Understanding redshift surveys

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In summary: VizieR?-source=VII/237A summary, The conversation discusses the use of the software Galaxy Explorer 2.0 for research on the Sloan Digital Sky Survey, specifically the center of the observed 3D distribution of galaxies. The conversation also mentions the incomplete nature of the data and suggests using VizieR for further study of the published data.
  • #1
batboy
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...With Galaxy Explorer 2.0


Hi!

I'm doing some personal reaserch on Sloan Digital Sky Survey, and I was wondering if anyone here uses this software?


If so, could you tell me what the center is?

For details of the SDSS project check the websites:
GalaxyExplorer: a 3D visualization tool: http://cas.sdss.org/dr4/en/help/download/
http://www.sdss.org/
http://skyserver.sdss.org/




thank you
 
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  • #2
I use the radial search and photometric catalogues a bit. What do you need to know specifically?
 
  • #3
Sorry, should've uploaded that from the beginning. I zoomed out as far I could to give some perspective. Specifically, I just wanted get some perspective about the middle. http://img446.imageshack.us/img446/9670/capture48200631255pm2vf.png Here is what the read-me says.

This program shows you the 3D distribution of galaxies observed by the Sloan
Digital Sky Survey. The data consists of the 3D positions of 131,000 galaxies
observed to date. Note, how galaxies tend to be close to one another, forming
walls and filaments.

The data is located on several 'wings', these only reflect the sky coverage,
i.e. the observations are still rather incomplete. When finished, in 2005,
there will have a full three-dimensional map of a large cone in the Northern
Sky. There will always be a gap around the plane of the Milky Way -- there is
too much dust there to see through, therefore that region was avoided.
 
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  • #4
batboy said:
If so, could you tell me what the center is?

The center is us (the Milky Way). The pie slices are the parts of the universe that we can see with SDSS. A galaxy's radial distance from us is estimated from its redshift.
 
  • #5
Thank you, SpaceTiger and matt.o.
 
  • #6
I recommend VizieR if you wish to study the published data from SDSS, or other redshift surveys: http://cdsweb.u-strasbg.fr/cats/Cats.htx. I use HTML format and copy it to an MS spreadsheet:
 

1. What is a redshift survey?

A redshift survey is a type of astronomical survey that measures the redshift of galaxies. Redshift is the phenomenon where the light emitted from an object appears to be shifted towards longer wavelengths, indicating that the object is moving away from us. By measuring the redshift of a large number of galaxies, scientists can map out the distribution of matter in the universe.

2. How do redshift surveys work?

Redshift surveys work by using a spectrograph to measure the redshift of light emitted by galaxies. The spectrograph uses a diffraction grating to break down the light into its component wavelengths, allowing scientists to determine the amount of redshift. The data from the spectrograph is then used to create a map of the distribution of galaxies in the universe.

3. What can we learn from redshift surveys?

Redshift surveys provide valuable information about the large-scale structure of the universe. By measuring the redshift of galaxies, scientists can determine the distance to these galaxies and their relative positions in the universe. This allows us to study the formation and evolution of galaxies, as well as the overall structure and expansion of the universe.

4. What are the limitations of redshift surveys?

One limitation of redshift surveys is that they only provide a 2-dimensional map of the universe, as they are limited by the field of view of the spectrograph. This makes it difficult to accurately map out the distribution of matter in the universe in 3 dimensions. Additionally, redshift surveys are biased towards brighter and more massive galaxies, which may not accurately represent the overall distribution of matter in the universe.

5. How are redshift surveys used in cosmology?

Redshift surveys are an important tool in cosmology, as they allow us to study the large-scale structure of the universe and the expansion of space. By measuring the redshift of galaxies, scientists can also determine the cosmological parameters of the universe, such as its age and rate of expansion. Redshift surveys are also used to test theories of gravity and dark matter, and to study the effects of dark energy on the expansion of the universe.

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