ARCHEOPS :Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (∼8') over a large fraction (∼25%) of the sky in the millimetre domain. ARCHEOPS/KS3 :ARCHEOPS performance during its third science flight in 2002 from Kiruna (Sweden) for a 24-h flight from which 12 night hours were exploited for scientific purposes.id:ARCHEOPS/KS3.a |
| ARCHEOPS/KS3.545GHz | 5.73e+6 | 5.88e+6 | 5.52e+6 | 4.34e+6 | 8.3e+6 | 2.05e+6 | 0.0114 | 1.04e-20 | ARCHEOPS | ARCHEOPS | ARCHEOPS 545GHz filter response at KS3 flight | | ARCHEOPS/KS3.353GHz | 8.31e+6 | 8.43e+6 | 8.13e+6 | 6.62e+6 | 1.13e+7 | 2.31e+6 | 0.00524 | 2.27e-21 | ARCHEOPS | ARCHEOPS | ARCHEOPS 353GHz filter response at KS3 flight | | ARCHEOPS/KS3.217GHz | 1.35e+7 | 1.36e+7 | 1.32e+7 | 1.03e+7 | 1.56e+7 | 3.62e+6 | 0.00195 | 3.22e-22 | ARCHEOPS | ARCHEOPS | ARCHEOPS 217GHz filter response at KS3 flight | | ARCHEOPS/KS3.143GHz | 2.05e+7 | 2.07e+7 | 2.01e+7 | 1.6e+7 | 2.38e+7 | 5.52e+6 | 0.00083 | 5.93e-23 | ARCHEOPS | ARCHEOPS | ARCHEOPS 143GHz filter response at KS3 flight |
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 ≡ filter transmission<p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl</ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission<br> Vg(λ) ≡ Vega spectrum.<p><u>More info:</u><p>Vega spectrum from calspec database.<ul><li><a href="https://ui.adsabs.harvard.edu/abs/2014PASP..126..711B/abstract" target="_blank">Bohlin, Gordon, & Tremblay (2014)</a>.<li><a href="https://www.stsci.edu/hst/instrumentation/reference-data-for-calibration-and-tools/astronomical-catalogs/calspec" target="_blank">STScI current calspec</a>.<li><a href="morefiles/vega.dat" target="_blank">Vega spectrum file</a> (units: Angstrom erg/cm2/s/A).</ul><p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl.effective</ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission<p>Equivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve.<p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:instr.bandwidth<li><b>Utype</b>: <i>photdm:PhotometryFilter.bandwidth.extent.value</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission (energy counter).<br> Vg(λ) ≡ Vega spectrum.<p><i>(T(λ) must be multiplied by λ for photon counting devices)</i><p>F<sub>0,ν</sub>(Jy) = (2.9979246)<sup>-1</sup> 10<sup>5</sup> * λ<sub>ref</sub><sup>2</sup> * F<sub>0,λ</sub>(erg/cm<sup>2</sup>/s/A)<p>In the case that filter owner specifies its own values, they will be the ones provided by the service when queried through the VO.<p><u>Property info:</u><ul><li><b>Unit</b>:Jy<li><b>UCD</b>:phot.flux.density<li><b>Utype</b>: <i>photdm:PhotCal.zeroPoint.flux.value</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission (energy counter).<br> Vg(λ) ≡ Vega spectrum.<p><i>(T(λ) must be multiplied by λ for photon counting devices)</i><p><u>Property info:</u><ul><li><b>Unit</b>:erg/cm2/s/A<li><b>Utype</b>: <i>PhotCal.ZeroPoint</i></ul></td></table>',WIDTH,400)){kind=link}
