ADEOS :The Advanced Earth Observing Satellite-II ADEOS/POLDER-2 :POLDER-2 is a passive optical imaging radiometer of CNES. The instrument is an identical twin to its predecessor, POLDER-1 flown on ADEOS.id:ADEOS/POLDER-2.a |
| ADEOS/POLDER-2.443 | 4444.44 | 4446.34 | 4447.37 | 4224.49 | 4710.00 | 196.45 | 4198.56 | 6.37e-9 | ADEOS | POLDER | ADEOS POLDER-2 443nm spectral response | | ADEOS/POLDER-2.443P | 4447.13 | 4448.96 | 4449.98 | 4228.73 | 4710.00 | 192.45 | 4206.82 | 6.38e-9 | ADEOS | POLDER | ADEOS POLDER-2 443nm P spectral response | | ADEOS/POLDER-2.490 | 4927.17 | 4928.53 | 4930.72 | 4727.65 | 5154.16 | 187.31 | 3712.50 | 4.58e-9 | ADEOS | POLDER | ADEOS POLDER-2 490nm spectral response | | ADEOS/POLDER-2.565 | 5648.32 | 5649.90 | 5646.75 | 5411.10 | 5893.47 | 216.54 | 3512.39 | 3.3e-9 | ADEOS | POLDER | ADEOS POLDER-2 565nm spectral response | | ADEOS/POLDER-2.565 | Filter Description | Filter ID (?) : | ADEOS/POLDER-2.565 |
| Description (?) : | ADEOS POLDER-2 565nm spectral response |
| Phot.System (?) : | POLDER |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | ADEOS |
| Instrument (?) : | POLDER |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
5648.32 | ------- | (Angstrom) |
| λmean (?) : |
5649.90 | ------- | (Angstrom) |
| λcen (?) : |
5651.53 | ------- | (Angstrom) |
| λeff (?) : |
5646.75 | ------- | (Angstrom) |
| λpeak (?) : |
5600.00 | ------- | (Angstrom) |
| λpivot (?) : |
5648.32 | ------- | (Angstrom) |
| λphot (?) : |
5647.81 | ------- | (Angstrom) |
| λmin (?) : |
5411.10 | ------- | (Angstrom) |
| λmax (?) : |
5893.47 | ------- | (Angstrom) |
| Weff (?) : |
216.54 | ------- | (Angstrom) |
| FWHM (?) : |
215.82 | ------- | (Angstrom) |
| Af/AV (?) : |
0.972 | ------- | () |
| Fsun (?) : |
184.63 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
PARASOL mission Transmission components: Filter + Instrumentid:ADEOS/POLDER-2.565 | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.30054e-9 | (erg/cm2/s/A) |
| |
------- |
3512.39 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
ADEOS/POLDER-2.565/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.412e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
ADEOS/POLDER-2.565/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
3864.06 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
ADEOS/POLDER-2.565/ST |
| |
|
Filter added: 2020-08-31 23:49:25
Last update: 2021-07-27 18:35:11 | | ADEOS/POLDER-2.670P | 6693.46 | 6694.60 | 6693.77 | 6486.73 | 6929.02 | 186.71 | 2888.48 | 1.93e-9 | ADEOS | POLDER | ADEOS POLDER-2 670nm P spectral response | | ADEOS/POLDER-2.765 | 7619.62 | 7623.07 | 7615.61 | 7192.46 | 8021.69 | 380.81 | 2530.54 | 1.31e-9 | ADEOS | POLDER | ADEOS POLDER-2 765nm spectral response | | ADEOS/POLDER-2.763 | 7630.35 | 7630.64 | 7630.04 | 7509.18 | 7747.86 | 110.22 | 2527.41 | 1.3e-9 | ADEOS | POLDER | ADEOS POLDER-2 763nm spectral response | | ADEOS/POLDER-2.865P | 8599.82 | 8602.90 | 8598.83 | 8241.10 | 8994.75 | 388.46 | 2233.88 | 9.06e-10 | ADEOS | POLDER | ADEOS POLDER-2 865nm P spectral response | | ADEOS/POLDER-2.910 | 9082.01 | 9082.89 | 9083.26 | 8871.05 | 9300.67 | 212.88 | 2282.34 | 8.3e-10 | ADEOS | POLDER | ADEOS POLDER-2 910nm spectral response |
|
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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=5649.903388401&id=ADEOS/POLDER-2.565><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=5646.7528789768&id=ADEOS/POLDER-2.565><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=5648.3154280793&id=ADEOS/POLDER-2.565><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=5647.8106528713&id=ADEOS/POLDER-2.565><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=216.5438304535,5651.5278323863,0.9998&id=ADEOS/POLDER-2.565><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}
