KOMPSTAT :KOMPSAT-3 is an optical high-resolution Korean observation mission of KARI (Korea Aerospace Research Institute). The project was started in 2004. The objective is to provide observation continuity from the KOMPSAT-1 and KOMPSAT-2 missions to meet the nation's needs for high-resolution optical imagery required for GIS (Geographical Information Systems) and other environmental, agricultural and oceanographic monitoring applications. KOMPSTAT/AEISS3 :AEISS (Advanced Earth Imaging Sensor System), on board KOMPSTAT-3, is a high-resolution pushbroom imager (Pan and MS) for land applications of cartography and disaster monitoring.id:KOMPSTAT/AEISS3.a |
| KOMPSTAT/AEISS3.Blue | 4855.58 | 4876.73 | 4834.91 | 4310.26 | 5409.09 | 783.40 | 4061.26 | 5.16e-9 | KOMPSTAT | AEISS | KOMPSTAT-3 AEISS Blue normalized spectral response | | KOMPSTAT/AEISS3.Green | 5553.40 | 5572.20 | 5534.81 | 5003.72 | 6192.00 | 859.30 | 3576.41 | 3.48e-9 | KOMPSTAT | AEISS | KOMPSTAT-3 AEISS Green normalized spectral response | | KOMPSTAT/AEISS3.Red | 6692.29 | 6702.67 | 6682.14 | 6171.43 | 7100.00 | 596.50 | 2914.31 | 1.95e-9 | KOMPSTAT | AEISS | KOMPSTAT-3 AEISS Red normalized spectral response | | KOMPSTAT/AEISS3.Pan | 6381.50 | 6818.26 | 5959.96 | 4247.33 | 9300.60 | 4217.50 | 3283.31 | 2.42e-9 | KOMPSTAT | AEISS | KOMPSTAT-3 AEISS Panchromatic normalized spectral response | | KOMPSTAT/AEISS3.NIR | 8361.15 | 8406.71 | 8329.29 | 7347.06 | 9397.00 | 1619.20 | 2348.80 | 1.01e-9 | KOMPSTAT | AEISS | KOMPSTAT-3 AEISS NIR normalized spectral response |
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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}
