GOES :The Geostationary Operational Environmental Satellite Program (GOES) is a joint effort of NASA and the National Oceanic and Atmospheric Administration (NOAA). GOES/ABI1 :Advanced Baseline Imager (ABI) PFM, on board GOES-16 |
| GOES/ABI1.Ch01 | 4706.92 | 4711.39 | 4696.34 | 4444.56 | 4966.64 | 375.61 | 4029.85 | 5.45e-9 | GOES | GOES-ABI | GOES16 PFM ABI Ch01 normalized SRF | | GOES/ABI1.Ch02 | 6380.15 | 6395.63 | 6360.91 | 5803.57 | 6933.38 | 825.65 | 3047.08 | 2.24e-9 | GOES | GOES-ABI | GOES16 PFM ABI Ch02 normalized SRF | | GOES/ABI1.Ch03 | 8641.48 | 8643.79 | 8641.14 | 8346.49 | 8952.92 | 347.16 | 2231.18 | 8.96e-10 | GOES | GOES-ABI | GOES16 PFM ABI Ch03 normalized SRF | | GOES/ABI1.Ch04 | 13732.02 | 13732.23 | 13731.74 | 13615.39 | 13843.93 | 136.82 | 1332.33 | 2.12e-10 | GOES | GOES-ABI | GOES16 PFM ABI Ch04 normalized SRF | | GOES/ABI1.Ch05 | 16092.97 | 16095.18 | 16090.57 | 15683.96 | 16493.20 | 451.65 | 1033.55 | 1.2e-10 | GOES | GOES-ABI | GOES16 PFM ABI Ch05 normalized SRF | | GOES/ABI1.Ch06 | 22425.72 | 22427.11 | 22423.64 | 22048.22 | 22797.80 | 461.57 | 612.58 | 3.65e-11 | GOES | GOES-ABI | GOES16 PFM ABI Ch06 normalized SRF | | GOES/ABI1.Ch07 | 38919.22 | 38933.60 | 38897.11 | 37341.43 | 40555.15 | 1763.32 | 228.00 | 4.51e-12 | GOES | GOES-ABI | GOES16 PFM ABI Ch07 normalized SRF | | GOES/ABI1.Ch07 | Filter Description | Filter ID (?) : | GOES/ABI1.Ch07 |
| Description (?) : | GOES16 PFM ABI Ch07 normalized SRF |
| Phot.System (?) : | GOES-ABI |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | GOES |
| Instrument (?) : | GOES-ABI |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
38919.22 | ------- | (Angstrom) |
| λmean (?) : |
38933.60 | ------- | (Angstrom) |
| λcen (?) : |
38974.10 | ------- | (Angstrom) |
| λeff (?) : |
38897.11 | ------- | (Angstrom) |
| λpeak (?) : |
38878.70 | ------- | (Angstrom) |
| λpivot (?) : |
38919.22 | ------- | (Angstrom) |
| λphot (?) : |
38906.66 | ------- | (Angstrom) |
| λmin (?) : |
37341.43 | ------- | (Angstrom) |
| λmax (?) : |
40555.15 | ------- | (Angstrom) |
| Weff (?) : |
1763.32 | ------- | (Angstrom) |
| FWHM (?) : |
1896.01 | ------- | (Angstrom) |
| Af/AV (?) : |
0.0607 | ------- | () |
| Fsun (?) : |
0.966 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
Advanced Baseline Imager(ABI) Transmission components: Filter + Instrument | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
4.51268e-12 | (erg/cm2/s/A) |
| |
------- |
228.00 | (Jy) |
| PhotCal ID (?) : |
GOES/ABI1.Ch07/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
7.18652e-11 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
GOES/ABI1.Ch07/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
183456.77 | (Jy) |
| PhotCal ID (?) : |
GOES/ABI1.Ch07/ST |
| |
|
Filter added: 2020-08-27 20:18:43
Last update: 2021-07-27 19:15:30 | | GOES/ABI1.Ch08 | 61843.57 | 61978.83 | 61632.06 | 56688.99 | 67058.51 | 7728.28 | 95.81 | 7.51e-13 | GOES | GOES-ABI | GOES16 PFM ABI Ch08 normalized SRF | | GOES/ABI1.Ch09 | 69311.59 | 69349.66 | 69254.44 | 65729.71 | 72667.94 | 4140.25 | 76.76 | 4.79e-13 | GOES | GOES-ABI | GOES16 PFM ABI Ch09 normalized SRF | | GOES/ABI1.Ch10 | 73362.45 | 73369.62 | 73349.82 | 71862.42 | 74892.64 | 1869.97 | 68.82 | 3.83e-13 | GOES | GOES-ABI | GOES16 PFM ABI Ch10 normalized SRF | | GOES/ABI1.Ch11 | 84477.13 | 84510.48 | 84420.46 | 81037.61 | 88189.65 | 4138.66 | 52.47 | 2.2e-13 | GOES | GOES-ABI | GOES16 PFM ABI Ch11 normalized SRF | | GOES/ABI1.Ch12 | 96093.03 | 96114.53 | 96059.82 | 93166.11 | 99210.64 | 3768.02 | 40.82 | 1.33e-13 | GOES | GOES-ABI | GOES16 PFM ABI Ch12 normalized SRF | | GOES/ABI1.Ch13 | 103328.16 | 103350.75 | 103288.77 | 99517.64 | 107833.28 | 3175.82 | 35.38 | 9.94e-14 | GOES | GOES-ABI | GOES16 PFM ABI Ch13 normalized SRF | | GOES/ABI1.Ch14 | 111940.28 | 112023.93 | 111799.69 | 105392.08 | 118651.96 | 7710.76 | 30.28 | 7.24e-14 | GOES | GOES-ABI | GOES16 PFM ABI Ch14 normalized SRF | | GOES/ABI1.Ch15 | 122760.65 | 122866.09 | 122567.89 | 114765.27 | 130440.28 | 8989.17 | 25.21 | 5.01e-14 | GOES | GOES-ABI | GOES16 PFM ABI Ch15 normalized SRF | | GOES/ABI1.Ch16 | 132699.61 | 132736.32 | 132639.34 | 128373.55 | 137570.24 | 5428.59 | 21.71 | 3.7e-14 | GOES | GOES-ABI | GOES16 PFM ABI Ch16 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=38933.60348721&id=GOES/ABI1.Ch07><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=38897.105784379&id=GOES/ABI1.Ch07><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=38919.217005783&id=GOES/ABI1.Ch07><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=38906.657332912&id=GOES/ABI1.Ch07><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=1763.3240889603,38974.100347955,0.99999243&id=GOES/ABI1.Ch07><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}
