activity
20162024
most citedPICO: Probe of Inflation and Cosmic Origins

45 citations · 63 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

6 papers · 1 filter

astro-ph.IM20242 cited

CCAT: Nonlinear effects in 280 GHz aluminum kinetic inductance detectors

Cody J. Duell, Jason Austermann, James R. Burgoyne +22

Prime-Cam, a first-generation science instrument for the Atacama-based Fred Young Submillimeter Telescope, is being built by the CCAT Collaboration to observe at millimeter and sub…

astro-ph.IM2021

The optical design of the LiteBIRD Middle and High Frequency Telescope

L. Lamagna, J. E. Gudmundsson, H. Imada +26

LiteBIRD is a JAXA strategic L-class mission devoted to the measurement of polarization of the Cosmic Microwave Background, searching for the signature of primordial gravitational…

astro-ph.IM20205 cited

Design and pre-flight performance of SPIDER 280 GHz receivers

E. C. Shaw, P. A. R. Ade, S. Akers +79

In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimize…

astro-ph.IM2019

PICO: Probe of Inflation and Cosmic Origins

S. Hanany, M. Alvarez, E. Artis +79

The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. W…

astro-ph.IM201945 cited

PICO: Probe of Inflation and Cosmic Origins

Shaul Hanany, Marcelo Alvarez, Emmanuel Artis +79

The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce f…

astro-ph.IM2016

Optical Demonstration of THz, Dual-Polarization Sensitive Microwave Kinetic Inductance Detectors

B. Dober, J. A. Austermann, J. A. Beall +17

The next generation BLAST experiment (BLAST-TNG) is a suborbital balloon payload that seeks to map polarized dust emission in the 250 m, 350 m and 500 m wavebands. The ins…