HST :The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community. HST/NICMOS3 :The Near Infrared Camera and Multi-Object Spectrometer, Camera 3 |
| HST/NICMOS3.G096 | 10350.2 | 10032.3 | 7848 | 12225 | 2332.5 | 1998.6 | HST | NICMOS | G096 grism for HST NICMOS detector 3 | | HST/NICMOS3.G096 | Filter Description | Filter ID (?) : | HST/NICMOS3.G096 |
| Description (?) : | G096 grism for HST NICMOS detector 3 |
| Phot.System (?) : | ------ |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | HST |
| Instrument (?) : | NICMOS |
| Comments (?) : | Response calculated using the stsynphot python package by STScI. In particular, function stsynphot.band("nicmos,3,g096"). Please, take a look to stsynphot documentation and HST instrument documentation |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λmean (?) : |
10350.22 | ------- | (Angstrom) |
| λcen (?) : |
10549.68 | ------- | (Angstrom) |
| λeff (?) : |
10032.31 | ------- | (Angstrom) |
| λpeak (?) : |
11380.00 | ------- | (Angstrom) |
| λpivot (?) : |
10188.37 | ------- | (Angstrom) |
| λphot (?) : |
10143.20 | ------- | (Angstrom) |
| λmin (?) : |
7847.76 | ------- | (Angstrom) |
| λmax (?) : |
12224.96 | ------- | (Angstrom) |
| Weff (?) : |
2332.51 | ------- | (Angstrom) |
| FWHM (?) : |
2659.59 | ------- | (Angstrom) |
| Af/AV (?) : |
0.43 | ------- | () |
| Fsun (?) : |
------- | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
stsynphot documentation Transmission components: Filter + Instrument | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
5.953e-10 | (erg/cm2/s/A) |
| |
------- |
1998.60 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS3.G096/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
1.082e-9 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS3.G096/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
12190.10 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS3.G096/ST |
| |
|
Filter added: 2019-07-16 12:14:42
Last update: 2020-03-23 12:58:04 | | HST/NICMOS3.F108N | 10799.6 | 10799.0 | 10694 | 10908 | 104.7 | 1945.5 | HST | NICMOS | F108N filter for HST NICMOS detector 3 | | HST/NICMOS3.F113N | 11283.5 | 11283.0 | 11180 | 11388 | 110.6 | 1824.8 | HST | NICMOS | F113N filter for HST NICMOS detector 3 | | HST/NICMOS3.F110W | 11561.0 | 10786.3 | 7827 | 14329 | 3589.5 | 1728.1 | HST | NICMOS | F110W filter for HST NICMOS detector 3 | | HST/NICMOS3.G141 | 15854.9 | 14734.2 | 10598 | 19790 | 5135.8 | 1103.8 | HST | NICMOS | G141 grism for HST NICMOS detector 3 | | HST/NICMOS3.F150W | 15856.2 | 14619.8 | 10565 | 19737 | 5239.7 | 1105.3 | HST | NICMOS | F150W filter for HST NICMOS detector 3 | | HST/NICMOS3.F160W | 16168.9 | 15872.3 | 13628 | 18416 | 3079.3 | 1062.8 | HST | NICMOS | F160W filter for HST NICMOS detector 3 | | HST/NICMOS3.F164N | 16460.4 | 16462.1 | 16297 | 16631 | 177.9 | 1003.2 | HST | NICMOS | F164N filter for HST NICMOS detector 3 | | HST/NICMOS3.F166N | 16583.1 | 16582.5 | 16421 | 16764 | 169.9 | 1048.9 | HST | NICMOS | F166N filter for HST NICMOS detector 3 | | HST/NICMOS3.F187N | 18747.5 | 18746.2 | 18581 | 18926 | 187.6 | 803.8 | HST | NICMOS | F187N filter for HST NICMOS detector 3 | | HST/NICMOS3.F175W | 18890.0 | 16893.6 | 11802 | 23564 | 5802.2 | 844.1 | HST | NICMOS | F175W filter for HST NICMOS detector 3 | | HST/NICMOS3.F190N | 19004.0 | 19003.2 | 18821 | 19203 | 184.7 | 835.5 | HST | NICMOS | F190N filter for HST NICMOS detector 3 | | HST/NICMOS3.F196N | 19640.1 | 19639.8 | 19434 | 19836 | 194.0 | 786.6 | HST | NICMOS | F196N filter for HST NICMOS detector 3 | | HST/NICMOS3.F200N | 19975.0 | 19974.1 | 19774 | 20185 | 208.1 | 768.5 | HST | NICMOS | F200N filter for HST NICMOS detector 3 | | HST/NICMOS3.F212N | 21219.1 | 21216.6 | 20982 | 22394 | 215.3 | 690.2 | HST | NICMOS | F212N filter for HST NICMOS detector 3 | | HST/NICMOS3.G206 | 21348.1 | 20056.1 | 13895 | 25250 | 5644.8 | 687.8 | HST | NICMOS | G206 grism for HST NICMOS detector 3 | | HST/NICMOS3.F215N | 21488.3 | 21485.8 | 21286 | 21681 | 205.0 | 670.6 | HST | NICMOS | F215N filter for HST NICMOS detector 3 | | HST/NICMOS3.F222M | 22193.3 | 22153.5 | 20498 | 23990 | 1499.3 | 633.9 | HST | NICMOS | F222M filter for HST NICMOS detector 3 | | HST/NICMOS3.F240M | 23979.1 | 23924.6 | 22555 | 25329 | 1875.9 | 558.4 | HST | NICMOS | F240M filter for HST NICMOS detector 3 |
|
© SVO, 6356 filters available, Last update: 2020-07-31 | 
 ≡ filter transmission<p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl<li><b>Utype</b>: <i>photdm:PhotometryFilter.SpectralAxis.Coverage.Location.Value</i></ul></td></table>',WIDTH,400)){kind=link}
 ≡ filter transmission<br> Vg(λ) ≡ Vega spectrum<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.SpectralAxis.Coverage.Bounds.Extent</i></ul></td></table>',WIDTH,400)){kind=link}
</b><br><table cellpadding=20><td class=helptd>Zero Point in Vega System.<p>Calculated by the service as:<p><img src=images/latex/zp.png> <p>where:<p> T(λ) ≡ 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>eff</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<p>f(λ) ≡ flux of the spectrum<p><u>Property info:</u><ul><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=10350.215900378&id=HST/NICMOS3.G096><p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:em.wl<li><b>Utype</b>: <i>photdm:PhotometryFilter.SpectralAxis.Coverage.Location.Value</i></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=10032.309595367&id=HST/NICMOS3.G096><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=10188.369504755&id=HST/NICMOS3.G096><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=10143.196569003&id=HST/NICMOS3.G096><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=2332.5087120869,10549.677134816,0.06675399645931938&id=HST/NICMOS3.G096><p><u>Property info:</u><ul><li><b>Unit</b>:Angstrom<li><b>UCD</b>:instr.bandwidth<li><b>Utype</b>: <i>photdm:PhotometryFilter.SpectralAxis.Coverage.Bounds.Extent</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>eff</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/extinctionlaw.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>Sun spectrum from calspec database: sun_reference_stis_002 with with sun_mod_001 for larger wavelengths.<p><img src=images/sunspec.png><p><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>eff</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>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}