Difference between revisions of "Instrumentation"
From PGSC Wiki
Line 1: | Line 1: | ||
− | Questions in this category have been asked by | + | Questions in this category have been asked by PJ,MT |
*What do you know about WMAP? | *What do you know about WMAP? | ||
Line 8: | Line 8: | ||
* why do we build large telescopes on the ground, if HST has a much better | * why do we build large telescopes on the ground, if HST has a much better | ||
resolution with just 2.3m? | resolution with just 2.3m? | ||
+ | |||
+ | *If we observed a neutron star in LMC from a X-ray telescope, are we able to use a optical telescope to find out if it has a optical companion? | ||
+ | ** How many stars in LMC? | ||
+ | ** What's the angular resolution for a X-ray telescope (some early X-ray telescope before Chandra)? | ||
+ | ** What's the angular resolution for a typical optical telescope? | ||
+ | ** In the field we observed the neutron star, how many stars we would observed in optical? |
Revision as of 22:56, 11 December 2007
Questions in this category have been asked by PJ,MT
- What do you know about WMAP?
- What spacecraft have gone up recently?
- What's the latest, coolest instrumentation?
- what do you know about HST?
- why do we build large telescopes on the ground, if HST has a much better
resolution with just 2.3m?
- If we observed a neutron star in LMC from a X-ray telescope, are we able to use a optical telescope to find out if it has a optical companion?
- How many stars in LMC?
- What's the angular resolution for a X-ray telescope (some early X-ray telescope before Chandra)?
- What's the angular resolution for a typical optical telescope?
- In the field we observed the neutron star, how many stars we would observed in optical?