ISO :The Infrared Space Observatory (ISO) was the world's first true orbiting infrared observatory. ISO/PHT-P :ISO PHT-P filtersid:ISO/PHT-P.a |
| ISO/PHT-P.3_29mu | 33024.66 | 33043.23 | 32995.47 | 31147.20 | 35207.56 | 1828.45 | 307.02 | 8.44e-12 | ISO | PHT | ISO PHT-P 3.29 μm filter. | | ISO/PHT-P.3_6mu | 35547.84 | 35899.54 | 34990.51 | 29558.83 | 41610.49 | 8139.19 | 275.09 | 6.53e-12 | ISO | PHT | ISO PHT-P 3.6 μm filter. | | ISO/PHT-P.4_85mu | 47934.45 | 48558.02 | 46979.03 | 39922.52 | 58518.43 | 13935.83 | 159.22 | 2.08e-12 | ISO | PHT | ISO PHT-P 4.85 μm filter. | | ISO/PHT-P.7_3mu | 71956.35 | 73975.86 | 68738.48 | 54385.83 | 93798.81 | 26929.41 | 76.51 | 4.43e-13 | ISO | PHT | ISO PHT-P 7.3 μm filter. | | ISO/PHT-P.7_7mu | 76511.62 | 76622.46 | 76341.93 | 70510.79 | 83910.24 | 6843.81 | 63.41 | 3.25e-13 | ISO | PHT | ISO PHT-P 7.7 μm filter. | | ISO/PHT-P.10mu | 99620.05 | 100033.83 | 98953.81 | 88259.10 | 113563.21 | 15770.95 | 38.40 | 1.16e-13 | ISO | PHT | ISO PHT-P 10 μm filter. | | ISO/PHT-P.11_3mu | 113456.86 | 113530.34 | 113336.83 | 106616.77 | 121300.24 | 6178.79 | 29.46 | 6.86e-14 | ISO | PHT | ISO PHT-P 11.3 μm filter. | | ISO/PHT-P.11_3mu | Filter Description | Filter ID (?) : | ISO/PHT-P.11_3mu |
| Description (?) : | ISO PHT-P 11.3 μm filter. |
| Phot.System (?) : | ISO |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | ISO |
| Instrument (?) : | PHT |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
113456.86 | ------- | (Angstrom) |
| λmean (?) : |
113530.34 | ------- | (Angstrom) |
| λcen (?) : |
113551.77 | ------- | (Angstrom) |
| λeff (?) : |
113336.83 | ------- | (Angstrom) |
| λpeak (?) : |
112725.80 | ------- | (Angstrom) |
| λpivot (?) : |
113456.86 | ------- | (Angstrom) |
| λphot (?) : |
113385.29 | ------- | (Angstrom) |
| λmin (?) : |
106616.77 | ------- | (Angstrom) |
| λmax (?) : |
121300.24 | ------- | (Angstrom) |
| Weff (?) : |
6178.79 | ------- | (Angstrom) |
| FWHM (?) : |
6306.09 | ------- | (Angstrom) |
| Af/AV (?) : |
0.0461 | ------- | () |
| Fsun (?) : |
0.0148 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
ISO Handbook, Volume IV: PHT-The Imaging Photo-Polarimeter Transmission components: Filter + Instrumentid:ISO/PHT-P.11_3mu | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
6.86043e-14 | (erg/cm2/s/A) |
| |
------- |
29.46 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
ISO/PHT-P.11_3mu/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
8.4564e-12 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
ISO/PHT-P.11_3mu/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
1559075.08 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
ISO/PHT-P.11_3mu/ST |
| |
|
Filter added: 2019-02-04 15:06:35
Last update: 2021-07-27 19:45:40 | | ISO/PHT-P.11_5mu | 114118.05 | 118898.38 | 106235.77 | 79169.81 | 155762.08 | 52560.74 | 32.57 | 7.5e-14 | ISO | PHT | ISO PHT-P 11.5 μm filter. | | ISO/PHT-P.12_8mu | 127660.19 | 128181.63 | 126811.29 | 112889.98 | 145281.02 | 20803.13 | 23.62 | 4.35e-14 | ISO | PHT | ISO PHT-P 12.8 μm filter. | | ISO/PHT-P.16mu | 150944.55 | 151594.48 | 149924.44 | 135422.50 | 176678.86 | 19330.98 | 16.99 | 2.24e-14 | ISO | PHT | ISO PHT-P 16 μm filter. | | ISO/PHT-P.20mu | 204902.61 | 210277.81 | 195300.99 | 147849.56 | 255676.79 | 65554.50 | 9.88 | 7.06e-15 | ISO | PHT | ISO PHT-P 20 μm filter. | | ISO/PHT-P.25mu | 233752.69 | 237987.42 | 227109.64 | 185213.43 | 307365.54 | 67757.99 | 7.38 | 4.05e-15 | ISO | PHT | ISO PHT-P 25 μm filter. | | ISO/PHT-P.60mu | 592881.36 | 608540.36 | 562706.43 | 391659.29 | 748856.09 | 134173.02 | 1.18 | 1.01e-16 | ISO | PHT | ISO PHT-P 60 μm filter. | | ISO/PHT-P.100mu | 1.0e+6 | 1.02e+6 | 968221.42 | 700579.61 | 1.39e+6 | 286336.95 | 0.396 | 1.18e-17 | ISO | PHT | ISO PHT-P 100 μm filter. |
|
| 
 ≡ 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=113530.34019208&id=ISO/PHT-P.11_3mu><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=113336.83124496&id=ISO/PHT-P.11_3mu><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=113456.85559821&id=ISO/PHT-P.11_3mu><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=113385.28606532&id=ISO/PHT-P.11_3mu><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=6178.7895282355,113551.76737728,0.381854&id=ISO/PHT-P.11_3mu><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}
