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I think what I'm technically computing are "rotational light curves", not phase curves, since the phase of a planet refers specifically to the illumination pattern due to the star, which doesn't matte…
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```2017-10-27 00:23:36,130 ERROR [17824:MainThread:__init__.py:432] Task=46394980-c387-4882-8eda-00e4d9d9cf00 failed.
args=[{u'modtime': u'2017-10-27T00:23:26.020239Z', u'bibcode': u'1963JNuM.…
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In the Rayleigh-Jeans limit, the PPO depth scales as T_p R_p^2/(L_*^{1/4} R_*^{3/2}). So, for fixed planet properties & stellar luminosity, a smaller star has a larger depth. If TRAPPIST-1A were a W…
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I forgot to mention: we should look into mid-infrared observations from the ground (this is important if we want to justify JWST time - one shouldn't be able to make a measurement from the ground). …
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HI @brantr, Changes and additions in **BOLD** ... rest is for context. Please let me know if you prefer me to make these changes directly. @daranorman
3.1.1 AGN Selection from LSST Data
AGN-1. …
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Merge two concepts with similar names:
Observational astronomy
> Methods
>> Infrared astronomy
>>>Far infrared astronomy
>>> Far-infrared astronomy
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### Trillian Data Needs
This document will describe the data needs in detail for the [Trillian project](http://trillianverse.com). Trillian is an attempt to address the difficulty (or inability) to e…
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The raw data should be kept raw and archived immediately. This is the data which shall not be overwritten or modified. This is the data others will want, and against which your choice of subsequent an…
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_From [andre.knoerig@gmail.com](https://code.google.com/u/andre.knoerig@gmail.com/) on October 22, 2009 03:54:19_
This is a space for Fritzing users to upload and share their self-created
parts with…