Selene :Kaguya, originally named SELENE (Selenological and Engineering Explorer) was Japan's second mission to Explore the Moon from orbit. Selene/MI :The Multiband Imager (MI) is a high-resolution, multi-spectral imaging instru- ment for lunar exploration. It consists of two cameras, VIS and NIR, and is carried on the SELenological and ENgineering Explorer (SELENE), launched on Sep. 14, 2007id:Selene/MI.a |
| Selene/MI.VIS1 | 4142.45 | 4144.14 | 4144.87 | 3929.05 | 4369.21 | 196.51 | 4255.61 | 7.43e-9 | Selene | MI | SELENE MI VIS1 band | | Selene/MI.VIS2 | 7490.80 | 7491.38 | 7490.17 | 7305.98 | 7692.35 | 129.42 | 2582.80 | 1.38e-9 | Selene | MI | SELENE MI VIS2 band | | Selene/MI.VIS3 | 9009.77 | 9010.71 | 9009.57 | 8771.63 | 9238.78 | 214.49 | 2286.54 | 8.44e-10 | Selene | MI | SELENE MI VIS3 band | | Selene/MI.VIS4 | 9501.86 | 9503.68 | 9498.17 | 9173.62 | 9848.22 | 314.40 | 2203.21 | 7.32e-10 | Selene | MI | SELENE MI VIS4 band | | Selene/MI.NIR1 | 10012.35 | 10013.36 | 10009.14 | 9818.11 | 10192.31 | 268.35 | 2050.41 | 6.13e-10 | Selene | MI | SELENE MI NIR1 band | | Selene/MI.VIS5 | 10013.99 | 10017.14 | 10008.83 | 9583.65 | 10479.26 | 437.66 | 2088.79 | 6.24e-10 | Selene | MI | SELENE MI VIS5 band | | Selene/MI.NIR2 | 10482.62 | 10483.77 | 10481.07 | 10205.73 | 10768.00 | 280.03 | 2013.43 | 5.49e-10 | Selene | MI | SELENE MI NIR2 band | | Selene/MI.NIR3 | 12484.27 | 12485.49 | 12482.51 | 12244.51 | 12744.12 | 324.13 | 1545.44 | 2.97e-10 | Selene | MI | SELENE MI NIR3 band | | Selene/MI.NIR4 | 15474.77 | 15476.83 | 15471.29 | 15134.55 | 15831.96 | 463.67 | 1099.37 | 1.38e-10 | Selene | MI | SELENE MI NIR4 band |
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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}
