BOOMERANG :BOOMERANG (Balloon Observations of Millimetric Extragalactic Radiation and Geophysics) is a balloon-borne microwave telescope designed to map the cosmic microwave background BOOMERANG/LDB :BOOMERANG is a balloon-borne microwave telescope designed to map the cosmic microwave background at a resolution of 10' from the Long Duration Balloon (LDB) platform.id:BOOMERANG/LDB.a |
| BOOMERANG/LDB.410GHz | 7.28e+6 | 7.29e+6 | 7.27e+6 | 6.89e+6 | 7.7e+6 | 453276.17 | 0.00663 | 3.75e-21 | BOOMERANG | BOOMERANG | BOOMERANG LDB 410GHz normalized response | | BOOMERANG/LDB.240GHz | 1.27e+7 | 1.29e+7 | 1.25e+7 | 1.05e+7 | 1.55e+7 | 2.56e+6 | 0.00218 | 4.02e-22 | BOOMERANG | BOOMERANG | BOOMERANG LDB 240GHz normalized response | | BOOMERANG/LDB.150GHz | 1.88e+7 | 1.89e+7 | 1.86e+7 | 1.62e+7 | 2.21e+7 | 3.27e+6 | 0.000981 | 8.36e-23 | BOOMERANG | BOOMERANG | BOOMERANG LDB 150GHz normalized response | | BOOMERANG/LDB.90GHz | 3.43e+7 | 3.46e+7 | 3.38e+7 | 2.9e+7 | 4.14e+7 | 5.27e+6 | 0.00029 | 7.38e-24 | BOOMERANG | BOOMERANG | BOOMERANG LDB 90GHz normalized response |
| Filter Plots
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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}
