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SPIDER :Suborbital Polarimeter for Inflation Dust and the Epoch of Reionization (SPIDER) is a balloon-borne millimeter-wave polarimeter specifically designed to scan the cosmic microwave back- ground (CMB
SPIDER/SPIDER :Spider bands

SPIDER/SPIDER.280GHz1.38e+71.38e+79.1e+61.33e+79.25e+6-2.56e+40.01131.76e-21SPIDERSPIDERSPIDER 280GHz band
SPIDER/SPIDER.150GHz2.54e+72.54e+71.66e+72.53e+71.66e+7-3.58e+40.003311.54e-22SPIDERSPIDERSPIDER 150GHz band
SPIDER/SPIDER.90GHz4.23e+74.23e+72.58e+74.14e+72.61e+7-1.27e+50.001322.2e-23SPIDERSPIDERSPIDER 90GHz band
 

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If your research benefits from the use of the SVO Filter Profile Service, we would appreciate if you could include the following acknowledgement in your publication:

This research has made use of the Spanish Virtual Observatory (https://svo.cab.inta-csic.es) project funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00

and we would appreciate if you could include the following references in your publication: