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main:grb_observing [2014/11/06 01:46] bruce |
main:grb_observing [2021/01/12 00:50] (current) |
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| ====== Observing GRBs ====== | ====== Observing GRBs ====== | ||
| + | ---- | ||
| - | + | ====== Space Backgrounds | |
| - | ====== Space Backgrounds | + | ---- |
| - | ====== Space Environment ====== | + | |
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| + | ===== Diffuse X-ray Background ===== | ||
| - | ====== Cosmic Backgrounds ====== | + | ===== Diffuse |
| - | + | ||
| - | ===== X-ray ===== | + | |
| - | + | ||
| - | ===== UV background ===== | + | |
| is given in [[Media: | is given in [[Media: | ||
| - | ===== Optical-IR background ===== | + | ===== Diffuse |
| My favorite plot of space (zodiacal) background opt-NIR is the one by Michael Lampton (though I think aldering' | My favorite plot of space (zodiacal) background opt-NIR is the one by Michael Lampton (though I think aldering' | ||
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| </ul> | </ul> | ||
| </ul> | </ul> | ||
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| ====== X-ray Observations ====== | ====== X-ray Observations ====== | ||
| - | + | ---- | |
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| - | ====== X-ray Energy Band Selection | + | ===== X-ray Energy Band Selection ===== |
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| - | ======= How Far to Integrate Down in Energy ======+ | + | ==== How Far to Integrate Down in Energy ==== |
| - | ======= How far to integrate up in energy | + | |
| + | ==== How far to integrate up in energy | ||
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| Note that the SGRB are still rising at the highest energy while the LGRB is flattening. | Note that the SGRB are still rising at the highest energy while the LGRB is flattening. | ||
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| + | ---- | ||
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| + | ===== What about integrating down? ===== | ||
| + | | ||
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| + | How far down should one go in energy before this is not favorable increase in S/N? | ||
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| + | {{ : | ||
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| + | {{ : | ||
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| + | So, its quite clear that you still get photons for BOTH spectra in this idealized picture. | ||
| ====== Optical Observations ====== | ====== Optical Observations ====== | ||
| + | ---- | ||
| - | ====== Lya Forest Spectroscopy | + | |
| + | ===== Lya Forest Spectroscopy ===== | ||
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| http:// | http:// | ||
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