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/NICMOS1 :The Near Infrared Camera and Multi-Object Spectrometer, Camera 1 |
| HST/NICMOS1.F090M | 9086.0 | 9008.5 | 7843 | 10133 | 1222.6 | 2252.8 | HST | NICMOS | F090M filter for HST NICMOS detector 1 | | HST/NICMOS1.F095N | 9536.2 | 9534.1 | 9448 | 9631 | 93.4 | 2047.2 | HST | NICMOS | F095N filter for HST NICMOS detector 1 | | HST/NICMOS1.F097N | 9714.3 | 9713.6 | 9626 | 9821 | 96.4 | 2275.2 | HST | NICMOS | F097N filter for HST NICMOS detector 1 | | HST/NICMOS1.POL240S | 10804.9 | 10312.7 | 7942 | 13109 | 3265.0 | 1889.0 | HST | NICMOS | POL240S polarizer for HST NICMOS detector 1 | | HST/NICMOS1.POL120S | 10804.9 | 10312.7 | 7942 | 13109 | 3265.0 | 1889.0 | HST | NICMOS | POL120S polarizer for HST NICMOS detector 1 | | HST/NICMOS1.POL0S | 10804.9 | 10312.7 | 7942 | 13109 | 3265.0 | 1889.0 | HST | NICMOS | POL0S polarizer for HST NICMOS detector 1 | | HST/NICMOS1.F108N | 10815.9 | 10815.3 | 10713 | 10924 | 103.4 | 1937.0 | HST | NICMOS | F108N filter for HST NICMOS detector 1 | | HST/NICMOS1.F110M | 11065.4 | 10960.8 | 9684 | 12346 | 1787.1 | 1864.7 | HST | NICMOS | F110M filter for HST NICMOS detector 1 | | HST/NICMOS1.F113N | 11297.8 | 11297.4 | 11194 | 11402 | 110.7 | 1821.0 | HST | NICMOS | F113N filter for HST NICMOS detector 1 | | HST/NICMOS1.F110W | 11580.0 | 10832.8 | 7826 | 14328 | 3632.4 | 1725.7 | HST | NICMOS | F110W filter for HST NICMOS detector 1 | | HST/NICMOS1.F110W | Filter Description | Filter ID (?) : | HST/NICMOS1.F110W |
| Description (?) : | F110W filter for HST NICMOS detector 1 |
| 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,1,f110w"). Please, take a look to stsynphot documentation and HST instrument documentation |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λmean (?) : |
11580.04 | ------- | (Angstrom) |
| λcen (?) : |
11326.57 | ------- | (Angstrom) |
| λeff (?) : |
10832.80 | ------- | (Angstrom) |
| λpeak (?) : |
13430.00 | ------- | (Angstrom) |
| λpivot (?) : |
11233.77 | ------- | (Angstrom) |
| λphot (?) : |
11072.51 | ------- | (Angstrom) |
| λmin (?) : |
7826.29 | ------- | (Angstrom) |
| λmax (?) : |
14328.23 | ------- | (Angstrom) |
| Weff (?) : |
3632.45 | ------- | (Angstrom) |
| FWHM (?) : |
5261.84 | ------- | (Angstrom) |
| Af/AV (?) : |
0.38 | ------- | () |
| 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 (?) : |
------- |
4.409e-10 | (erg/cm2/s/A) |
| |
------- |
1725.73 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS1.F110W/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
9.276e-10 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS1.F110W/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
14213.04 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS1.F110W/ST |
| |
|
Filter added: 2019-07-16 12:14:24
Last update: 2020-03-23 12:58:04 | | HST/NICMOS1.F145M | 14583.8 | 14498.9 | 13283 | 15861 | 1713.9 | 1238.7 | HST | NICMOS | F145M filter for HST NICMOS detector 1 | | HST/NICMOS1.F140W | 14830.9 | 13479.9 | 9711 | 18466 | 4592.8 | 1225.7 | HST | NICMOS | F140W filter for HST NICMOS detector 1 | | HST/NICMOS1.F160W | 16163.8 | 15868.4 | 13629 | 18416 | 3098.1 | 1063.3 | HST | NICMOS | F160W filter for HST NICMOS detector 1 | | HST/NICMOS1.F164N | 16460.4 | 16462.1 | 16297 | 16631 | 178.0 | 1003.2 | HST | NICMOS | F164N filter for HST NICMOS detector 1 | | HST/NICMOS1.F165M | 16512.1 | 16439.8 | 15247 | 17781 | 1710.9 | 1021.7 | HST | NICMOS | F165M filter for HST NICMOS detector 1 | | HST/NICMOS1.F166N | 16607.1 | 16606.3 | 16444 | 16784 | 172.7 | 1047.6 | HST | NICMOS | F166N filter for HST NICMOS detector 1 | | HST/NICMOS1.F170M | 17089.5 | 17020.4 | 15799 | 18371 | 1789.8 | 977.5 | HST | NICMOS | F170M filter for HST NICMOS detector 1 | | HST/NICMOS1.F187N | 18748.3 | 18747.0 | 18581 | 18926 | 187.6 | 803.8 | HST | NICMOS | F187N filter for HST NICMOS detector 1 | | HST/NICMOS1.F190N | 18986.1 | 18985.5 | 18808 | 19177 | 185.3 | 836.4 | HST | NICMOS | F190N filter for HST NICMOS detector 1 |
|
© 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=11580.041572892&id=HST/NICMOS1.F110W><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=10832.798836552&id=HST/NICMOS1.F110W><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=11233.768129907&id=HST/NICMOS1.F110W><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=11072.509656099&id=HST/NICMOS1.F110W><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=3632.445488163,11326.570824115,0.14354228892643703&id=HST/NICMOS1.F110W><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}