17 - Redshift Surveys

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14 Terms

1
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We an measure the recession velocity using ________.

Redshifts

2
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Galaxy light is composed of the cumulative light from all its ____, _______ ___, and _____ black holes.

Stars, shining gas, active

3
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Shining gas emits ______ _____.

Emission lines

4
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What do emission lines correspond to?

Specific atomic transition of hot gas

5
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What do absorption lines correspond to?

Specific atomic transition of cool outer parts of stars

6
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What can emission and absorption lines be used for?

Markers to measure redshift

7
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How to do a redshift survey?

Map a region of the sky, take a spectrum for each galaxy, identify known features, then make a 3-D catalog

8
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Why is distance from hubble’s law approximate?

Peculiar velocities can vary significantly, and we have no way to correct for them.

9
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What effect does peculiar velocities lead to?

Fingers of God

10
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How are Fingers of God formed?

Dense regions have more gravity, making galaxies orbit faster, and have a higher peculiar velocity, broadening dense groups of galaxies in redshifts

11
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When were the first redshift surveys?

1980s

12
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What would happen if the universe had more matter?

More matter so more gravity so faster growth so more structure

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What happens if dark energy was 0?

Structure can still grow early on before dark energy dominated

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How would you measure the growth rate of large-scale structure since the CMB?

Measure galaxy clustering, measure strength of Fingers of God, and measure weak lensing