activity
20102026
most citedUnified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing

20 citations · 91 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

12 papers · 1 filter

astro-ph.IM2026

The SPT-3G+ receiver design

H. Athreya, Z. Ahmed, J. E. Austermann +71

We present the thermo-mechanical design of the cryostat and camera optics for SPT-3G+, a new receiver being developed for the South Pole Telescope (SPT). The receiver consists of 1…

astro-ph.IM2026

Map Multi-Tool: A Map-Based Approach to Modeling Beam Systematics for Cosmic Microwave Background Experiments

Cesiley L. King, Alec Hryciuk, Jeff McMahon +2

Cosmic microwave background (CMB) experiments use simulations of instrumental systematic effects to ensure high-fidelity measurements of cosmological parameters. Quantifying the ex…

astro-ph.IM2026

picoMUX: microcontroller based time-domain multiplexing readout for kilopixel TES arrays

Simon Tartakovsky, Alexandre E. Adler, Jason E. Austermann +23

Advances in cryogenic SQUID-based time-domain multiplexing (TDM) have outpaced their warm readout electronics. Next generation CMB telescopes are baselining kilopixel TES arrays wi…

astro-ph.IM2026

Sub-Kelvin Cryogenics for a Super-Pressure Balloon-Borne CMB Polarimeter: Taurus

Jared L. May, Alexandre E. Adler, Jason E. Austermann +23

Taurus is a balloon-borne cosmic microwave background (CMB) experiment designed to operate more than 10,000 transition-edge sensor bolometers at a base temperature near 100 mK duri…

astro-ph.IM2024★ 1 cited

In-Flight Performance of Spider's 280 GHz Receivers

Elle C. Shaw, P. A. R. Ade, S. Akers +84

SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky…

astro-ph.IM2024

Overview of the Optical Design of the CMB-S4 Large Aperture Telescopes and Camera Optics

Patricio A. Gallardo, Kathleen Harrington, Roberto Puddu +8

CMB-S4, the next-generation CMB observatory, will deploy hundreds of thousands of detectors to enable mapping the millimeter-wavelength sky with unprecedented speed. The large aper…

astro-ph.IM2023★ 7 cited

Freeform three-mirror anastigmatic large-aperture telescope and receiver optics for CMB-S4

Patricio A. Gallardo, Roberto Puddu, Kathleen Harrington +14

CMB-S4, the next-generation ground-based cosmic microwave background (CMB) observatory, will provide detailed maps of the CMB at millimeter wavelengths to dramatically advance our…

astro-ph.IM2022★ 5 cited

Conceptual Design of the Modular Detector and Readout System for the CMB-S4 survey experiment

D. R. Barron, Z. Ahmed, J. Aguilar +47

We present the conceptual design of the modular detector and readout system for the Cosmic Microwave Background Stage 4 (CMB-S4) ground-based survey experiment. CMB-S4 will map the…

astro-ph.IM2018★ 15 cited

Design and characterization of the SPT-3G receiver

J. A. Sobrin, P. A. R. Ade, Z. Ahmed +68

The SPT-3G receiver was commissioned in early 2017 on the 10-meter South Pole Telescope (SPT) to map anisotropies in the cosmic microwave background (CMB). New optics, detector, an…

astro-ph.IM2018★ 10 cited

Broadband anti-reflective coatings for cosmic microwave background experiments

A. Nadolski, A. M. Kofman, J. D. Vieira +71

The desire for higher sensitivity has driven ground-based cosmic microwave background (CMB) experiments to employ ever larger focal planes, which in turn require larger reimaging o…

astro-ph.IM2014★ 14 cited

Pointing control for the SPIDER balloon-borne telescope

Jamil A. Shariff, Peter A. R. Ade, Mandana Amiri +45

We present the technology and control methods developed for the pointing system of the SPIDER experiment. SPIDER is a balloon-borne polarimeter designed to detect the imprint of pr…

astro-ph.IM2010★ 19 cited

Modeling and characterization of the SPIDER half-wave plate

Sean A. Bryan, Peter A. R. Ade, Mandana Amiri +42

Spider is a balloon-borne array of six telescopes that will observe the Cosmic Microwave Background. The 2624 antenna-coupled bolometers in the instrument will make a polarization…