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 optimized to search for a primordial B-mode polarization signature in the cosmic microwave background at degree angular scales. During its first flight in 2015, Spider mapped ~10% of the sky at 95 and 150 GHz. The payload for the second Antarctic flight will incorporate three new 280 GHz receivers alongside three refurbished 95- and 150 GHz receivers from Spider's first flight. In this work we discuss the design and characterization of these new receivers, which employ over 1500 feedhorn-coupled transition-edge sensors. We describe pre-flight laboratory measurements of de...
We describe Spider, a balloon-borne instrument to map the polarization of the millimeter-wave sky wi...
SPIDER is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Back...
Spider is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Back...
In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its secon...
International audienceSpider is a balloon-borne instrument designed to map the polarization of the m...
We present the results of integration and characterization of the Spider instrument after the 2013 p...
We describe the construction and characterization of the 280 GHz bolometric focal plane units (FPUs)...
We describe SPIDER, a balloon-borne instrument to map the polarization of the millimeter-wave sky wi...
We describe Spider, a balloon-borne instrument to map the polarization of the millimeter-wave sky wi...
SPIDER is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Back...
Spider is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Back...
In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its secon...
International audienceSpider is a balloon-borne instrument designed to map the polarization of the m...
We present the results of integration and characterization of the Spider instrument after the 2013 p...
We describe the construction and characterization of the 280 GHz bolometric focal plane units (FPUs)...
We describe SPIDER, a balloon-borne instrument to map the polarization of the millimeter-wave sky wi...
We describe Spider, a balloon-borne instrument to map the polarization of the millimeter-wave sky wi...
SPIDER is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Back...
Spider is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Back...