activity
19952023
most citedMeasurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35

1.6k citations · 13.8k across the 142 of their papers we have counts for

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20 papers · 1 filter

astro-ph.IM2023

Fast and efficient identification of anomalous galaxy spectra with neural density estimation

Vanessa Böhm, Alex G. Kim, Stéphanie Juneau

Current large-scale astrophysical experiments produce unprecedented amounts of rich and diverse data. This creates a growing need for fast and flexible automated data inspection me…

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-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.IM2020★ 11 cited

Optimising a magnitude-limited spectroscopic training sample for photometric classification of supernovae

Jonathan E. Carrick, Isobel M. Hook, Elizabeth Swann +4

In preparation for photometric classification of transients from the Legacy Survey of Space and Time (LSST) we run tests with different training data sets. Using estimates of the d…

astro-ph.IM2019★ 18 cited

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.IM2019★ 13 cited

Enabling catalog simulations of transient and variable sources based on LSST cadence strategies

Rahul Biswas, Scott F. Daniel, R. Hložek +2

The Large Synoptic Survey Telescope (LSST) project will conduct a ten year multi-band survey starting in 2022. Observing strategies for this survey are being actively investigated,…

astro-ph.IM2019★ 1 cited

ASTRO2020 White Paper: JWST: Probing the Epoch of Reionization with a Wide Field Time-Domain Survey

L. Wang, J. Mould, D. Baade +29

A major scientific goal of JWST is to probe the epoch of re-ionization of the Universe at z above 6, and up to 20 and beyond. At these redshifts, galaxies are just beginning to for…

astro-ph.IM2019★ 4 cited

Direct Acceleration: Cosmic and Exoplanet Synergies

David Erskine, Alex Kim, Eric Linder +10

Direct measurement of acceleration is a key scientific goal for both cosmology and exoplanets. For cosmology, the concept of redshift drift (more than 60 years old by the 2020s) co…

astro-ph.IM2018★ 13 cited

Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Wide-Fast-Deep Survey

Michelle Lochner, Daniel M. Scolnic, Humna Awan +33

Cosmology is one of the four science pillars of LSST, which promises to be transformative for our understanding of dark energy and dark matter. The LSST Dark Energy Science Collabo…

astro-ph.IM2018★ 3 cited

LSST Observing Strategy White Paper: LSST Observations of WFIRST Deep Fields

R. J. Foley, A. M. Koekemoer, D. N. Spergel +38

The Wide-Field Infrared Survey Telescope (WFIRST) is expected to launch in the mid-2020s. With its wide-field near-infrared (NIR) camera, it will survey the sky to unprecedented de…

astro-ph.IM2018★ 93 cited

First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release

D. Brout, M. Sako, D. Scolnic +89

We present griz light curves of 251 Type Ia Supernovae (SNe Ia) from the first 3 years of the Dark Energy Survey Supernova Program's (DES-SN) spectroscopically classified sample. T…

astro-ph.IM2017

Science-Driven Optimization of the LSST Observing Strategy

LSST Science Collaboration, Phil Marshall, Timo Anguita +102

The Large Synoptic Survey Telescope is designed to provide an unprecedented optical imaging dataset that will support investigations of our Solar System, Galaxy and Universe, acros…

astro-ph.IM2017★ 10 cited

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.IM2016★ 236 cited

The DESI Experiment Part II: Instrument Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…

astro-ph.IM2016★ 1.3k cited

The DESI Experiment Part I: Science,Targeting, and Survey Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…

astro-ph.IM2015★ 208 cited

redMaGiC: Selecting Luminous Red Galaxies from the DES Science Verification Data

E. Rozo, E. S. Rykoff, A. Abate +84

We introduce redMaGiC, an automated algorithm for selecting Luminous Red Galaxies (LRGs). The algorithm was specifically developed to minimize photometric redshift uncertainties in…

astro-ph.IM2015★ 155 cited

Automated Transient Identification in the Dark Energy Survey

D. A. Goldstein, C. B. D'Andrea, J. A. Fischer +64

We describe an algorithm for identifying point-source transients and moving objects on reference-subtracted optical images containing artifacts of processing and instrumentation. T…

astro-ph.IM2014★ 180 cited

Photometric redshift analysis in the Dark Energy Survey Science Verification data

C. Sánchez, M. Carrasco Kind, H. Lin +74

We present results from a study of the photometric redshift performance of the Dark Energy Survey (DES), using the early data from a Science Verification (SV) period of observation…

astro-ph.IM2012

Dithering Strategies and Point-Source Photometry

Johan Samsing, Alex G. Kim

The accuracy in the photometry of a point source depends on the point-spread function (PSF), detector pixelization, and observing strategy. The PSF and pixel response describe the…

astro-ph.IM2011★ 6 cited

Science Yield of an Improved Wide Field Infrared Survey Telescope (WFIRST)

Michael E. Levi, Alex G. Kim, Michael L. Lampton +1

The Astronomy and Astrophysics Decadal Survey's highest recommended space mission was a Wide-Field Infrared Survey Telescope (WFIRST) to efficiently conduct three kinds of studies:…