The Primordial Inflation Polarization Explorer (PIPER): Current Status and Performance of the First Flight

Pawlyk, Samuel ; Ade, Peter A R ; Benford, Dominic ; Bennett, Charles L ; Chuss, David T ; Datta, Rahul ; Dotson, Jessie L ; Eimer, Joseph R ; Fixsen, Dale J ; Gandilo, Natalie N(Johns Hopkins Univ, Baltimore, MD, United States)

关键词: BALLOON-BORNE INSTRUMENTS;    BOLOMETERS;    CRYOGENICS;    DUST;    FREQUENCIES;    MODULATORS;    MULTIPLEXING;    PAYLOADS;    PIXELS;    SENSITIVITY;    SYSTEMS ENGINEERING;    BALLOON FLIGHT;   

RP-ID  :  GSFC-E-DAA-TN66753

学科分类：原子、分子光学和等离子物理

美国|英语

来源: NASA Technical Reports Server

【 摘 要 】

The Primordial Inflation Polarization ExploreR (PIPER) is a balloon-borne instrument optimized to measure the polarization of the CMB at large angular scales. It will map 85% of the sky over a series of conventional balloon flights from the Northern and Southern hemispheres, measuring the B-mode polarization power spectrumover a range of multipoles from 2-300 covering both the reionization bump and the recombination peak, with sensitivity to measure the tensor-to-scalar ratio down to r = 0.007. PIPER will observe in four frequency bands centered at 200, 270, 350, and 600 GHz to characterize dust foregrounds. The instrument has background-limited sensitivity provided by fully cryogenic (1.7 K) optics focusing the sky signal onto kilo-pixel arrays of time-domain multiplexed Transition-Edge Sensor (TES) bolometers held at 100 mK. Polarization sensitivity and systematiccontrol are provided by front-end Variable-delay Polarization Modulators (VPMs). PIPER had its engineering flight in October 2017 from Fort Sumner, New Mexico. This papers outlines the major components in the PIPER system discussing the conceptual design as well as specific choices made for PIPER. We also report on the results of the engineering flight, looking at the functionality of the payload systems, particularly VPM, as well as pointing out areas of improvement.