activity
20092022
most citedDark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

1.2k citations · 12.8k across the 105 of their papers we have counts for

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Showing astro-ph.IMShow all

11 papers · 1 filter

astro-ph.IM2022★ 77 cited

The DECam Local Volume Exploration Survey Data Release 2

A. Drlica-Wagner, P. S. Ferguson, M. Adamów +121

We present the second public data release (DR2) from the DECam Local Volume Exploration survey (DELVE). DELVE DR2 combines new DECam observations with archival DECam data from the…

astro-ph.IM2022★ 2 cited

Testing low-loss microstrip materials with MKIDs for microwave applications

J. Hood, P. Barry, T. Cecil +6

Future measurements of the millimeter-wavelength sky require a low-loss superconducting microstrip, typically made from niobium and silicon-nitride, coupling the antenna to detecto…

astro-ph.IM2021

Design of SPT-SLIM focal plane; a spectroscopic imaging array for the South Pole Telescope

P. S. Barry, A. Anderson, B. Benson +15

The Summertime Line Intensity Mapper (SLIM) is a mm-wave line-intensity mapping (mm-LIM) experiment for the South Pole Telescope (SPT). The goal of SPT-SLIM is to serve as a techni…

astro-ph.IM2021★ 34 cited

SPT-SLIM: A Line Intensity Mapping Pathfinder for the South Pole Telescope

K. S. Karkare, A. J. Anderson, P. S. Barry +15

The South Pole Telescope Summertime Line Intensity Mapper (SPT-SLIM) is a pathfinder experiment that will demonstrate the use of on-chip filter-bank spectrometers for mm-wave line…

astro-ph.IM2021

The Design and Integrated Performance of SPT-3G

J. A. Sobrin, A. J. Anderson, A. N. Bender +120

SPT-3G is the third survey receiver operating on the South Pole Telescope dedicated to high-resolution observations of the cosmic microwave background (CMB). Sensitive measurements…

astro-ph.IM2020★ 82 cited

Dark Energy Survey Year 3 Results: Point-Spread Function Modeling

M. Jarvis, G. M. Bernstein, A. Amon +79

We introduce a new software package for modeling the point-spread function (PSF) of astronomical images, called Piff (PSFs In the Full FOV), which we apply to the first three years…

astro-ph.IM2015★ 189 cited

The DES Science Verification Weak Lensing Shear Catalogues

M. Jarvis, E. Sheldon, J. Zuntz +92

We present weak lensing shear catalogues for 139 square degrees of data taken during the Science Verification (SV) time for the new Dark Energy Camera (DECam) being used for the Da…

astro-ph.IM2014★ 47 cited

Modelling the Transfer Function for the Dark Energy Survey

C. Chang, M. T. Busha, R. H. Wechsler +40

We present a forward-modelling simulation framework designed to model the data products from the Dark Energy Survey (DES). This forward-model process can be thought of as a transfe…

astro-ph.IM2014★ 325 cited

SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope

B. A. Benson, P. A. R. Ade, Z. Ahmed +61

We describe the design of a new polarization sensitive receiver, SPT-3G, for the 10-meter South Pole Telescope (SPT). The SPT-3G receiver will deliver a factor of ~20 improvement i…

astro-ph.IM2013★ 10 cited

A Study of Al-Mn Transition Edge Sensor Engineering for Stability

E. M. George, J. E. Austermann, J. A. Beall +32

The stability of Al-Mn transition edge sensor (TES) bolometers is studied as we vary the engineered TES transition, heat capacity, and/or coupling between the heat capacity and TES…

astro-ph.IM2009★ 694 cited

The 10 Meter South Pole Telescope

J. E. Carlstrom, P. A. R. Ade, K. A. Aird +41

The South Pole Telescope (SPT) is a 10 m diameter, wide-field, offset Gregorian telescope with a 966-pixel, multi-color, millimeter-wave, bolometer camera. It is located at the Amu…