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| − | =[[Photometry]]=
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| − | A discussion of what photometry is and why you would want to do it. Includes where to find already-reduced Spitzer photometry.
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| − | Also see [[Aperture photometry using APT]].
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| − | =[[Units]]=
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| − | If you've done photometry before and expect to do it the same way here, BE CAREFUL because IT WILL NOT WORK. The units of Spitzer images can be tricky. This page has a lot of information about these units and how to convert them into more familiar units.
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| − | =[[Color-Magnitude and Color-Color plots]]=
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| − | A general discussion of color-magnitude and color-color plots.
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| − | =[[SED plots]]=
| + | =[[I%27m_ready_to_advance_to_a_highly_technical_and_in-depth_discussion_on_processing_Spitzer_data.|Making a mosaic from the BCDs]]= |
| − | A general discussion of spectral energy distribution (SED) plots.
| + | very skeletal, more to come eventually |
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| − | =[[Make_a_simple_mosaic|Making a simple mosaic]] (with Spitzer data and tools) =
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| − | This page describes how to make a simple mosaic by combining post-BCD mosaics from more than 1 AOR into one large mosaic.
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| − | =[[Making Mosaics Using MONTAGE]]=
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| − | MONTAGE is a software package that allows you to make mosaics from any set of astronomical images (e.g., not just Spitzer images).
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| − | =[[I%27m_ready_to_advance_to_a_highly_technical_and_in-depth_discussion_on_downloading_Spitzer_data.|Making a mosaic from the BCDs]]= | |
| − | to come | |
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| − | =[[Accessing Kepler and CoRoT data]]=
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| − | Kepler and CoRoT data are much more than just exoplanets, but of course they're in here too.
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| − | =[[What is a periodogram?]]=
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| − | Information on periodograms -- what they are, why you care about them, and how to use NStED's tool for determining them.
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| − | =[[Studying Young Stars]]=
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| − | More information on the study of young stars, not necessarily specifically Spitzer-related.
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| − | =[[Working with L1688]]=
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| − | An entire chain of analysis for Lynds 1688 (a star-forming region), start to finish.
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| − | =[[Studying Variable Stars]]=
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| − | More information on the study of variable stars, light curves, eclipsing binaries, etc.
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