Difference between revisions of "Measuring distances on images"
From CoolWiki
Jump to navigationJump to searchm |
m |
||
| (5 intermediate revisions by the same user not shown) | |||
| Line 1: | Line 1: | ||
| − | + | =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= | =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 | [[Finding the diameter of a region we care about]] -- Dr. Luisa Rebull, 2018, for the Ceph-C team | ||
| + | |||
| + | <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
