Difference between revisions of "Measuring distances on images"
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=Most coherent, developed, tested materials= | =Most coherent, developed, tested materials= | ||
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[[Finding the diameter of a region we care about]] -- Dr. Luisa Rebull, 2018, for the Ceph-C team | [[Finding the diameter of a region we care about]] -- Dr. Luisa Rebull, 2018, for the Ceph-C team | ||
| − | measuring angular size of objects, e.g., cartwheel galaxy, in several different wavelengths. | + | <font color="red">to do:</font> |
| + | *<font color="red">measuring angular size of objects, e.g., cartwheel galaxy, in several different wavelengths. is it the same in different wavelengths?</font> | ||
| + | *<font color="red">distances between clumps in ic417 and relationship to ages of stars</font> | ||
=Other sources of interest= | =Other sources of interest= | ||
Latest revision as of 20:47, 13 August 2020
Contents
Most coherent, developed, tested materials
Finding the velocity of a high-proper-motion star in IC2118 -- Dr. Luisa Rebull, 2020
Other important CoolWiki pages
- FITS format
- Finding FITS files
- Viewing FITS files
- All ds9 information in one place
- Overview of measuring distances
Somewhat less coherent (or less standalone) materials
Finding the diameter of a region we care about -- Dr. Luisa Rebull, 2018, for the Ceph-C team
to do:
- measuring angular size of objects, e.g., cartwheel galaxy, in several different wavelengths. is it the same in different wavelengths?
- distances between clumps in ic417 and relationship to ages of stars
