Subaru :Subaru Telescope Subaru/OHS :OHS helps the detection of faint astronomical objects at near-infrared wavelength by removing background light caused by OH molecules in the Earth’s upper atmosphere. |
| Subaru/OHS.z | 10213.5 | 10115.9 | 9184 | 11283 | 1775.5 | 2068.2 | Subaru | OHS | OHS z filter | | Subaru/OHS.J | 12484.1 | 12417.4 | 11482 | 13495 | 1516.7 | 1562.2 | Subaru | OHS | OHS J filter | | Subaru/OHS.H | 16298.3 | 16141.1 | 14510 | 18091 | 2845.7 | 1045.9 | Subaru | OHS | OHS H filter | | Subaru/OHS.N204 | 20331.2 | 20330.3 | 20130 | 20544 | 206.0 | 745.2 | Subaru | OHS | OHS N204 filter | | Subaru/OHS.Kp | 21125.2 | 20941.5 | 19018 | 23235 | 3401.9 | 693.7 | Subaru | OHS | OHS K' filter | | Subaru/OHS.H210 | 21198.1 | 21197.1 | 20981 | 21418 | 207.8 | 691.8 | Subaru | OHS | OHS H2 1-0 filter | | Subaru/OHS.N215 | 21468.9 | 21467.4 | 21257 | 21683 | 216.6 | 672.6 | Subaru | OHS | OHS N215 filter | | Subaru/OHS.K | 22005.4 | 21840.4 | 19859 | 24015 | 3242.3 | 647.7 | Subaru | OHS | OHS K filter | | Subaru/OHS.H221 | 22502.4 | 22501.4 | 22277 | 22725 | 218.7 | 623.6 | Subaru | OHS | OHS H2 2-1 filter |
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© SVO, 6376 filters available, Last update: 2020-08-12 | 
 ≡ 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>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}
</b><br><table cellpadding=20><td class=helptd>Zero Point in Vega System.<p>Calculated by the service as:<p><img src=images/latex/zp.png> <p>where:<p> T(λ) ≡ filter transmission<br> Vg(λ) ≡ Vega spectrum<p>F<sub>0,ν</sub>(Jy) = (2.9979246)<sup>-1</sup> 10<sup>5</sup> * λ<sub>eff</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}