LaSilla :La Silla ESO Observatory LaSilla/TIMMI2 :TIMMI (Thermal Infrared MultiMode Instrument) was a combined camera and spectrometer installed on the ESO 3.6-metre telescope at La Silla.id:LaSilla/TIMMI2.a |
| LaSilla/TIMMI2.NB790 | 77916.51 | 78009.08 | 77779.35 | 72711.22 | 83814.12 | 6998.02 | 61.21 | 3.02e-13 | La Silla | TIMMI2 | TIMMI2 NB7.9 (filter only) | | LaSilla/TIMMI2.N1 | 86956.30 | 87175.58 | 86599.76 | 79679.52 | 95143.48 | 11485.83 | 49.80 | 1.97e-13 | La Silla | TIMMI2 | TIMMI2 N1 (filter only) | | LaSilla/TIMMI2.NB890 | 87310.83 | 87409.58 | 87149.08 | 81354.44 | 93055.28 | 7476.76 | 49.20 | 1.94e-13 | La Silla | TIMMI2 | TIMMI2 NB8.9 (filter only) | | LaSilla/TIMMI2.NB980 | 96757.35 | 96881.51 | 96559.14 | 90637.18 | 103498.12 | 9001.39 | 40.36 | 1.29e-13 | La Silla | TIMMI2 | TIMMI2 NB9.8 (filter only) | | LaSilla/TIMMI2.NB104 | 103775.09 | 103917.28 | 103539.30 | 96067.42 | 111980.00 | 9991.27 | 35.21 | 9.8e-14 | La Silla | TIMMI2 | TIMMI2 NB10.4 (filter only) | | LaSilla/TIMMI2.SiV | 104469.90 | 104474.20 | 104459.40 | 102871.58 | 106118.48 | 1611.79 | 34.45 | 9.46e-14 | La Silla | TIMMI2 | TIMMI2 SiV (filter only) | | LaSilla/TIMMI2.N2 | 106715.81 | 106975.74 | 106287.06 | 97782.81 | 116867.45 | 13477.42 | 33.41 | 8.8e-14 | La Silla | TIMMI2 | TIMMI2 N2 (filter only) | | LaSilla/TIMMI2.IRWBP | 106859.02 | 107623.91 | 105608.40 | 93404.65 | 122233.36 | 23557.40 | 33.75 | 8.86e-14 | La Silla | TIMMI2 | TIMMI2 IRWBP (filter only) | | LaSilla/TIMMI2.NB119 | 116523.98 | 116679.42 | 116273.89 | 108030.00 | 124472.27 | 11266.46 | 28.05 | 6.19e-14 | La Silla | TIMMI2 | TIMMI2 NB11.9 (filter only) | | LaSilla/TIMMI2.SiC | 117647.33 | 118231.13 | 116673.54 | 100307.42 | 133859.79 | 21181.10 | 27.76 | 6.01e-14 | La Silla | TIMMI2 | TIMMI2 SiC (filter only) | | LaSilla/TIMMI2.NB129 | 123425.59 | 123593.67 | 123146.30 | 114000.00 | 133950.00 | 11678.86 | 25.05 | 4.93e-14 | La Silla | TIMMI2 | TIMMI2 NB12.9 (filter only) | | LaSilla/TIMMI2.NeII | 127899.41 | 127907.18 | 127859.90 | 125580.98 | 130558.57 | 2156.84 | 23.31 | 4.27e-14 | La Silla | TIMMI2 | TIMMI2 NeII (filter only) | | LaSilla/TIMMI2.Q1 | 177164.49 | 177247.25 | 177027.21 | 167496.17 | 187839.30 | 8600.37 | 12.24 | 1.17e-14 | La Silla | TIMMI2 | TIMMI2 Q1 (filter only) | | LaSilla/TIMMI2.Q1 | Filter Description | Filter ID (?) : | LaSilla/TIMMI2.Q1 |
| Description (?) : | TIMMI2 Q1 (filter only) |
| Phot.System (?) : | TIMMI2 |
| Detector Type (?) : | Photon counter |
| Band Name (?) : | ------ |
| Obs. Facility (?) : | La Silla |
| Instrument (?) : | TIMMI2 |
| Comments (?) : | ------ |
| | Mathematical properties | Property | Calculated | Specified | Unit | | λref (?) : |
177164.49 | ------- | (Angstrom) |
| λmean (?) : |
177247.25 | ------- | (Angstrom) |
| λcen (?) : |
177187.15 | ------- | (Angstrom) |
| λeff (?) : |
177027.21 | ------- | (Angstrom) |
| λpeak (?) : |
176980.00 | ------- | (Angstrom) |
| λpivot (?) : |
177164.49 | ------- | (Angstrom) |
| λphot (?) : |
177082.16 | ------- | (Angstrom) |
| λmin (?) : |
167496.17 | ------- | (Angstrom) |
| λmax (?) : |
187839.30 | ------- | (Angstrom) |
| Weff (?) : |
8600.37 | ------- | (Angstrom) |
| FWHM (?) : |
8199.47 | ------- | (Angstrom) |
| Af/AV (?) : |
0.0275 | ------- | () |
| Fsun (?) : |
0.00253 | ------- | (erg/cm2/s/A) |
| Transmission
Data file: ascii, VOTable Reference for filter response:
ESO: WFI Transmission components: Filterid:LaSilla/TIMMI2.Q1 | | Calibration properties
Vega System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
1.16931e-14 | (erg/cm2/s/A) |
| |
------- |
12.24 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
LaSilla/TIMMI2.Q1/Vega |
| |
AB System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.46812e-12 | (erg/cm2/s/A) |
| |
------- |
3631.00 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
LaSilla/TIMMI2.Q1/AB |
| |
ST System | Property | Specified | Calculated | Unit | | Zero Point (?) : |
------- |
3.631e-9 | (erg/cm2/s/A) |
| |
------- |
3801534.30 | (Jy) |
| ZP Type (?) : |
Pogson |
| PhotCal ID (?) : |
LaSilla/TIMMI2.Q1/ST |
| |
|
Filter added: 2020-01-15 18:59:29
Last update: 2021-07-27 20:08:22 | | LaSilla/TIMMI2.Q2 | 187396.94 | 187472.38 | 187270.73 | 177573.76 | 196589.80 | 8860.81 | 10.96 | 9.35e-15 | La Silla | TIMMI2 | TIMMI2 Q2 (filter only) |
|
| 
 ≡ 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=177247.24670806&id=LaSilla/TIMMI2.Q1><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=177027.21275061&id=LaSilla/TIMMI2.Q1><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=177164.49275992&id=LaSilla/TIMMI2.Q1><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=177082.15854637&id=LaSilla/TIMMI2.Q1><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=8600.3718368551,177187.1494007,1&id=LaSilla/TIMMI2.Q1><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}
