activity
20082026
most citedThe Atacama Cosmology Telescope: The Receiver and Instrumentation

265 citations · 974 across the 25 of their papers we have counts for

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Showing astro-ph.IMShow all

12 papers · 1 filter

astro-ph.IM2026

BICEP/Keck XXII: Analysis of the South Pole Atmosphere for CMB Observations

P. A. R. Ade, Z. Ahmed, M. Amiri +92

The South Pole is among the driest sites on Earth, and the resulting high atmospheric transparency makes it an excellent site for millimeter-wave astronomical observations. Neverth…

astro-ph.IM2026

Status of BICEP Array and Integration of the 220/270 GHz Receiver

A. Steiger, P. A. R. Ade, Z. Ahmed +83

Measurements of the polarization of the cosmic microwave background are critical for modern cosmology as they constrain the physics of the early universe and cosmic inflation. BICE…

astro-ph.IM2026

Engineering of titanium transition edge sensor wafers for the BA4-90/150 receiver of BICEP Array

A. Patel, P. A. R. Ade, Z. Ahmed +83

BA4-90/150, the fourth receiver to be deployed in the BICEP Array (BA) series, is a dichroic 90/150 GHz instrument targeting the frequency space where sensitivity to the CMB polari…

astro-ph.IM2026

Advanced Time-Division Multiplexed Readout Chain for the BICEP Array 90/150 GHz Receiver

B. Cantrall, P. A. R. Ade, Z. Ahmed +89

This work presents the current performance of the advanced time-division multiplexed (TDM) readout chain for the BICEP Array 90/150 GHz receiver. BA4-90/150, scheduled for deployme…

astro-ph.IM2026

Overview and status of BICEP Array's BA4-90/150 CMB polarimeter

M. A. Petroff, P. A. R. Ade, Z. Ahmed +83

The inflation paradigm postulates a period of rapid expansion in the early Universe, which would generate gravitational waves. These tensor perturbations would produce a faint B-mo…

astro-ph.IM2024★ 2 cited

Superfluid-tight cryogenic receiver with continuous sub-Kelvin cooling for EXCLAIM

Sumit Dahal, Peter A. R. Ade, Christopher J. Anderson +67

The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) is a balloon-borne telescope designed to survey star formation over cosmological time scales using intensity…

astro-ph.IM2023★ 1 cited

Optimization of an Optical Testbed for Characterization of EXCLAIM u-Spec Integrated Spectrometers

Maryam Rahmani, Emily M. Barrentine, Eric R. Switzer +19

We describe a testbed to characterize the optical response of compact superconducting on-chip spectrometers in development for the Experiment for Cryogenic Large-Aperture Intensity…

astro-ph.IM2021★ 1 cited

In-flight gain monitoring of SPIDER's transition-edge sensor arrays

J. P. Filippini, A. E. Gambrel, A. S. Rahlin +67

Experiments deploying large arrays of transition-edge sensors (TESs) often require a robust method to monitor gain variations with minimal loss of observing time. We propose a sens…

astro-ph.IM2020★ 10 cited

Optical Design of the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)

Thomas Essinger-Hileman, Danny Chmaytelli, Trevor Oxholm +23

This work describes the design and implementation of optics for EXCLAIM, the EXperiment for Cryogenic Large-Aperture Intensity Mapping. EXCLAIM is a balloon-borne telescope that wi…

astro-ph.IM2017★ 43 cited

Exploring Cosmic Origins with CORE: The Instrument

P. de Bernardis, P. A. R. Ade, J. J. A. Baselmans +126

We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is…

astro-ph.IM2016★ 25 cited

BICEP2 / Keck Array VII: Matrix based E/B Separation applied to BICEP2 and the Keck Array

Keck Array, BICEP2 Collaborations, : +63

A linear polarization field on the sphere can be uniquely decomposed into an E-mode and a B-mode component. These two components are analytically defined in terms of spin-2 spheric…

astro-ph.IM2010★ 265 cited

The Atacama Cosmology Telescope: The Receiver and Instrumentation

D. S. Swetz, P. A. R. Ade, M. Amiri +38

The Atacama Cosmology Telescope was designed to measure small-scale anisotropies in the Cosmic Microwave Background and detect galaxy clusters through the Sunyaev-Zel'dovich effect…