S. Perlmutter

Union through UNITY: Cosmology with 2000 SNe Using a Unified Bayesian Framework

Protecting scientific integrity in an age of generative AI

Carnegie Supernova Project I and II: Measurements of H ₀ Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae*

Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and II

Carnegie Supernova Project. II. Near-infrared Spectral Diversity and Template of Type Ia Supernovae

Bump Morphology of the CMAGIC Diagram

Accuracy of environmental tracers and consequences for determining the Type Ia supernova magnitude step

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

A Probabilistic Autoencoder for Type Ia Supernova Spectral Time Series

An Assessment of the In Situ Growth of the Intracluster Light in the High-redshift Galaxy Cluster SpARCS1049+56

Accuracy of environmental tracers and consequences for determining the Type Ia supernova magnitude step

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

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

The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries*

Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events*

The H α star formation main sequence in cluster and field galaxies at <i>z</i> ∼ 1.6

The SNEMO and SUGAR Companion Data Sets

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

Carnegie Supernova Project II: The slowest rising Type Ia supernova LSQ14fmg and clues to the origin of super-Chandrasekhar/03fg-like events

The growth of brightest cluster galaxies and intracluster light over the past 10 billion years

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

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

Carnegie Supernova Project-II: Extending the Near-infrared Hubble Diagram for Type Ia Supernovae to <i>z</i> ∼ 0.1

Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program

The Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population

SNEMO: Improved Empirical Models for Type Ia Supernovae

Eddington-limited Accretion in z ∼ 2 WISE-selected Hot, Dust-obscured Galaxies

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

ALMA Observations of Gas-rich Galaxies in z ∼ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments

SCALA: In situ calibration for integral field spectrographs