSF-DOE Vera C. Rubin Observatory, Roman Space Telescope, Euclid, and other next-generation surveys will deliver imaging, spectroscopic, and time-domain data at scales that inc…

astro-ph.HE2021

The Foundation Supernova Survey: Photospheric Velocity Correlations in Type Ia Supernovae

Kyle G. Dettman, Saurabh W. Jha, Mi Dai +14

The ejecta velocities of type-Ia supernovae (SNe Ia), as measured by the Si II line, have been shown to correlate with other supernova properties, including color and stan…

astro-ph.HE2026

JWST Spectroscopy of SN Ia 2022aaiq and 2024gy: Evidence for Enhanced Central Stable Ni Abundance and a Deflagration-to-Detonation Transition

Lindsey A. Kwok, Chang Liu, Saurabh W. Jha +48

We present optical + near-infrared (NIR) + mid-infrared (MIR) observations of the normal Type Ia supernovae (SN Ia) 2022aaiq and 2024gy in the nebular phase, continuously spanning…

astro-ph.HE2026

JWST Nebular Spectroscopy of SN 2023qov: Circumstellar Dust Emission in a Normal Type Ia Supernova

Colin W. Macrie, Conor Larison, Huei Sears +42

We present panchromatic observations of the Type Ia supernova (SN Ia) 2023qov, ranging from 2 weeks before to 1 year after maximum light. \textit{JWST} near- and mid-in…

astro-ph.CO2022

The Pantheon+ Analysis: SuperCal-Fragilistic Cross Calibration, Retrained SALT2 Light Curve Model, and Calibration Systematic Uncertainty

Dillon Brout, Georgie Taylor, Dan Scolnic +9

We present here a re-calibration of the photometric systems used in the Pantheon+ sample of Type Ia supernovae (SNe Ia) including those used for the SH0ES distance-ladder measureme…

astro-ph.CO2013

SZ effect or Not? - Detecting most galaxy clusters' main foreground effect

Weike Xiao, Chen Chen, Bin Zhang +2

Galaxy clusters are the most massive objects in the Universe and comprise a high-temperature intracluster medium of about 10^7 K, believed to offer a main foreground effect for cos…

astro-ph.IM2018

The Photometric LSST Astronomical Time-series Classification Challenge (PLAsTiCC): Data set

The PLAsTiCC team, Tarek Allam, Anita Bahmanyar +23

The Photometric LSST Astronomical Time Series Classification Challenge (PLAsTiCC) is an open data challenge to classify simulated astronomical time-series data in preparation for o…

astro-ph.CO2018

Photometric classification and redshift estimation of LSST Supernovae

Mi Dai, Steve Kuhlmann, Yun Wang +1

Supernova (SN) classification and redshift estimation using photometric data only have become very important for the Large Synoptic Survey Telescope (LSST), given the large number…

astro-ph.IM2026

LightCurveLynx: Forward Modeling of Time-Domain Surveys with Application to ZTF SN Ia DR2

Mi Dai, Jeremy Kubica, Konstantin Malanchev +5

We present LightCurveLynx, a flexible and extensible software framework for end-to-end forward modeling time-domain light curves. Given the growing need for realistic simulations i…

astro-ph.CO2023

Are classification metrics good proxies for SN Ia cosmological constraining power?

Alex I. Malz, Mi Dai, Kara A. Ponder +10

Context: When selecting a classifier to use for a supernova Ia (SN Ia) cosmological analysis, it is common to make decisions based on metrics of classification performance, i.e. co…

astro-ph.CO2022

The Pantheon+ Analysis: Cosmological Constraints

Dillon Brout, Dan Scolnic, Brodie Popovic +43

We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves of 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift from t…

astro-ph.CO2025

Tip of the Red Giant Branch Distances to NGC 1316, NGC 1380, NGC 1404, & NGC 4457: A Pilot Study of a Parallel Distance Ladder Using Type Ia Supernovae in Early-Type Host Galaxies

Max J. B. Newman, Conor Larison, Saurabh W. Jha +10

Though type-Ia supernovae (SNe Ia) are found in all types of galaxies, recent local Hubble constant measurements have disfavored using SNe Ia in early-type or quiescent galaxies, a…

astro-ph.IM2020

Active learning with RESSPECT: Resource allocation for extragalactic astronomical transients

Noble Kennamer, Emille E. O. Ishida, Santiago Gonzalez-Gaitan +12

The recent increase in volume and complexity of available astronomical data has led to a wide use of supervised machine learning techniques. Active learning strategies have been pr…

astro-ph.HE2023

Over 500 Days in the Life of the Photosphere of the Type Iax Supernova SN 2014dt

Yssavo Camacho-Neves, Saurabh W. Jha, Barnabas Barna +20

Type Iax supernovae (SN Iax) are the largest known class of peculiar white dwarf supernovae, distinct from normal Type Ia supernovae (SN Ia). The unique properties of SN Iax, espec…