MKO :Mauna Kea Observatories MKO/MIRSI :MIRSI (Mid-InfraRed Spectrometer and Imager) is a mid-infrared camera system with both spectroscopic and imaging capabilities. |
| MKO/MIRSI.K | 21859.45 | 21952.68 | 21721.89 | 19670.77 | 24331.32 | 3625.29 | 651.57 | 4.14e-11 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI K filter | | MKO/MIRSI.4_9 | 49027.79 | 49308.21 | 48590.58 | 42802.87 | 56038.36 | 9984.32 | 151.37 | 1.92e-12 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 4.9m filter | | MKO/MIRSI.7_7 | 77152.85 | 77243.27 | 77017.98 | 72225.76 | 83260.01 | 6871.01 | 63.83 | 3.23e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 7.7m filter | | MKO/MIRSI.8_7 | 87162.73 | 87261.70 | 87001.35 | 81231.20 | 93272.56 | 7650.67 | 50.54 | 2.0e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 8.7m filter | | MKO/MIRSI.9_7 | 96639.73 | 96768.69 | 96433.99 | 89588.65 | 104384.88 | 9319.11 | 41.41 | 1.33e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 9.7m filter | | MKO/MIRSI.N | 103310.70 | 106025.58 | 99054.28 | 78225.76 | 134489.00 | 44136.53 | 35.69 | 1.09e-13 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI N filter | | MKO/MIRSI.11_7 | 116297.09 | 116453.57 | 116042.48 | 107429.84 | 124727.50 | 11480.37 | 28.81 | 6.41e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 11.7m filter | | MKO/MIRSI.12_282 | 122649.22 | 122656.86 | 122636.53 | 120089.05 | 125529.64 | 1992.04 | 25.97 | 5.18e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 12.282m filter | | MKO/MIRSI.12_282 | Filter Description | Filter ID (?) : | MKO/MIRSI.12_282 |
| Description (?) : | Mauna kea Obsevatory. MIRSI 12.282m filter |
| Phot.System (?) : | MIRSI |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | MKO |
| Instrument (?) : | MIRSI |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
122649.22 | ------- | (Angstrom) |
| λmean (?) : |
122656.86 | ------- | (Angstrom) |
| λcen (?) : |
122634.43 | ------- | (Angstrom) |
| λeff (?) : |
122636.53 | ------- | (Angstrom) |
| λpeak (?) : |
122512.05 | ------- | (Angstrom) |
| λpivot (?) : |
122649.22 | ------- | (Angstrom) |
| λphot (?) : |
122641.72 | ------- | (Angstrom) |
| λmin (?) : |
120089.05 | ------- | (Angstrom) |
| λmax (?) : |
125529.64 | ------- | (Angstrom) |
| Weff (?) : |
1992.04 | ------- | (Angstrom) |
| FWHM (?) : |
1779.35 | ------- | (Angstrom) |
| Af/AV (?) : |
0.0338 | ------- | () |
| Fsun (?) : |
0.0109 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
MIRSI Transmission components: Filter | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
5.1767e-14 | (erg/cm2/s/A) |
| |
------- |
25.97 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MKO/MIRSI.12_282/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
7.23781e-12 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MKO/MIRSI.12_282/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
1821567.46 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
MKO/MIRSI.12_282/ST |
| |
|
Filter added: 2017-07-26 22:35:07
Last update: 2020-12-10 16:33:06 | | MKO/MIRSI.12_33 | 123288.64 | 123451.72 | 123016.57 | 114236.73 | 132638.27 | 11764.34 | 25.69 | 5.09e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 12.33m filter | | MKO/MIRSI.18 | 183224.55 | 183407.87 | 182922.72 | 172670.74 | 197233.41 | 15057.92 | 11.76 | 1.05e-14 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 18m filter | | MKO/MIRSI.20 | 209807.66 | 214280.08 | 202871.45 | 162500.35 | 289684.76 | 75307.92 | 8.87 | 6.46e-15 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 20m filter | | MKO/MIRSI.24 | 247768.84 | 248081.26 | 247226.23 | 224811.65 | 276399.86 | 20449.81 | 6.46 | 3.17e-15 | MKO | MIRSI | Mauna kea Obsevatory. MIRSI 24m filter |
|
| 
 ≡ 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}
 ≡ filter transmission<p>f(λ) ≡ flux of the spectrum<p><u>Property info:</u><ul><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=122656.8645503&id=MKO/MIRSI.12_282><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>',STICKY,true,CLOSEBTN,true,WIDTH,400)){kind=link}
 ≡ filter transmission<br> Vg(λ) ≡ Vega spectrum.<p><img src=showgraph.php?what=leff&val=122636.53143502&id=MKO/MIRSI.12_282><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=122649.22343357&id=MKO/MIRSI.12_282><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=122641.71847244&id=MKO/MIRSI.12_282><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=1992.0397863811,122634.43200757,0.7878&id=MKO/MIRSI.12_282><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>',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/extinctionlaw.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/sunspec.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}
