Filter Profile Service
Carlos Rodrigo
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Grant PID2020-112494GBI00 funded by
Astronomy (7905)Planetary science (616)Earth Obs. (2452)


TopHat :The TopHat experiment was designed to measure the anisotropy in the cosmic microwave background radiation on angular scales from 0.3d to 30d and the thermal emission from both Galactic and extragalactic dust. The balloon-borne instrument had five spectral bands spanning frequencies from 175 to 630 GHz.
TopHat/TopHat :TopHat passbandsid:TopHat/TopHat.a

TopHat/TopHat.Band54.89e+64.98e+64.76e+63.75e+67.6e+6982528.090.01561.95e-20TopHatTopHatTopHat Band 5 normalized transmission
TopHat/TopHat.Band46.61e+66.67e+66.5e+64.83e+68.16e+61.03e+60.008275.67e-21TopHatTopHatTopHat Band 4 normalized transmission
TopHat/TopHat.Band37.61e+67.7e+67.47e+65.73e+61.12e+71.3e+60.006243.23e-21TopHatTopHatTopHat Band 3 normalized transmission
TopHat/TopHat.Band21.38e+71.45e+71.28e+78.16e+62.71e+73.32e+60.002043.21e-22TopHatTopHatTopHat Band 2 normalized transmission
TopHat/TopHat.Band11.88e+71.93e+71.8e+71.36e+72.77e+75.33e+60.001038.76e-23TopHatTopHatTopHat Band 1 normalized transmission
 

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This research has made use of the SVO Filter Profile Service "Carlos Rodrigo", funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00

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