AKARI :AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI/IRC :AKARI Infrared Camera id:AKARI/IRC.a |
| AKARI/IRC.N2 | 23550.41 | 24106.09 | 22682.79 | 16799.51 | 29496.94 | 6973.78 | 589.12 | 3.18e-11 | AKARI | IRC | IRC NIR N2 | | AKARI/IRC.N3 | 32179.03 | 32761.46 | 31299.86 | 25370.24 | 39869.70 | 8605.39 | 335.19 | 9.7e-12 | AKARI | IRC | IRC NIR N3 | | AKARI/IRC.N4 | 43830.10 | 44703.96 | 42505.84 | 33990.71 | 57514.48 | 15279.14 | 190.95 | 2.98e-12 | AKARI | IRC | IRC NIR N4 | | AKARI/IRC.S7 | 71763.59 | 73059.12 | 69537.99 | 55235.69 | 87425.96 | 17325.82 | 75.20 | 4.38e-13 | AKARI | IRC | IRC MIR-S S7 | | AKARI/IRC.S9W | 88508.56 | 92181.96 | 82281.47 | 58460.61 | 121879.82 | 41027.14 | 53.49 | 2.05e-13 | AKARI | IRC | IRC MIR-S S9W | | AKARI/IRC.S11 | 106378.81 | 109489.17 | 101905.34 | 82698.24 | 152992.79 | 41042.69 | 35.71 | 9.46e-14 | AKARI | IRC | IRC MIR-S S11 | | AKARI/IRC.L15 | 158029.96 | 161620.40 | 152145.36 | 122114.20 | 214681.41 | 59787.68 | 16.28 | 1.95e-14 | AKARI | IRC | IRC MIR-L L15 | | AKARI/IRC.L18W | 189217.77 | 198065.57 | 176079.23 | 136082.25 | 286690.68 | 99690.53 | 12.05 | 1.01e-14 | AKARI | IRC | IRC MIR-L L18W | | AKARI/IRC.L24 | 231201.08 | 233524.38 | 227526.47 | 184025.14 | 287036.54 | 53337.74 | 7.39 | 4.15e-15 | AKARI | IRC | IRC MIR-L L24 |
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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}
