JWST :James Webb Space Telescope JWST/MIRI :The JWST Mid-Infrared Instrument (MIRI) provides imaging and spectroscopic observing modes from 4.9 to 28.8 μm |
| JWST/MIRI.F560W | 56352.57 | 56651.28 | 55870.54 | 48847.40 | 64242.60 | 9461.36 | 116.38 | 1.12e-12 | JWST | MIRI | MIRI F560W filter | | JWST/MIRI.F770W | 76393.24 | 77111.39 | 75224.94 | 64740.10 | 88353.20 | 18278.13 | 64.83 | 3.43e-13 | JWST | MIRI | MIRI F770W filter | | JWST/MIRI.F1000W | 99531.16 | 99981.09 | 98792.57 | 87627.69 | 111018.10 | 17036.69 | 38.99 | 1.2e-13 | JWST | MIRI | MIRI F1000W filter | | JWST/MIRI.F1065C | 105628.39 | 105681.52 | 105542.39 | 100201.08 | 111538.67 | 5647.25 | 33.89 | 9.11e-14 | JWST | MIRI | MIRI F1065C coronographic filter | | JWST/MIRI.F1140C | 113103.03 | 113156.52 | 113013.47 | 107334.19 | 119536.96 | 6036.53 | 29.63 | 6.94e-14 | JWST | MIRI | MIRI F1140C coronographic filter | | JWST/MIRI.F1130W | 113085.01 | 113159.44 | 112960.72 | 106389.50 | 119837.00 | 7229.15 | 30.42 | 7.15e-14 | JWST | MIRI | MIRI F1130W filter | | JWST/MIRI.F1280W | 128101.37 | 128738.34 | 127060.62 | 112516.00 | 143369.40 | 24337.72 | 23.79 | 4.42e-14 | JWST | MIRI | MIRI F1280W filter | | JWST/MIRI.F1280W | Filter Description | Filter ID (?) : | JWST/MIRI.F1280W |
| Description (?) : | MIRI F1280W filter |
| Phot.System (?) : | MIRI |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | JWST |
| Instrument (?) : | MIRI |
| Comments (?) : | nominal transmission of the JWST OTE is not included |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
128101.37 | ------- | (Angstrom) |
| λmean (?) : |
128738.34 | ------- | (Angstrom) |
| λcen (?) : |
128539.68 | ------- | (Angstrom) |
| λeff (?) : |
127060.62 | ------- | (Angstrom) |
| λpeak (?) : |
120780.00 | ------- | (Angstrom) |
| λpivot (?) : |
128101.37 | ------- | (Angstrom) |
| λphot (?) : |
127481.80 | ------- | (Angstrom) |
| λmin (?) : |
112516.00 | ------- | (Angstrom) |
| λmax (?) : |
143369.40 | ------- | (Angstrom) |
| Weff (?) : |
24337.72 | ------- | (Angstrom) |
| FWHM (?) : |
25339.06 | ------- | (Angstrom) |
| Af/AV (?) : |
0.0294 | ------- | () |
| Fsun (?) : |
0.00928 | ------- | (erg/cm2/s/A) |
| Response
Data file: ascii, VOTable Reference for filter response:
James Webb Space Telescope User Documentation Transmission components: Filter + Instrument | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
4.41715e-14 | (erg/cm2/s/A) |
| |
------- |
23.79 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
JWST/MIRI.F1280W/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
6.74256e-12 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
JWST/MIRI.F1280W/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
1955363.34 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
JWST/MIRI.F1280W/ST |
| |
|
Filter added: 2017-03-11 12:33:37
Last update: 2020-12-10 16:32:16 | | JWST/MIRI.F1500W | 150635.07 | 151469.08 | 149256.55 | 131189.10 | 171410.90 | 29426.23 | 17.28 | 2.32e-14 | JWST | MIRI | MIRI F1500W filter | | JWST/MIRI.F1550C | 155167.74 | 155219.65 | 155079.50 | 149400.62 | 161523.61 | 7038.01 | 15.93 | 1.98e-14 | JWST | MIRI | MIRI F1550C coronographic filter | | JWST/MIRI.F1800W | 179837.23 | 180508.31 | 178732.78 | 160278.80 | 202850.60 | 29145.64 | 12.18 | 1.14e-14 | JWST | MIRI | MIRI F1800W filter | | JWST/MIRI.F2100W | 207950.06 | 209373.20 | 205607.10 | 178759.00 | 244051.00 | 44045.65 | 9.11 | 6.46e-15 | JWST | MIRI | MIRI F2100W filter | | JWST/MIRI.F2300C | 226446.44 | 227630.49 | 224493.76 | 196351.35 | 261867.66 | 43032.65 | 7.62 | 4.45e-15 | JWST | MIRI | MIRI F2300C coronographic filter | | JWST/MIRI.F2550W | 253640.04 | 254994.19 | 251520.10 | 223391.40 | 299940.00 | 38759.89 | 6.14 | 2.91e-15 | JWST | MIRI | MIRI F2550W 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=128738.3368061&id=JWST/MIRI.F1280W><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 (photon counter)<br> Vg(λ) ≡ Vega spectrum<p><img src=showgraph.php?what=leff&val=127060.61771058&id=JWST/MIRI.F1280W><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=128101.36999074&id=JWST/MIRI.F1280W><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 (photon counter)<br> Vg(λ) ≡ Vega spectrum<p><img src=showgraph.php?what=lphot&val=127481.80123344&id=JWST/MIRI.F1280W><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=24337.719010728,128539.67989002,0.3504&id=JWST/MIRI.F1280W><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 (photon counter).<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 (photon counter).<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}
