IRTF :NASA Infrared Telescope Facility (IRTF) IRTF/MORIS :MIT Optical Rapid Imaging System (MORIS) is a facility science camera used for observing on the IRTF. This high-speed, visible wavelength camera is mounted on the side window of SpeX, a near-IR imager and spectrograph.id:IRTF/MORIS.a → GaiaXPy base XML file. You can download here the GaiaXPy base XML file for the full IRTF/MORIS filter set. Please, take a look to the GaiaXPy web page and additional documentation for more information. |
| IRTF/MORIS.g | 2612.14 | 2799.10 | 2682.35 | 1371.93 | 3750.28 | 1331.00 | 911.41 | 4.0e-9 | IRTF | MORIS | MORIS g filter | | IRTF/MORIS.V | 3384.51 | 3471.68 | 3587.73 | 2537.94 | 4890.00 | 1302.73 | 1656.70 | 4.34e-9 | IRTF | MORIS | MORIS V filter | | IRTF/MORIS.VR | 4110.96 | 4352.88 | 4367.27 | 2564.12 | 5899.24 | 2288.50 | 2732.79 | 4.85e-9 | IRTF | MORIS | MORIS VR filter | | IRTF/MORIS.r | 4552.40 | 4653.88 | 4569.05 | 3404.61 | 5827.42 | 1669.60 | 3693.02 | 5.34e-9 | IRTF | MORIS | MORIS r filter | | IRTF/MORIS.Dichr_800nm | 4085.09 | 5141.16 | 4582.74 | 1082.42 | 9993.00 | 4263.69 | 2087.92 | 3.75e-9 | IRTF | MORIS | MORIS 0.8mic dichroic | | IRTF/MORIS.Dichr_950nm | 4465.52 | 5747.55 | 4854.58 | 1084.18 | 9993.00 | 5447.01 | 2120.44 | 3.19e-9 | IRTF | MORIS | MORIS 0.95mic dichroic | | IRTF/MORIS.OG590 | 6090.02 | 6507.84 | 5713.20 | 3907.54 | 9827.00 | 4225.12 | 3373.11 | 2.73e-9 | IRTF | MORIS | MORIS OG590 filter | | IRTF/MORIS.i | 6587.05 | 6660.29 | 6509.64 | 5434.47 | 7921.58 | 1896.75 | 2993.55 | 2.07e-9 | IRTF | MORIS | MORIS i filter | | IRTF/MORIS.z | 8249.06 | 8286.92 | 8220.53 | 7452.43 | 10032.00 | 1128.97 | 2347.89 | 1.03e-9 | IRTF | MORIS | MORIS z filter |
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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}
