Sentinel :ESA is developing a series of next-generation Earth observation missions, on behalf of the joint ESA/European Commission initiative GMES (Global Monitoring for Environment and Security). Sentinel/SLSTR-B :SLSTR instrument on board Sentinel-3B. Following ENVISAT's AATSR instrument, the SLSTR instrument is a conical scanning imaging radiometer employing the along track scanning dual view technique.id:Sentinel/SLSTR-B.a |
| Sentinel/SLSTR-B.S1 | 5555.96 | 5556.89 | 5555.03 | 5418.95 | 5704.76 | 187.50 | 3568.71 | 3.47e-9 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S1 normalized SRF | | Sentinel/SLSTR-B.S2 | 6599.11 | 6599.94 | 6600.61 | 6454.29 | 6747.44 | 192.94 | 2772.78 | 1.91e-9 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S2 normalized SRF | | Sentinel/SLSTR-B.S3 | 8675.60 | 8676.35 | 8675.27 | 8503.93 | 8836.63 | 206.03 | 2217.96 | 8.83e-10 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S3 normalized SRF | | Sentinel/SLSTR-B.S3 | Filter Description | Filter ID (?) : | Sentinel/SLSTR-B.S3 |
| Description (?) : | Sentinel3 SLSTR-B S3 normalized SRF |
| Phot.System (?) : | SLSTR-B |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | Sentinel |
| Instrument (?) : | SLSTR-B |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
8675.60 | ------- | (Angstrom) |
| λmean (?) : |
8676.35 | ------- | (Angstrom) |
| λcen (?) : |
8676.06 | ------- | (Angstrom) |
| λeff (?) : |
8675.27 | ------- | (Angstrom) |
| λpeak (?) : |
8744.00 | ------- | (Angstrom) |
| λpivot (?) : |
8675.60 | ------- | (Angstrom) |
| λphot (?) : |
8675.77 | ------- | (Angstrom) |
| λmin (?) : |
8503.93 | ------- | (Angstrom) |
| λmax (?) : |
8836.63 | ------- | (Angstrom) |
| Weff (?) : |
206.03 | ------- | (Angstrom) |
| FWHM (?) : |
207.87 | ------- | (Angstrom) |
| Af/AV (?) : |
0.533 | ------- | () |
| Fsun (?) : |
96.41 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
Sentinel3 SLSTR Transmission components: Filter + Instrumentid:Sentinel/SLSTR-B.S3 | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
8.83435e-10 | (erg/cm2/s/A) |
| |
------- |
2217.96 | (Jy) |
| PhotCal ID (?) : |
Sentinel/SLSTR-B.S3/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
1.44626e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
Sentinel/SLSTR-B.S3/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
9116.01 | (Jy) |
| PhotCal ID (?) : |
Sentinel/SLSTR-B.S3/ST |
| |
|
Filter added: 2020-08-28 23:12:09
Last update: 2021-07-27 20:34:34 | | Sentinel/SLSTR-B.S4 | 13750.69 | 13751.11 | 13750.13 | 13606.88 | 13901.08 | 206.22 | 1329.86 | 2.11e-10 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S4 normalized SRF | | Sentinel/SLSTR-B.S5 | 16112.67 | 16116.53 | 16106.82 | 15642.06 | 16591.31 | 663.55 | 1026.82 | 1.19e-10 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S5 normalized SRF | | Sentinel/SLSTR-B.S6 | 22530.61 | 22532.25 | 22528.14 | 22160.79 | 22942.02 | 505.69 | 607.59 | 3.59e-11 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S6 normalized SRF | | Sentinel/SLSTR-B.S7 | 37355.59 | 37423.61 | 37248.23 | 34061.85 | 41412.12 | 4053.47 | 246.18 | 5.29e-12 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S7 normalized SRF | | Sentinel/SLSTR-B.S8 | 108153.83 | 108242.84 | 108011.83 | 101767.20 | 115564.37 | 7618.54 | 32.41 | 8.31e-14 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S8 normalized SRF | | Sentinel/SLSTR-B.S9 | 120329.74 | 120452.11 | 120125.72 | 111815.79 | 130545.52 | 8988.37 | 26.32 | 5.45e-14 | Sentinel | SLSTR-B | Sentinel3 SLSTR-B S9 normalized SRF |
|
| 
 ≡ 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=8676.3523072651&id=Sentinel/SLSTR-B.S3><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=8675.273126386&id=Sentinel/SLSTR-B.S3><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=8675.6034647262&id=Sentinel/SLSTR-B.S3><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=8675.7727160811&id=Sentinel/SLSTR-B.S3><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=206.02586742212,8676.055685857,0.99999837275481&id=Sentinel/SLSTR-B.S3><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}
