TBD for 2019!!

Data locations
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Near-infrared 3.6um
 /d/crow1/edges/data/nir/mosaic/   Mosaics with foreground stars
 /d/crow1/edges/data/nir/masked/   Edited for major foreground stars (but just a subset so far)
Optical
 /d/crow1/edges/data/opt/vanzee/   See README for which are star edited
 /d/pawnee3/davec/LVLbroadband/Data/optical/*/star_edit/ 
 /d/pawnee3/davec/LVLbroadband/Data/sdss/star_edit/ 
Far-Ultraviolet
 /d/crow1/edges/data/uv/
 /d/pawnee3/davec/LVLbroadband/Data/UV/FUV
Mid-infrared 22um or 24um
 /d/pawnee3/davec/LVLbroadband/Data/IR/
 Otherwise grab 22um W4 WISE images http://irsa.ipac.caltech.edu/applications/wise/

By June 18
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1. Process initial ugr data to OTZF, align/stack, and WCS.
2. Calibrate initial ugr stacks via SDSS imaging.
3. Divvy up ~2 galaxies to each person.  
4. Carry out ellipse fitting on your 3.6um mosaics.

By June 25
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1. Carry out ellipse fitting on FUV and 24um.
2. Make multi-wavelength surface brightness profile plots using FUV, 3.6um, 24um

By June 30
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1. Process next set of ugr data to OTZF, align/stack, and WCS.
2. Calibrate next set of ugr stacks via SDSS imaging.

By July 06
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1. Carry out ellipse fitting on optical data (ugr and/or UBVR).
2. Correct s.b. profiles for dust attenuation

By July 12
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1. Foreground star subtractions from images (if necessary).
2. Smooth star-edited stacks to have 6" PSFs
3. Redo ellipse fits (your script machinery should already be set; just copy and paste to redo)
4. Learn how to use CIGALE code to find best-fit age as function of radius in your galaxies.

July 23 to July 27
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1. Carry out CIGALE fits
2. Work on posters.  Include plots of:
 a. Multi-wavelength surface brightness profiles
 b. Age vs radius plots of your three galaxies
 c. Comparison of ensemble slopes in age vs radius plots 
3. Optional: (learn how to) create a webpage of your REU experience