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 1id:HST/NICMOS1.a → GaiaXPy base XML file. You can download here the GaiaXPy base XML file for the full HST/NICMOS1 filter set. Please, take a look to the GaiaXPy web page and additional documentation for more information. |
| HST/NICMOS1.F090M | 9034.55 | 9085.81 | 9006.59 | 7849.37 | 10140.93 | 1222.43 | 2243.34 | 8.24e-10 | HST | NICMOS | F090M filter for HST NICMOS detector 1 | | HST/NICMOS1.F095N | 9537.25 | 9537.41 | 9536.04 | 9448.33 | 9631.76 | 92.43 | 2030.39 | 6.69e-10 | HST | NICMOS | F095N filter for HST NICMOS detector 1 | | HST/NICMOS1.F097N | 9717.24 | 9717.42 | 9717.06 | 9626.15 | 9821.00 | 95.74 | 2242.25 | 7.12e-10 | HST | NICMOS | F097N filter for HST NICMOS detector 1 | | HST/NICMOS1.POL0S | 10564.84 | 10804.79 | 10308.19 | 7956.14 | 13124.74 | 3264.82 | 1956.24 | 5.25e-10 | HST | NICMOS | POL0S polarizer for HST NICMOS detector 1 | | HST/NICMOS1.POL240S | 10564.84 | 10804.79 | 10308.19 | 7956.14 | 13124.74 | 3264.82 | 1956.24 | 5.25e-10 | HST | NICMOS | POL240S polarizer for HST NICMOS detector 1 | | HST/NICMOS1.POL120S | 10564.84 | 10804.79 | 10308.19 | 7956.14 | 13124.74 | 3264.82 | 1956.24 | 5.25e-10 | HST | NICMOS | POL120S polarizer for HST NICMOS detector 1 | | HST/NICMOS1.F108N | 10816.12 | 10816.29 | 10815.64 | 10713.30 | 10923.79 | 103.18 | 1907.05 | 4.89e-10 | HST | NICMOS | F108N filter for HST NICMOS detector 1 | | HST/NICMOS1.F110M | 11018.17 | 11065.40 | 10959.75 | 9698.29 | 12355.19 | 1786.94 | 1856.10 | 4.58e-10 | HST | NICMOS | F110M filter for HST NICMOS detector 1 | | HST/NICMOS1.F110M | Filter Description | Filter ID (?) : | HST/NICMOS1.F110M |
| Description (?) : | F110M filter for HST NICMOS detector 1 |
| Phot.System (?) : | NICMOS1 |
| 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,f110m"). Please, take a look to stsynphot documentation and HST instrument documentation |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
11018.17 | ------- | (Angstrom) |
| λmean (?) : |
11065.40 | ------- | (Angstrom) |
| λcen (?) : |
11032.79 | ------- | (Angstrom) |
| λeff (?) : |
10959.75 | ------- | (Angstrom) |
| λpeak (?) : |
11300.00 | ------- | (Angstrom) |
| λpivot (?) : |
11018.17 | ------- | (Angstrom) |
| λphot (?) : |
10991.42 | ------- | (Angstrom) |
| λmin (?) : |
9698.29 | ------- | (Angstrom) |
| λmax (?) : |
12355.19 | ------- | (Angstrom) |
| Weff (?) : |
1786.94 | ------- | (Angstrom) |
| FWHM (?) : |
1971.48 | ------- | (Angstrom) |
| Af/AV (?) : |
0.369 | ------- | () |
| Fsun (?) : |
58.72 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
stsynphot documentation Transmission components: Filter + CCD + Instrumentid:HST/NICMOS1.F110M
You can download here the GaiaXPy base XML file for the full HST/NICMOS1 filter set.
Please, take a look to GaiaXPy documentation for more information. - GaiaXPy base XML file. | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
4.58355e-10 | (erg/cm2/s/A) |
| |
------- |
1856.10 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS1.F110M/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
8.96661e-10 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS1.F110M/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
14703.62 | (Jy) |
| PhotCal ID (?) : |
HST/NICMOS1.F110M/ST |
| |
|
Filter added: 2019-07-16 12:14:24
Last update: 2022-03-01 15:19:20 | | HST/NICMOS1.F113N | 11297.69 | 11297.87 | 11297.41 | 11193.83 | 11402.49 | 110.71 | 1793.06 | 4.21e-10 | HST | NICMOS | F113N filter for HST NICMOS detector 1 | | HST/NICMOS1.F110W | 11233.62 | 11579.82 | 10826.77 | 7848.73 | 14335.73 | 3632.25 | 1829.18 | 4.35e-10 | HST | NICMOS | F110W filter for HST NICMOS detector 1 | | HST/NICMOS1.F145M | 14548.35 | 14583.78 | 14498.86 | 13293.05 | 15868.87 | 1713.74 | 1222.24 | 1.73e-10 | HST | NICMOS | F145M filter for HST NICMOS detector 1 | | HST/NICMOS1.F140W | 14268.28 | 14830.60 | 13473.20 | 9763.96 | 18467.54 | 4592.30 | 1348.06 | 1.99e-10 | HST | NICMOS | F140W filter for HST NICMOS detector 1 | | HST/NICMOS1.F160W | 16036.90 | 16163.52 | 15867.12 | 13646.65 | 18419.13 | 3097.78 | 1063.08 | 1.24e-10 | HST | NICMOS | F160W filter for HST NICMOS detector 1 | | HST/NICMOS1.F164N | 16460.00 | 16460.31 | 16461.92 | 16297.18 | 16630.81 | 178.00 | 981.07 | 1.09e-10 | HST | NICMOS | F164N filter for HST NICMOS detector 1 | | HST/NICMOS1.F165M | 16480.20 | 16512.03 | 16439.37 | 15252.96 | 17782.41 | 1710.72 | 1004.50 | 1.11e-10 | HST | NICMOS | F165M filter for HST NICMOS detector 1 | | HST/NICMOS1.F166N | 16606.26 | 16606.57 | 16605.81 | 16444.61 | 16784.53 | 172.45 | 1024.50 | 1.11e-10 | HST | NICMOS | F166N filter for HST NICMOS detector 1 | | HST/NICMOS1.F170M | 17058.03 | 17089.47 | 17020.35 | 15807.57 | 18372.85 | 1789.73 | 959.99 | 9.89e-11 | HST | NICMOS | F170M filter for HST NICMOS detector 1 | | HST/NICMOS1.F187N | 18749.56 | 18749.96 | 18748.53 | 18580.62 | 18926.44 | 188.27 | 785.30 | 6.7e-11 | HST | NICMOS | F187N filter for HST NICMOS detector 1 | | HST/NICMOS1.F190N | 18989.42 | 18989.93 | 18988.80 | 18808.48 | 19176.78 | 186.03 | 817.03 | 6.79e-11 | HST | NICMOS | F190N filter for HST NICMOS detector 1 |
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 ≡ 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=11065.397312998&id=HST/NICMOS1.F110M><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=10959.751477674&id=HST/NICMOS1.F110M><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=11018.165600718&id=HST/NICMOS1.F110M><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=10991.4249422&id=HST/NICMOS1.F110M><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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=1786.9381735613,11032.793294519,1&id=HST/NICMOS1.F110M><p>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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>Filter transmission is transformed to "<i>energy counter</i>" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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>Filter transmission is transformed to \"<i>energy counter</i>\" for these calculations, that is, the photon count transmission is multiplied by λ and normalized so that peak transmission is equal to 1.<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}
