GOES :The Geostationary Operational Environmental Satellite Program (GOES) is a joint effort of NASA and the National Oceanic and Atmospheric Administration (NOAA). GOES/ABI4 :Advanced Baseline Imager (ABI) FM4, on board GOES-19id:GOES/ABI4.a |
| GOES/ABI4.Ch01 | 4705.22 | 4709.70 | 4694.65 | 4443.98 | 4966.25 | 375.68 | 4033.65 | 5.46e-9 | GOES | GOES-ABI | GOES19 FM4 ABI Ch01 normalized SRF | | GOES/ABI4.Ch02 | 6379.87 | 6395.36 | 6360.64 | 5803.70 | 6933.58 | 827.05 | 3047.26 | 2.24e-9 | GOES | GOES-ABI | GOES19 FM4 ABI Ch02 normalized SRF | | GOES/ABI4.Ch03 | 8634.47 | 8636.78 | 8634.07 | 8340.01 | 8946.59 | 347.76 | 2230.92 | 8.97e-10 | GOES | GOES-ABI | GOES19 FM4 ABI Ch03 normalized SRF | | GOES/ABI4.Ch03 | Filter Description | Filter ID (?) : | GOES/ABI4.Ch03 |
| Description (?) : | GOES19 FM4 ABI Ch03 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 (?) : |
8634.47 | ------- | (Angstrom) |
| λmean (?) : |
8636.78 | ------- | (Angstrom) |
| λcen (?) : |
8637.64 | ------- | (Angstrom) |
| λeff (?) : |
8634.07 | ------- | (Angstrom) |
| λpeak (?) : |
8549.93 | ------- | (Angstrom) |
| λpivot (?) : |
8634.47 | ------- | (Angstrom) |
| λphot (?) : |
8635.63 | ------- | (Angstrom) |
| λmin (?) : |
8340.01 | ------- | (Angstrom) |
| λmax (?) : |
8946.59 | ------- | (Angstrom) |
| Weff (?) : |
347.76 | ------- | (Angstrom) |
| FWHM (?) : |
352.10 | ------- | (Angstrom) |
| Af/AV (?) : |
0.537 | ------- | () |
| Fsun (?) : |
96.69 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
Advanced Baseline Imager(ABI) Transmission components: Filter + Instrumentid:GOES/ABI4.Ch03 | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
8.97083e-10 | (erg/cm2/s/A) |
| |
------- |
2230.92 | (Jy) |
| PhotCal ID (?) : |
GOES/ABI4.Ch03/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
1.46008e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
GOES/ABI4.Ch03/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
9029.78 | (Jy) |
| PhotCal ID (?) : |
GOES/ABI4.Ch03/ST |
| |
|
Filter added: 2020-08-27 20:18:17
Last update: 2021-07-27 19:16:20 | | GOES/ABI4.Ch04 | 13791.15 | 13791.46 | 13790.75 | 13640.77 | 13933.07 | 159.87 | 1323.98 | 2.09e-10 | GOES | GOES-ABI | GOES19 FM4 ABI Ch04 normalized SRF | | GOES/ABI4.Ch05 | 16081.54 | 16083.77 | 16079.15 | 15669.68 | 16485.23 | 448.19 | 1034.38 | 1.2e-10 | GOES | GOES-ABI | GOES19 FM4 ABI Ch05 normalized SRF | | GOES/ABI4.Ch06 | 22421.65 | 22423.03 | 22419.58 | 22051.57 | 22793.74 | 461.58 | 612.77 | 3.65e-11 | GOES | GOES-ABI | GOES19 FM4 ABI Ch06 normalized SRF | | GOES/ABI4.Ch07 | 39051.30 | 39067.72 | 39025.15 | 37525.61 | 40691.02 | 2026.81 | 226.52 | 4.45e-12 | GOES | GOES-ABI | GOES19 FM4 ABI Ch07 normalized SRF | | GOES/ABI4.Ch08 | 61953.89 | 62103.84 | 61719.96 | 56566.50 | 67448.57 | 8175.63 | 95.54 | 7.46e-13 | GOES | GOES-ABI | GOES19 FM4 ABI Ch08 normalized SRF | | GOES/ABI4.Ch09 | 69441.14 | 69474.31 | 69392.34 | 66404.57 | 72843.19 | 3892.82 | 76.47 | 4.75e-13 | GOES | GOES-ABI | GOES19 FM4 ABI Ch09 normalized SRF | | GOES/ABI4.Ch10 | 73333.07 | 73339.99 | 73321.12 | 71870.37 | 74798.36 | 1814.23 | 68.89 | 3.84e-13 | GOES | GOES-ABI | GOES19 FM4 ABI Ch10 normalized SRF | | GOES/ABI4.Ch11 | 84955.94 | 84980.69 | 84912.42 | 82174.43 | 88177.16 | 3510.21 | 51.85 | 2.15e-13 | GOES | GOES-ABI | GOES19 FM4 ABI Ch11 normalized SRF | | GOES/ABI4.Ch12 | 95884.68 | 95906.06 | 95852.71 | 92984.12 | 98978.93 | 3798.70 | 40.97 | 1.34e-13 | GOES | GOES-ABI | GOES19 FM4 ABI Ch12 normalized SRF | | GOES/ABI4.Ch13 | 103146.30 | 103168.58 | 103107.78 | 99358.39 | 107683.41 | 3080.62 | 35.52 | 1.0e-13 | GOES | GOES-ABI | GOES19 FM4 ABI Ch13 normalized SRF | | GOES/ABI4.Ch14 | 111976.95 | 112055.21 | 111845.08 | 105400.03 | 118377.63 | 7392.81 | 30.26 | 7.23e-14 | GOES | GOES-ABI | GOES19 FM4 ABI Ch14 normalized SRF | | GOES/ABI4.Ch15 | 122543.67 | 122652.00 | 122346.05 | 114250.06 | 130210.05 | 9141.00 | 25.30 | 5.05e-14 | GOES | GOES-ABI | GOES19 FM4 ABI Ch15 normalized SRF | | GOES/ABI4.Ch16 | 132842.84 | 132878.15 | 132784.93 | 128789.69 | 137474.15 | 5340.61 | 21.67 | 3.68e-14 | GOES | GOES-ABI | GOES19 FM4 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=8636.7846005128&id=GOES/ABI4.Ch03><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=8634.0742845355&id=GOES/ABI4.Ch03><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=8634.4724527211&id=GOES/ABI4.Ch03><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=8635.6251605178&id=GOES/ABI4.Ch03><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=347.75542215098,8637.6360777494,1&id=GOES/ABI4.Ch03><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}
