| GOES/Imager11.VIS_d1 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 1 normalized SRF |
| GOES/Imager11.VIS_d2 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 2 normalized SRF |
| GOES/Imager11.VIS_d3 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 3 normalized SRF |
| GOES/Imager11.VIS_d4 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 4 normalized SRF |
| GOES/Imager11.VIS_d5 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 5 normalized SRF |
| GOES/Imager11.VIS_d6 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 6 normalized SRF |
| GOES/Imager11.VIS_d7 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 7 normalized SRF |
| GOES/Imager11.VIS_d8 | 6449.87 | 6576.76 | 6317.41 | 5080.00 | 8200.00 | 2262.36 | 3090.69 | 2.23e-9 | GOES | GOES-Imager | GOES11 Imager VIS Channel, detector 8 normalized SRF |
| GOES/Imager11.IR2_d1s1 | 39060.50 | 39081.38 | 39026.00 | 37522.00 | 40739.80 | 2365.94 | 226.27 | 4.45e-12 | GOES | GOES-Imager | GOES11 Imager IR Channel 2, detector 1 side 1 normalized SRF |
| GOES/Imager11.IR2_d1s2 | 39060.50 | 39081.38 | 39026.00 | 37522.00 | 40739.80 | 2365.94 | 226.27 | 4.45e-12 | GOES | GOES-Imager | GOES11 Imager IR Channel 2, detector 1 side 2 normalized SRF |
| GOES/Imager11.IR2_d2s1 | 39060.50 | 39081.38 | 39026.00 | 37522.00 | 40739.80 | 2365.94 | 226.27 | 4.45e-12 | GOES | GOES-Imager | GOES11 Imager IR Channel 2, detector 2 side 1 normalized SRF |
| GOES/Imager11.IR2_d2s2 | 39060.50 | 39081.38 | 39026.00 | 37522.00 | 40739.80 | 2365.94 | 226.27 | 4.45e-12 | GOES | GOES-Imager | GOES11 Imager IR Channel 2, detector 2 side 2 normalized SRF |
| GOES/Imager11.IR3_d1s1 | 67526.45 | 67588.20 | 67425.85 | 64065.60 | 71174.40 | 5353.70 | 80.85 | 5.32e-13 | GOES | GOES-Imager | GOES11 Imager IR Channel 3, detector 1 side 1 normalized SRF |
| GOES/Imager11.IR3_d1s2 | 67526.45 | 67588.20 | 67425.85 | 64065.60 | 71174.40 | 5353.70 | 80.85 | 5.32e-13 | GOES | GOES-Imager | GOES11 Imager IR Channel 3, detector 1 side 2 normalized SRF |
| GOES/Imager11.IR4_d1s1 | 107383.47 | 107511.82 | 107175.89 | 101112.00 | 113895.00 | 9553.08 | 32.90 | 8.55e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 4, detector 1 side 1 normalized SRF |
| GOES/Imager11.IR4_d1s2 | 107383.47 | 107511.82 | 107175.89 | 101112.00 | 113895.00 | 9553.08 | 32.90 | 8.55e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 4, detector 1 side 2 normalized SRF |
| GOES/Imager11.IR4_d2s1 | 107383.47 | 107511.82 | 107175.89 | 101112.00 | 113895.00 | 9553.08 | 32.90 | 8.55e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 4, detector 2 side 1 normalized SRF |
| GOES/Imager11.IR4_d2s2 | 107383.47 | 107511.82 | 107175.89 | 101112.00 | 113895.00 | 9553.08 | 32.90 | 8.55e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 4, detector 2 side 2 normalized SRF |
| GOES/Imager11.IR5_d1s1 | 120142.08 | 120236.79 | 119981.34 | 114181.00 | 127389.00 | 8487.00 | 26.39 | 5.48e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 5, detector 1 side 1 normalized SRF |
| GOES/Imager11.IR5_d2s2 | 120204.95 | 120297.52 | 120047.60 | 114220.00 | 127356.00 | 8245.09 | 26.36 | 5.47e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 5, detector 2 side 2 normalized SRF |
| GOES/Imager11.IR5_d2s1 | 120219.31 | 120313.22 | 120059.64 | 114220.00 | 127372.00 | 8318.45 | 26.35 | 5.47e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 5, detector 2 side 1 normalized SRF |
| GOES/Imager11.IR5_d2s1 | Filter Description | Filter ID (?) : | GOES/Imager11.IR5_d2s1 |
| Description (?) : | GOES11 Imager IR Channel 5, detector 2 side 1 normalized SRF |
| Phot.System (?) : | GOES-Imager |
| Detector Type (?) : | Energy counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | GOES |
| Instrument (?) : | GOES-Imager |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
120219.31 | ------- | (Angstrom) |
| λmean (?) : |
120313.22 | ------- | (Angstrom) |
| λcen (?) : |
120429.97 | ------- | (Angstrom) |
| λeff (?) : |
120059.64 | ------- | (Angstrom) |
| λpeak (?) : |
120351.00 | ------- | (Angstrom) |
| λpivot (?) : |
120219.31 | ------- | (Angstrom) |
| λphot (?) : |
120121.47 | ------- | (Angstrom) |
| λmin (?) : |
114220.00 | ------- | (Angstrom) |
| λmax (?) : |
127372.00 | ------- | (Angstrom) |
| Weff (?) : |
8318.45 | ------- | (Angstrom) |
| FWHM (?) : |
9117.53 | ------- | (Angstrom) |
| Af/AV (?) : |
0.0368 | ------- | () |
| Fsun (?) : |
0.0118 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
OSPO: GOES Transmission components: Filter + Instrumentid:GOES/Imager11.IR5_d2s1 | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
5.46649e-14 | (erg/cm2/s/A) |
| |
------- |
26.35 | (Jy) |
| PhotCal ID (?) : |
GOES/Imager11.IR5_d2s1/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
7.53179e-12 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
GOES/Imager11.IR5_d2s1/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
1750467.44 | (Jy) |
| PhotCal ID (?) : |
GOES/Imager11.IR5_d2s1/ST |
| |
|
Filter added: 2020-08-27 12:20:55
Last update: 2021-07-27 19:16:48 |
| GOES/Imager11.IR5_d1s2 | 120233.04 | 120326.22 | 120074.58 | 114220.00 | 127372.00 | 8217.47 | 26.35 | 5.46e-14 | GOES | GOES-Imager | GOES11 Imager IR Channel 5, detector 1 side 2 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=120313.22476768&id=GOES/Imager11.IR5_d2s1><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=120059.64041622&id=GOES/Imager11.IR5_d2s1><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=120219.31424232&id=GOES/Imager11.IR5_d2s1><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=120121.46922192&id=GOES/Imager11.IR5_d2s1><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=8318.4538864166,120429.96670274,1&id=GOES/Imager11.IR5_d2s1><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}
