MKO :Mauna Kea Observatories MKO/MIRSI :MIRSI (Mid-InfraRed Spectrometer and Imager) is a mid-infrared camera system with both spectroscopic and imaging capabilities. id:MKO/MIRSI.a |
| MKO/MIRSI.K | 21859.43 | 21952.66 | 21721.17 | 19670.77 | 24331.32 | 3625.34 | 644.71 | 4.04e-11 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI K filter | | MKO/MIRSI.K | Filter Description | Filter ID (?) : | MKO/MIRSI.K |
| Description (?) : | Mauna kea Obsevatory. MIRSI K filter |
| Phot.System (?) : | MIRSI |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | K |
| Obs. Facility (?) : | MKO |
| Instrument (?) : | MIRSI |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
21859.43 | ------- | (Angstrom) |
| λmean (?) : |
21952.66 | ------- | (Angstrom) |
| λcen (?) : |
22004.88 | ------- | (Angstrom) |
| λeff (?) : |
21721.17 | ------- | (Angstrom) |
| λpeak (?) : |
20243.40 | ------- | (Angstrom) |
| λpivot (?) : |
21859.43 | ------- | (Angstrom) |
| λphot (?) : |
21782.35 | ------- | (Angstrom) |
| λmin (?) : |
19670.77 | ------- | (Angstrom) |
| λmax (?) : |
24331.32 | ------- | (Angstrom) |
| Weff (?) : |
3625.34 | ------- | (Angstrom) |
| FWHM (?) : |
3973.10 | ------- | (Angstrom) |
| Af/AV (?) : |
0.123 | ------- | () |
| Fsun (?) : |
8.44 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
MIRSI Transmission components: Filterid:MKO/MIRSI.K | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
4.04488e-11 | (erg/cm2/s/A) |
| |
------- |
644.71 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MKO/MIRSI.K/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
2.27808e-10 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MKO/MIRSI.K/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
57873.96 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MKO/MIRSI.K/ST |
| |
|
Filter added: 2017-07-26 22:30:49
Last update: 2021-07-27 20:18:52 | | MKO/MIRSI.4_9 | 49027.77 | 49308.19 | 48590.74 | 42802.87 | 56038.36 | 9984.30 | 150.09 | 1.87e-12 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 4.9m filter | | MKO/MIRSI.7_7 | 77152.84 | 77243.27 | 77019.44 | 72225.76 | 83260.01 | 6871.00 | 62.32 | 3.14e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 7.7m filter | | MKO/MIRSI.8_7 | 87162.73 | 87261.70 | 87000.53 | 81231.20 | 93272.56 | 7650.69 | 49.38 | 1.95e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 8.7m filter | | MKO/MIRSI.9_7 | 96639.73 | 96768.69 | 96434.09 | 89588.65 | 104384.88 | 9319.11 | 40.46 | 1.3e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 9.7m filter | | MKO/MIRSI.N | 103312.78 | 106027.21 | 99056.15 | 78225.76 | 134489.00 | 44133.66 | 37.78 | 1.06e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI N filter | | MKO/MIRSI.11_7 | 116297.09 | 116453.57 | 116045.47 | 107429.84 | 124727.50 | 11480.35 | 28.16 | 6.24e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 11.7m filter | | MKO/MIRSI.12_282 | 122649.22 | 122656.86 | 122633.88 | 120089.05 | 125529.64 | 1992.05 | 25.27 | 5.04e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 12.282m filter | | MKO/MIRSI.12_33 | 123288.64 | 123451.72 | 123017.05 | 114236.73 | 132638.27 | 11764.36 | 25.09 | 4.95e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 12.33m filter | | MKO/MIRSI.18 | 183224.57 | 183407.88 | 182920.60 | 172670.74 | 197233.41 | 15057.84 | 11.48 | 1.03e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 18m filter | | MKO/MIRSI.20 | 209807.83 | 214280.22 | 202858.11 | 162500.35 | 289684.76 | 75307.77 | 9.22 | 6.28e-15 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 20m filter | | MKO/MIRSI.24 | 247768.87 | 248081.29 | 247254.11 | 224811.65 | 276399.86 | 20449.75 | 6.30 | 3.07e-15 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 24m 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}
 ≡ filter transmission<p>f(λ) ≡ flux of the spectrum<p><u>Property info:</u><ul><li><b>UCD</b>:meta.code<li><b>Utype</b>: <i>photdm:PhotometricSystem.detectorType</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission<p><img src=showgraph.php?what=lmean&val=21952.661950405&id=MKO/MIRSI.K><p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl</ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission<br> Vg(λ) ≡ Vega spectrum.<p><img src=showgraph.php?what=leff&val=21721.174940495&id=MKO/MIRSI.K><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>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission<p><img src=showgraph.php?what=lpiv&val=21859.429819292&id=MKO/MIRSI.K><p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl</ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission<br> Vg(λ) ≡ Vega spectrum<p><img src=showgraph.php?what=lphot&val=21782.353285947&id=MKO/MIRSI.K><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</ul></td></table>',STICKY,true,CLOSEBTN,true,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><img src=showgraph.php?what=weff&val=3625.3404675169,22004.882162134,0.9235&id=MKO/MIRSI.K><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>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
![(?)](javascript:Tip('<b>A<sub>f</sub>/A<sub>V</sub></b><br><table cellpadding=20><td class=helptd>Ratio between extintion at λ<sub>ref</sub> and visual extintion. <p>Calculated by the service using the extinction law by <a href="http://adsabs.harvard.edu/abs/1999PASP..111...63F" target="_blank">Fitzpatrick (1999)</a> improved by <a href="http://adsabs.harvard.edu/abs/2005ApJ...619..931I" target="_blank">Indebetouw et al (2005)</a> in the infrared. <p><img src="images/extlaw.png"><p>You can download the corresponding <a href=\"getextlaw.php\" target=\"_blank\">data file</a> for the opacity k<sub>λ</sub>. The extinction at each wavelength is calculated as: A<sub>λ</sub> = A<sub>V</sub> * k<sub>λ</sub>/k<sub>V</sub>, where k<sub>λ</sub> is the opacity for a given λ and k<sub>V</sub>=211.4<p><p><u>Property info:</u><ul></ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission.<br> Sun(λ) ≡ Sun spectrum.<p><img src="images/sun.png"><p><p><u>More info:</u><p>Sun spectrum from calspec database: sun_reference_stis_002 composed with sun_mod_001 for larger wavelengths.<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/sun.dat" target="_blank">Sun composed spectrum</a> (units: Angstrom erg/cm2/s/A).</ul><p><u>Property info:</u><ul><li><b>Unit</b>:erg/cm2/s/A<li><b>UCD</b>:phot.flux.density</ul></td></table>',STICKY,true,CLOSEBTN,true,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>VO PhotDM Utypes</u>: <br><i>PhotCal.MagnitudeSystem.type</i> -> VEGAmag <br><i>PhotCal.ZeroPoint.Flux.value</i> -> F<sub>0</sub><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>UCD</b>:phot.flux.density<li><b>Utype</b>: <i>photdm:PhotCal.ZeroPoint.Flux.value</i></ul></td></table>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
