Me with the Magellanic Clouds in the background! |
This past summer I worked exclusively with processed data to make 3D tomographic maps of the high redshift IGM. I hadn’t looked at spectra much, so on my trip to the Magellan telescopes I was hoping to learn more about the properties of the galaxy spectra used in making tomographic maps. I was also really excited to learn about observing in general, as this was my first observing run.
I ended up most enjoying the time I spent in the Baade control room, learning about the interface and the procedures and strategies involved in observing. I learned about spectroscopic calibrations and was then able to take some on my own! I also learned about taking twilight flats, which are useful for getting calibration frames in the UV (as our targets are UV-bright galaxies). Several other highlights of my experience at LCO include holding (a broken version of) a grism customized for our targets, seeing an IMACS slitmask packed with spectra, and watching the telescope move.
I ended up most enjoying the time I spent in the Baade control room, learning about the interface and the procedures and strategies involved in observing. I learned about spectroscopic calibrations and was then able to take some on my own! I also learned about taking twilight flats, which are useful for getting calibration frames in the UV (as our targets are UV-bright galaxies). Several other highlights of my experience at LCO include holding (a broken version of) a grism customized for our targets, seeing an IMACS slitmask packed with spectra, and watching the telescope move.
Visiting LCO was amazing! I very much enjoyed learning about how the data I used was taken. And on the non-astronomy side of things, I got to see some interesting animals (like the viscacha shown in the low-quality photo below).
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