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 |
| AKARI/IRC.N2 | 23550.40 | 24106.08 | 22684.35 | 16799.51 | 29496.94 | 6973.78 | 559.84 | 3.26e-11 | AKARI | IRC | IRC NIR N2 | | AKARI/IRC.N3 | 32178.85 | 32761.32 | 31302.69 | 25370.24 | 39869.70 | 8605.42 | 325.50 | 9.96e-12 | AKARI | IRC | IRC NIR N3 | | AKARI/IRC.N4 | 43830.13 | 44703.98 | 42505.24 | 33990.71 | 57514.48 | 15278.93 | 184.40 | 3.06e-12 | AKARI | IRC | IRC NIR N4 | | AKARI/IRC.S7 | 71763.54 | 73059.08 | 69538.96 | 55235.69 | 87425.96 | 17325.83 | 72.54 | 4.5e-13 | AKARI | IRC | IRC MIR-S S7 | | AKARI/IRC.S9W | 88508.48 | 92181.96 | 82283.55 | 58460.61 | 121879.82 | 41027.11 | 47.51 | 2.1e-13 | AKARI | IRC | IRC MIR-S S9W | | AKARI/IRC.S11 | 106378.80 | 109489.15 | 101932.12 | 82698.24 | 152992.79 | 41042.64 | 33.73 | 9.73e-14 | AKARI | IRC | IRC MIR-S S11 | | AKARI/IRC.L15 | 158029.99 | 161620.41 | 152310.49 | 122114.20 | 214681.41 | 59787.65 | 15.54 | 2.01e-14 | AKARI | IRC | IRC MIR-L L15 | | AKARI/IRC.L18W | 189217.99 | 198065.72 | 176094.90 | 136082.25 | 286690.68 | 99690.07 | 10.73 | 1.04e-14 | AKARI | IRC | IRC MIR-L L18W | | AKARI/IRC.L24 | 231201.06 | 233524.36 | 227526.39 | 184025.14 | 287036.54 | 53337.79 | 7.36 | 4.26e-15 | AKARI | IRC | IRC MIR-L L24 |
|
| 
 ≡ filter transmission<p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl<li><b>Utype</b>: <i>photdm:PhotometryFilter.SpectralAxis.Coverage.Location.Value</i></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.SpectralAxis.Coverage.Bounds.Extent</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}
