WHT :William Herschel Telescope WHT/LRIS :LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph) is a near-IR imager/spectrograph for use at the Cassegrain focus of the 4.2m William Herschel Telescope. |
| WHT/LRIS.Z | 10329.75 | 10334.30 | 10326.43 | 9697.60 | 10926.72 | 507.09 | 2063.74 | 5.8e-10 | WHT | LRIS | LRIS Z | | WHT/LRIS.Jc | 12312.11 | 12312.69 | 12311.32 | 12112.00 | 12596.40 | 186.66 | 1608.30 | 3.18e-10 | WHT | LRIS | LRIS Jc | | WHT/LRIS.J | 12488.25 | 12516.58 | 12447.42 | 11010.00 | 13995.00 | 1544.37 | 1556.60 | 3.01e-10 | WHT | LRIS | LRIS J | | WHT/LRIS.Pab | 12945.35 | 12946.01 | 12946.57 | 12711.40 | 13195.80 | 211.29 | 1456.73 | 2.61e-10 | WHT | LRIS | LRIS Pab | | WHT/LRIS.Hc | 15773.52 | 15774.75 | 15771.67 | 15214.00 | 16398.10 | 243.85 | 1082.31 | 1.3e-10 | WHT | LRIS | LRIS Hc | | WHT/LRIS.H | 16189.15 | 16262.19 | 16093.91 | 14097.30 | 18198.20 | 2828.81 | 1049.01 | 1.21e-10 | WHT | LRIS | LRIS H | | WHT/LRIS.FeII | 16467.57 | 16468.61 | 16468.37 | 16013.00 | 16994.90 | 270.31 | 1016.57 | 1.12e-10 | WHT | LRIS | LRIS FeII | | WHT/LRIS.CH4 | 16823.29 | 16843.06 | 16797.44 | 15177.12 | 18496.70 | 1376.28 | 993.64 | 1.06e-10 | WHT | LRIS | LRIS CH4 | | WHT/LRIS.HeI | 20612.29 | 20613.70 | 20610.16 | 20017.70 | 21192.10 | 312.60 | 727.47 | 5.13e-11 | WHT | LRIS | LRIS HeI | | WHT/LRIS.H2p10 | 21240.66 | 21242.31 | 21237.83 | 20518.30 | 21991.10 | 339.09 | 688.78 | 4.58e-11 | WHT | LRIS | LRIS H2p10 | | WHT/LRIS.Ks | 21411.65 | 21472.76 | 21319.24 | 19016.50 | 23935.70 | 3012.80 | 675.84 | 4.46e-11 | WHT | LRIS | LRIS Ks | | WHT/LRIS.Brg | 21710.45 | 21712.67 | 21708.63 | 21018.80 | 22491.70 | 360.33 | 641.26 | 4.08e-11 | WHT | LRIS | LRIS Brg | | WHT/LRIS.H2p21 | 22416.73 | 22418.51 | 22414.12 | 21712.00 | 23098.20 | 403.07 | 627.69 | 3.75e-11 | WHT | LRIS | LRIS H2p21 | | WHT/LRIS.Kc | 22671.23 | 22673.41 | 22667.99 | 22010.40 | 23396.60 | 350.30 | 615.41 | 3.59e-11 | WHT | LRIS | LRIS Kc |
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© SVO, 8400 filters available, Last update: 2020-09-01 | 
 ≡ 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}
 ≡ 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>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<br> Vg(λ) ≡ Vega spectrum<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}
