Rosetta :Rosetta is an ESA cornerstone mission to chase, go into orbit around, and land on a comet. Rosetta/OSIRIS_WAC :The Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) is the main imaging system of the Rosetta mission. Wide-angle camera.id:Rosetta/OSIRIS_WAC.a |
| Rosetta/OSIRIS_WAC.UV245 | 2454.51 | 2456.07 | 2455.50 | 2331.98 | 2637.81 | 143.76 | 794.95 | 3.96e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC UV245 Filter | | Rosetta/OSIRIS_WAC.F31 | 2457.23 | 2458.77 | 2458.19 | 2334.94 | 2639.70 | 143.62 | 796.24 | 3.95e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F31 Filter (full) | | Rosetta/OSIRIS_WAC.F41 | 2580.46 | 2580.84 | 2580.95 | 2498.19 | 2673.05 | 60.48 | 853.25 | 3.84e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F41 Filter (full) | | Rosetta/OSIRIS_WAC.CS | 2580.56 | 2580.97 | 2581.06 | 2497.58 | 2677.92 | 60.50 | 862.27 | 3.88e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC CS Filter | | Rosetta/OSIRIS_WAC.UV295 | 2948.05 | 2948.75 | 2948.84 | 2842.54 | 3059.91 | 109.18 | 1069.76 | 3.69e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC UV295 Filter | | Rosetta/OSIRIS_WAC.F51 | 2948.46 | 2949.16 | 2949.25 | 2843.02 | 3060.67 | 109.73 | 1070.09 | 3.69e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F51 Filter (full) | | Rosetta/OSIRIS_WAC.OH | 3089.05 | 3089.23 | 3089.08 | 3023.98 | 3157.26 | 42.82 | 1138.92 | 3.58e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC OH Filter | | Rosetta/OSIRIS_WAC.F61 | 3089.09 | 3089.28 | 3089.14 | 3023.49 | 3157.77 | 43.52 | 1139.55 | 3.58e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F61 Filter (full) | | Rosetta/OSIRIS_WAC.UV325 | 3246.89 | 3247.59 | 3247.33 | 3105.66 | 3372.33 | 111.58 | 1196.93 | 3.4e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC UV325 Filter | | Rosetta/OSIRIS_WAC.F71 | 3247.30 | 3248.01 | 3247.76 | 3102.32 | 3375.18 | 111.11 | 1196.59 | 3.4e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F71 Filter (full) | | Rosetta/OSIRIS_WAC.NH | 3350.11 | 3350.25 | 3350.16 | 3290.47 | 3414.04 | 44.77 | 1232.42 | 3.29e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC NH Filter | | Rosetta/OSIRIS_WAC.F81 | 3350.21 | 3350.35 | 3350.23 | 3290.58 | 3414.58 | 44.94 | 1228.27 | 3.28e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F81 Filter (full) | | Rosetta/OSIRIS_WAC.UV375 | 3748.28 | 3748.99 | 3757.55 | 3613.20 | 3894.66 | 104.81 | 1896.86 | 4.05e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC UV375 Filter | | Rosetta/OSIRIS_WAC.F13 | 3751.44 | 3752.18 | 3761.00 | 3620.11 | 3940.44 | 103.17 | 1930.86 | 4.11e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F13 Filter (full) | | Rosetta/OSIRIS_WAC.CN | 3872.80 | 3873.10 | 3873.22 | 3784.95 | 3970.58 | 58.21 | 3323.40 | 6.64e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC CN Filter | | Rosetta/OSIRIS_WAC.F14 | 3874.25 | 3874.56 | 3874.64 | 3787.60 | 3975.96 | 59.56 | 3320.99 | 6.63e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F14 Filter (full) | | Rosetta/OSIRIS_WAC.F21 | 5346.46 | 5356.71 | 5336.42 | 4893.01 | 5845.03 | 597.85 | 3708.87 | 3.89e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F21 Filter (full) | | Rosetta/OSIRIS_WAC.Green | 5346.77 | 5357.04 | 5336.71 | 4892.55 | 5846.12 | 597.60 | 3708.66 | 3.89e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC Green Filter | | Rosetta/OSIRIS_WAC.F15 | 5712.28 | 5713.03 | 5711.57 | 5542.68 | 5903.16 | 128.45 | 3473.73 | 3.19e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F15 Filter (full) | | Rosetta/OSIRIS_WAC.NH2 | 5712.47 | 5713.22 | 5711.75 | 5543.11 | 5903.87 | 128.40 | 3473.63 | 3.19e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC NH2 Filter | | Rosetta/OSIRIS_WAC.F16 | 5895.95 | 5896.09 | 5895.82 | 5818.79 | 5976.36 | 53.07 | 3351.97 | 2.89e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F16 Filter (full) | | Rosetta/OSIRIS_WAC.NA | 5895.97 | 5896.11 | 5895.84 | 5819.45 | 5976.20 | 52.05 | 3352.41 | 2.89e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC NA Filter | | Rosetta/OSIRIS_WAC.F18 | 6116.34 | 6117.16 | 6115.48 | 5961.44 | 6316.56 | 109.96 | 3225.98 | 2.59e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F18 Filter (full) | | Rosetta/OSIRIS_WAC.VIS610 | 6116.76 | 6117.59 | 6115.87 | 5961.88 | 6318.37 | 110.05 | 3225.74 | 2.58e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC VIS610 Filter | | Rosetta/OSIRIS_WAC.F12 | 6248.78 | 6296.51 | 6196.01 | 5372.22 | 7240.76 | 1420.41 | 3153.93 | 2.42e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F12 Filter (full) | | Rosetta/OSIRIS_WAC.F17 | 6307.00 | 6307.17 | 6306.72 | 6222.08 | 6401.63 | 51.40 | 3125.34 | 2.36e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC F17 Filter (full) | | Rosetta/OSIRIS_WAC.OI | 6307.10 | 6307.27 | 6306.82 | 6223.69 | 6400.53 | 49.47 | 3125.52 | 2.36e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC OI Filter | | Rosetta/OSIRIS_WAC.Red | 6276.39 | 6324.75 | 6222.78 | 5374.93 | 7250.95 | 1388.29 | 3138.84 | 2.39e-9 | Rosetta | OSIRIS_WAC | OSIRIS_WAC Red Filter | | Rosetta/OSIRIS_WAC.Red | Filter Description | Filter ID (?) : | Rosetta/OSIRIS_WAC.Red |
| Description (?) : | OSIRIS_WAC Red Filter |
| Phot.System (?) : | Rosetta-Osiris |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | Rosetta |
| Instrument (?) : | OSIRIS_WAC |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
6276.39 | ------- | (Angstrom) |
| λmean (?) : |
6324.75 | ------- | (Angstrom) |
| λcen (?) : |
6278.10 | ------- | (Angstrom) |
| λeff (?) : |
6222.78 | ------- | (Angstrom) |
| λpeak (?) : |
6660.00 | ------- | (Angstrom) |
| λpivot (?) : |
6276.39 | ------- | (Angstrom) |
| λphot (?) : |
6255.35 | ------- | (Angstrom) |
| λmin (?) : |
5374.93 | ------- | (Angstrom) |
| λmax (?) : |
7250.95 | ------- | (Angstrom) |
| Weff (?) : |
1388.29 | ------- | (Angstrom) |
| FWHM (?) : |
1549.28 | ------- | (Angstrom) |
| Af/AV (?) : |
0.859 | ------- | () |
| Fsun (?) : |
164.86 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
Magrin et al, 2015 Transmission components: Filterid:Rosetta/OSIRIS_WAC.Red | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
2.38874e-9 | (erg/cm2/s/A) |
| |
------- |
3138.84 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Rosetta/OSIRIS_WAC.Red/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
2.76329e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Rosetta/OSIRIS_WAC.Red/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
4771.18 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
Rosetta/OSIRIS_WAC.Red/ST |
| |
|
Filter added: 2020-06-06 15:48:31
Last update: 2021-07-27 20:32:34 |
|
| 
 ≡ 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=6324.7535818328&id=Rosetta/OSIRIS_WAC.Red><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=6222.7802834025&id=Rosetta/OSIRIS_WAC.Red><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=6276.390206534&id=Rosetta/OSIRIS_WAC.Red><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=6255.3450699944&id=Rosetta/OSIRIS_WAC.Red><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=1388.2932265344,6278.0966767114,1&id=Rosetta/OSIRIS_WAC.Red><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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>Filter transmission is transformed to \"<i>energy counter</i>\" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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}
