papers

Publications (23)

quant-ph2014

Entanglement over global distances via quantum repeaters with satellite links

K. Boone, J. -P. Bourgoin, E. Meyer-Scott +3

We study entanglement creation over global distances based on a quantum repeater architecture that uses low-earth orbit satellites equipped with entangled photon sources, as well a…

astro-ph.IM2022

GIGA-Lens: Fast Bayesian Inference for Strong Gravitational Lens Modeling

A. Gu, X. Huang, W. Sheu +12

We present GIGA-Lens: a gradient-informed, GPU-accelerated Bayesian framework for modeling strong gravitational lensing systems, implemented in TensorFlow and JAX. The three compon…

astro-ph.CO2021

The Twins Embedding of Type Ia Supernovae I: The Diversity of Spectra at Maximum Light

K. Boone, G. Aldering, P. Antilogus +34

We study the spectral diversity of Type Ia supernovae (SNe Ia) at maximum light using high signal-to-noise spectrophotometry of 173 SNe Ia from the Nearby Supernova Factory. We dec…

astro-ph.GA2017

ALMA Observations of Gas-Rich Galaxies in z~1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-Density Environments

A. G. Noble, M. McDonald, A. Muzzin +16

We present ALMA CO (2-1) detections in 11 gas-rich cluster galaxies at z~1.6, constituting the largest sample of molecular gas measurements in z>1.5 clusters to date. The observati…

astro-ph.CO2022

A Probabilistic Autoencoder for Type Ia Supernovae Spectral Time Series

George Stein, Uros Seljak, Vanessa Bohm +37

We construct a physically-parameterized probabilistic autoencoder (PAE) to learn the intrinsic diversity of type Ia supernovae (SNe Ia) from a sparse set of spectral time series. T…

astro-ph.GA2020

See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies

S. C. Williams, I. M. Hook, B. Hayden +9

The Supernova Cosmology Project has conducted the `See Change' programme, aimed at discovering and observing high-redshift (1.13 z 1.75) Type Ia supernovae (SNe Ia).…

astro-ph.CO2015

Improving Cosmological Distance Measurements Using Twin Type Ia Supernovae

H. K. Fakhouri, K. Boone, G. Aldering +41

We introduce a method for identifying "twin" Type Ia supernovae, and using them to improve distance measurements. This novel approach to Type Ia supernova standardization is made p…

astro-ph.HE2025

An Agnostic Approach to Building Empirical Type Ia Supernova Light Curves: Evidence for Intrinsic Chromatic Flux Variation Using Nearby Supernova Factory Data

Jared Hand, A. G. Kim, G. Aldering +35

We present a new empirical Type Ia supernova (SN Ia) model with three chromatic flux variation templates: one phase dependent and two phase independent. No underlying dust extincti…

astro-ph.CO2014

Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant

M. Rigault, G. Aldering, M. Kowalski +35

Previously we used the Nearby Supernova Factory sample to show that SNe~Ia having locally star-forming environments are dimmer than SNe~Ia having locally passive environments.Here…

astro-ph.SR2023

Bump Morphology of the CMAGIC Diagram

L. Aldoroty, L. Wang, P. Hoeflich +38

We apply the color-magnitude intercept calibration method (CMAGIC) to the Nearby Supernova Factory SNe Ia spectrophotometric dataset. The currently existing CMAGIC parameters are t…

astro-ph.CO2018

Correcting for peculiar velocities of Type Ia Supernovae in clusters of galaxies

P. -F. Léget, M. V. Pruzhinskaya, A. Ciulli +43

Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. To perform such measurements the luminosity and cosmological redshift () of the SNe Ia have…

astro-ph.IM2018

A Binary Offset Effect in CCD Readout and Its Impact on Astronomical Data

K. Boone, G. Aldering, Y. Copin +5

We have discovered an anomalous behavior of CCD readout electronics that affects their use in many astronomical applications. An offset in the digitization of the CCD output voltag…

astro-ph.IM2022

Uniform Recalibration of Common Spectrophotometry Standard Stars onto the CALSPEC System using the SuperNova Integral Field Spectrograph

David Rubin, G. Aldering, P. Antilogus +35

We calibrate spectrophotometric optical spectra of 32 stars commonly used as standard stars, referenced to 14 stars already on the HST-based CALSPEC flux system. Observations of CA…

astro-ph.CO2018

SNEMO: Improved Empirical Models for Type Ia Supernovae

C. Saunders, G. Aldering, P. Antilogus +39

Type Ia supernova cosmology depends on the ability to fit and standardize observations of supernova magnitudes with an empirical model. We present here a series of new models of Ty…

astro-ph.CO2019

SUGAR: An improved empirical model of Type Ia Supernovae based on spectral features

P. -F. Léget, E. Gangler, F. Mondon +40

Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. Improving distance measurements of SNe Ia is one technique to better constrain the acceleratio…

astro-ph.CO2021

The Twins Embedding of Type Ia Supernovae II: Improving Cosmological Distance Estimates

K. Boone, G. Aldering, P. Antilogus +34

We show how spectra of Type Ia supernovae (SNe Ia) at maximum light can be used to improve cosmological distance estimates. In a companion article, we used manifold learning to bui…

astro-ph.HE2019

SN 2012dn from early to late times: 09dc-like supernovae reassessed

S. Taubenberger, A. Floers, C. Vogl +40

As a candidate 'super-Chandrasekhar' or 09dc-like Type Ia supernova (SN Ia), SN 2012dn shares many characteristics with other members of this remarkable class of objects but lacks…

astro-ph.HE2018

Understanding Type Ia supernovae through their U-band spectra

J. Nordin, G. Aldering, P. Antilogus +39

Context. Observations of Type Ia supernovae (SNe Ia) can be used to derive accurate cosmological distances through empirical standardization techniques. Despite this success neithe…

astro-ph.GA2017

Galaxy Merger Candidates in High-Redshift Cluster Environments

A. G. Delahaye, T. M. A. Webb, J. Nantais +14

We compile a sample of spectroscopically- and photometrically-selected cluster galaxies from four high-redshift galaxy clusters () from the Spitzer Adaptation of t…

astro-ph.IM2017

SCALA: In-situ calibration for Integral Field Spectrographs

S. Lombardo, D. Küsters, M. Kowalski +39

The scientific yield of current and future optical surveys is increasingly limited by systematic uncertainties in the flux calibration. This is the case for Type Ia supernova (SN I…

astro-ph.SR2017

The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cu

X. Huang, Z. Raha, G. Aldering +39

Correction of Type Ia Supernova brightnesses for extinction by dust has proven to be a vexing problem. Here we study the dust foreground to the highly reddened SN 2012cu, which is…

astro-ph.CO2020

Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate

M. Rigault, V. Brinnel, G. Aldering +40

As part of an on-going effort to identify, understand and correct for astrophysics biases in the standardization of Type Ia supernovae (SNIa) for cosmology, we have statistically c…

astro-ph.CO2020

The SNEMO and SUGAR Companion Datasets

G. Aldering, P. Antilogus, C. Aragon +41

The Nearby Supernova Factory has made spectrophotometric observations of Type Ia supernovae since . This work presents an interim version of the data produced, including $210…