papers

Publications (54)

astro-ph.CO2013

Integral field spectroscopy of supernova explosion sites: constraining mass and metallicity of the progenitors -- II. Type II-P and II-L supernovae

Hanindyo Kuncarayakti, Mamoru Doi, Greg Aldering +6

Thirteen explosion sites of type II-P and II-L supernovae in nearby galaxies have been observed using integral field spectroscopy, enabling both spatial and spectral study of the e…

astro-ph.HE2024

SCAT Uncovers ATLAS's First Tidal Disruption Event ATLAS18mlw: A Faint and Fast TDE in a Quiescent Balmer Strong Galaxy

Jason T. Hinkle, Michael A. Tucker, Benjamin. J. Shappee +10

We present the discovery that ATLAS18mlw was a tidal disruption event (TDE) in the galaxy WISEA J073544.83+663717.3, at a luminosity distance of 334 Mpc. Initially discovered by th…

astro-ph.IM2018

Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Deep Drilling Fields and other Special Programs

Daniel M. Scolnic, Michelle Lochner, Phillipe Gris +21

We review the measurements of dark energy enabled by observations of the Deep Drilling Fields and the optimization of survey design for cosmological measurements. This white paper…

astro-ph2006

Snapping Supernovae at z>1.7

Greg Aldering, Alex G. Kim, Marek Kowalski +2

We examine the utility of very high redshift Type Ia supernovae for cosmology and systematic uncertainty control. Next generation space surveys such as the Supernova/Acceleration P…

astro-ph.CO2025

Fishing for the Optimal Roman High Latitude Time Domain Survey: Cosmological Constraints for 1,000 Possible Surveys

David Rubin, Greg Aldering, Andy Fruchter +9

The upcoming Nancy Grace Roman Space Telescope is set to conduct a generation-defining SN Ia cosmology measurement with its High Latitude Time Domain Survey (HLTDS). However, betwe…

astro-ph.HE2012

Evidence for Type Ia Supernova Diversity from Ultraviolet Observations with the Hubble Space Telescope

Xiaofeng Wang, Lifan Wang, Alexei V. Filippenko +93

We present ultraviolet (UV) spectroscopy and photometry of four Type Ia supernovae (SNe 2004dt, 2004ef, 2005M, and 2005cf) obtained with the UV prism of the Advanced Camera for Sur…

astro-ph.IM2026

Three-dimensional scene reconstruction using Roman slitless spectra

Tri L. Astraatmadja, Andrew S. Fruchter, Susana E. Deustua +10

The Nancy Grace Roman Space Telescope will carry out a wide-field imaging and slitless spectroscopic survey of Type Ia Supernovae to improve our understanding of dark energy. Cruci…

astro-ph2003

Multi-Color Light Curves of Type Ia Supernovae on the Color-Magnitude Diagram: a Novel Step Toward More Precise Distance and Extinction Estimates

Lifan Wang, Gerson Goldhaber, Greg Aldering +1

We show empirically that fits to the color-magnitude relation of Type Ia supernovae after optical maximum can provide accurate relative extragalactic distances. We report the disco…

astro-ph.CO2022

Evaluating and Optimizing a Slitless Prism for Nancy Grace Roman Space Telescope SN Cosmology

David Rubin, Greg Aldering, Tri L. Astraatmadja +9

This work presents a set of studies addressing the use of the low-dispersion slitless prism on Roman for SN spectroscopy as part of the Roman High Latitude Time Domain Survey (HLTD…

astro-ph.CO2021

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

Brian Hayden, David Rubin, Kyle Boone +53

The See Change survey was designed to make cosmological measurements by efficiently discovering high-redshift Type Ia supernovae (SNe Ia) and improving cluster mass measureme…

astro-ph.CO2026

Banana Split: Improved Cosmological Constraints with Two Light-Curve-Shape and Color Populations Using Union3.1+UNITY1.8

David Rubin, Taylor Hoyt, Greg Aldering +1

SNe Ia have been used to provide key constraints on the equation-of-state parameter of dark energy. They are generally standardized under the assumption that they belong to a singl…

astro-ph.GA2019

The Growth of Brightest Cluster Galaxies and Intracluster Light Over the Past Ten Billion Years

Tahlia DeMaio, Anthony H. Gonzalez, Ann Zabludoff +9

We constrain the evolution of the brightest cluster galaxy plus intracluster light (BCG+ICL) using an ensemble of 42 galaxy groups and clusters that span redshifts of z = 0.05-1.75…

astro-ph.SR2009

V1647 Orionis: Reinvigorated Accretion and the Re-Appearance of McNeil's Nebula

Colin Aspin, Bo Reipurth, Tracy L. Beck +10

In late 2003, the young eruptive variable star V1647 Orionis optically brightened by over 5 magnitudes, stayed bright for around 26 months, and then decline to its pre-outburst lev…

astro-ph.HE2024

The MOST Hosts Survey: spectroscopic observation of the host galaxies of ~40,000 transients using DESI

Maayane T. Soumagnac, Peter Nugent, Robert A. Knop +54

We present the MOST Hosts survey (Multi-Object Spectroscopy of Transient Hosts). The survey is planned to run throughout the five years of operation of the Dark Energy Spectroscopi…

astro-ph.CO2025

Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

David Rubin, Greg Aldering, Marc Betoule +8

Type Ia supernovae (SNe Ia) were instrumental in establishing the acceleration of the universe's expansion. By virtue of their combination of distance reach, precision, and prevale…

astro-ph.SR2014

Kiso Supernova Survey (KISS): Survey Strategy

Tomoki Morokuma, Nozomu Tominaga, Masaomi Tanaka +58

The Kiso Supernova Survey (KISS) is a high-cadence optical wide-field supernova (SN) survey. The primary goal of the survey is to catch the very early light of a SN, during the sho…

astro-ph.IM2025

The La Silla Schmidt Southern Survey

Adam A. Miller, Natasha S. Abrams, Greg Aldering +75

We present the La Silla Schmidt Southern Survey (LS4), a new wide-field, time-domain survey to be conducted with the 1 m ESO Schmidt telescope. The 268 megapixel LS4 camera mosaics…

astro-ph.CO2019

Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z>1

Jinhyub Kim, M. James Jee, Saul Perlmutter +5

We present a detailed high-resolution weak-lensing (WL) study of SPT-CL J2106-5844 at z=1.132, claimed to be the most massive system discovered at z > 1 in the South Pole Telescope…

astro-ph.CO2019

The Next Generation of Cosmological Measurements with Type Ia Supernovae

Dan Scolnic, Saul Perlmutter, Greg Aldering +56

While Type Ia Supernovae (SNe Ia) are one of the most mature cosmological probes, the next era promises to be extremely exciting in the number of different ways SNe Ia are used to…

astro-ph.CO2015

The Massive and Distant Clusters of WISE Survey: MOO J1142+1527, A 10 M Galaxy Cluster at z=1.19

Anthony H. Gonzalez, Bandon Decker, Mark Brodwin +19

We present confirmation of the cluster MOO J1142+1527, a massive galaxy cluster discovered as part of the Massive and Distant Clusters of WISE Survey. The cluster is confirmed to l…

astro-ph.CO2022

Snowmass2021 Cosmic Frontier CF6 White Paper: Multi-Experiment Probes for Dark Energy -- Transients

Alex G. Kim, Antonella Palmese, Maria E. S. Pereira +14

This invited Snowmass 2021 White Paper highlights the power of joint-analysis of astronomical transients in advancing HEP Science and presents research activities that can realize…

astro-ph.GA2018

The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22

David Rubin, Brian Hayden, Xiaosheng Huang +32

We present the discovery and measurements of a gravitationally lensed supernova (SN) behind the galaxy cluster MOO J1014+0038. Based on multi-band Hubble Space Telescope and Very L…

astro-ph.IM2026

The Lazuli Space Observatory: Architecture & Capabilities

Arpita Roy, Stuart Feldman, Pete Klupar +51

The Lazuli Space Observatory is a 3-meter aperture astronomical facility designed for rapid-response observations and precision astrophysics across visible to near-infrared wavelen…

astro-ph.IM2019

Astro2020 APC White Paper: The MegaMapper: a z > 2 spectroscopic instrument for the study of Inflation and Dark Energy

David J. Schlegel, Juna A. Kollmeier, Greg Aldering +74

MegaMapper is a proposed ground-based experiment to measure Inflation parameters and Dark Energy from galaxy redshifts at 2<z<5. A 6.5-m Magellan telescope will be coupled with DES…

astro-ph.EP2011

Ground-Based Submillimagnitude CCD Photometry of Bright Stars Using Snapshot Observations

Andrew W. Mann, Eric Gaidos, Greg Aldering

We demonstrate ground-based submillimagnitude (<10^-3) photometry of widely separated bright stars using snapshot CCD imaging. We routinely achieved this photometric precision by (…

astro-ph.CO2022

A Spectroscopic Road Map for Cosmic Frontier: DESI, DESI-II, Stage-5

David J. Schlegel, Simone Ferraro, Greg Aldering +62

In this white paper, we present an experimental road map for spectroscopic experiments beyond DESI. DESI will be a transformative cosmological survey in the 2020s, mapping 40 milli…

astro-ph.IM2023

Roman CCS White Paper: Optimizing the HLTDS Cadence at Fixed Depth

David Rubin, Ben Rose, Rebekah Hounsell +4

The current proposal for the High Latitude Time Domain Survey (HLTDS) is two tiers (wide and deep) of multi-band imaging and prism spectroscopy with a cadence of five days (Rose et…

astro-ph.CO2026

Union3.1: Self-consistent Measurements of Host Galaxy Properties for 2000 Type Ia Supernovae

Taylor J. Hoyt, David Rubin, Greg Aldering +3

The determination of distances using time-series photometry of Type Ia supernovae (SNe Ia) relies on a ~5% empirical correction related to the properties of their host galaxies, e.…

astro-ph.IM2023

Approaches to lowering the cost of large space telescopes

Ewan S Douglas, Greg Aldering, Greg W. Allan +26

New development approaches, including launch vehicles and advances in sensors, computing, and software, have lowered the cost of entry into space, and have enabled a revolution in…

astro-ph.CO2009

Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae

Tomoki Morokuma, Kouichi Tokita, Christopher Lidman +30

We present spectra of high-redshift supernovae (SNe) that were taken with the Subaru low resolution optical spectrograph, FOCAS. These SNe were found in SN surveys with Suprime-Cam…

astro-ph.CO2025

HOLISMOKES XIX: SN 2025wny at , the first strongly lensed superluminous supernova

Stefan Taubenberger, Ana Acebron, Raoul Cañameras +45

We present imaging and spectroscopic observations of supernova SN 2025wny, associated with the lens candidate PS1 J0716+3821. Photometric monitoring from the Lulin and Maidanak obs…

astro-ph.CO2016

UNITY: Confronting Supernova Cosmology's Statistical and Systematic Uncertainties in a Unified Bayesian Framework

David Rubin, Greg Aldering, Kyle Barbary +12

While recent supernova cosmology research has benefited from improved measurements, current analysis approaches are not statistically optimal and will prove insufficient for future…

astro-ph.CO2026

The Carousel Lens II: Cosmological Constraints with GIGA-Lens

Felipe Urcelay, Xiaosheng Huang, William Sheu +28

The nature of dark matter and dark energy are among the central questions in cosmology. Strong gravitational lenses with multiple source planes provide a geometric probe of cosmolo…

astro-ph.GA2017

Eddington-Limited Accretion in z~2 WISE-selected Hot, Dust-Obscured Galaxies

Jingwen Wu, Hyunsung D. Jun, Roberto J. Assef +12

Hot, Dust-Obscured Galaxies, or "Hot DOGs", are a rare, dusty, hyperluminous galaxy population discovered by the WISE mission. Predominantly at redshifts 2-3, they include the most…

astro-ph.CO2011

The Most Slowly Declining Type Ia Supernova 2001ay

Kevin Krisciunas, Weidong Li, Thomas Matheson +28

We present optical and near-infrared photometry, as well as ground-based optical spectra and Hubble Space Telescope ultraviolet spectra, of the Type Ia supernova (SN) 2001ay. At ma…

astro-ph.CO2013

Integral field spectroscopy of supernova explosion sites: constraining mass and metallicity of the progenitors - I. Type Ib and Ic supernovae

Hanindyo Kuncarayakti, Mamoru Doi, Greg Aldering +6

Integral field spectroscopy of 11 type-Ib/c supernova explosion sites in nearby galaxies has been obtained using UH88/SNIFS and Gemini-N/GMOS. The use of integral field spectroscop…

astro-ph.CO2026

Testing CDM versus dynamical dark energy in one year: A DESI spectroscopic follow-up program for Rubin supernovae

Jannik Truong, Greg Aldering, Saul Perlmutter +2

Combined cosmological probes currently indicate that best-fit values in the parametrization of dynamical dark energy deviate from CDM by . In this work, we p…

astro-ph.IM2014

A flux calibration device for the SuperNova Integral Field Spectrograph (SNIFS)

Simona Lombardo, Greg Aldering, Akos Hoffmann +4

Observational cosmology employing optical surveys often require precise flux calibration. In this context we present SNIFS Calibration Apparatus (SCALA), a flux calibration system…

astro-ph2000

The Rise Times of High and Low Redshift Type Ia Supernovae are Consistent

Greg Aldering, Robert Knop, Peter Nugent

We present a self-consistent comparison of the rise times for low- and high-redshift Type Ia supernovae. Following previous studies, the early light curve is modeled using a t-squa…

astro-ph.CO2023

Target Selection for the DESI Peculiar Velocity Survey

Christoph Saulder, Cullan Howlett, Kelly A. Douglass +35

We describe the target selection and characteristics of the DESI Peculiar Velocity Survey, the largest survey of peculiar velocities (PVs) using both the fundamental plane (FP) and…

astro-ph.IM2022

The MegaMapper: A Stage-5 Spectroscopic Instrument Concept for the Study of Inflation and Dark Energy

David J. Schlegel, Juna A. Kollmeier, Greg Aldering +86

In this white paper, we present the MegaMapper concept. The MegaMapper is a proposed ground-based experiment to measure Inflation parameters and Dark Energy from galaxy redshifts a…

astro-ph2006

Visible and Near-Infrared Spectrophotometry of the Deep Impact Ejecta of Comet 9P/Tempel 1

Klaus W. Hodapp, Greg Aldering, Karen J. Meech +12

We have obtained optical spectrophotometry of the evolution of comet 9P/Tempel 1 after the impact of the Deep Impact probe, using the Supernova Integral Field Spectrograph (SNIFS)…

astro-ph.CO2014

The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey

Jun E. Okumura, Yutaka Ihara, Mamoru Doi +15

We present measurements of the rates of high-redshift Type Ia supernovae derived from the Subaru/XMM-Newton Deep Survey (SXDS). We carried out repeat deep imaging observations with…

astro-ph.GA2016

Isophote Shapes of Early-Type Galaxies in Massive Clusters at and 0

Kazuma Mitsuda, Mamoru Doi, Tomoki Morokuma +5

We compare the isophote shape parameter of early-type galaxies (ETGs) between and 0 as a proxy for dynamics to investigate the epoch at which the dynamical propert…

astro-ph.IM2021

Going Forward with the Nancy Grace Roman Space Telescope Transient Survey: Validation of Precision Forward-Modeling Photometry for Undersampled Imaging

David Rubin, Aleksandar Cikota, Greg Aldering +3

The Nancy Grace Roman Space Telescope (Roman) is an observatory for both wide-field observations and coronagraphy that is scheduled for launch in the mid 2020's. Part of the planne…

astro-ph.IM2023

Roman CCS White Paper: Measuring Type Ia Supernovae Discovered in the Roman High Latitude Time Domain Survey

Rebekah Hounsell, Dan Scolnic, Dillon Brout +14

We motivate the cosmological science case of measuring Type Ia supernovae with the Nancy Grace Roman Space Telescope as part of the High Latitude Time Domain Survey. We discuss pre…

astro-ph.IM2023

Roman CCS White Paper: Considerations for Selecting Fields for the Roman High-latitude Time Domain Core Community Survey

Benjamin Rose, Greg Aldering, Rebekah Hounsell +6

In this white paper, we review five top considerations for selecting locations of the fields of the Roman High-latitude Time Domain Survey. Based on these considerations, we recomm…

astro-ph.IM2023

Roman CCS White Paper: Balanced Prism Plus Filter Cadence in the High Latitude Time Domain Survey Core Community Survey

Greg Aldering, David Rubin, Benjamin Rose +3

The Nancy Grace Roman Space Telescope's (RST) Wide Field Imager (WFI) is equipped with a slitless prism that can be used for spectroscopic discovery and follow-up of explosive tran…

astro-ph.SR2020

Evaluating the Calibration of SN Ia Anchor Datasets with a Bayesian Hierarchical Model

Miles Currie, David Rubin, Greg Aldering +3

Inter-survey calibration remains an important systematic uncertainty in cosmological studies using type Ia supernova (SNe Ia). Ideally, each survey would measure its system through…

astro-ph.GA2019

The Massive and Distant Clusters of WISE Survey VI: Stellar Mass Fractions of a Sample of High-Redshift Infrared-selected Clusters

Bandon Decker, Mark Brodwin, Zubair Abdulla +17

We present measurements of the stellar mass fractions () for a sample of high-redshift () infrared-selected galaxy clusters from the Massive and Dista…

astro-ph.CO2025

DESI Peculiar Velocity Survey -- Fundamental Plane

Khaled Said, Cullan Howlett, Tamara Davis +52

The Dark Energy Spectroscopic Instrument (DESI) Peculiar Velocity Survey aims to measure the peculiar velocities of early and late type galaxies within the DESI footprint using bot…

astro-ph2007

SN 2005ap: A Most Brilliant Explosion

Robert M. Quimby, Greg Aldering, J. Craig Wheeler +3

We present unfiltered photometric observations with ROTSE-III and optical spectroscopic follow-up with the HET and Keck of the most luminous supernova yet identified, SN 2005ap. Th…

astro-ph.CO2026

A Natural Telescope: Discovery of the Strongly Lensed Type II SN 2025mkn at

Cameron Lemon, Ariel Goobar, Joel Johansson +90

We present the discovery of SN 2025mkn, a gravitationally lensed Type II supernova. First detected as a blue transient in ZTF, 0.83 from a elliptical gala…

astro-ph2007

The Subaru/XMM-Newton Deep Survey (SXDS) - V. Optically Faint Variable Object Survey

Tomoki Morokuma, Mamoru Doi, Naoki Yasuda +19

We present our survey for optically faint variable objects using multi-epoch (8-10 epochs over 2-4 years) -band imaging data obtained with Subaru Suprime-Cam over 0.918 deg