2dF Galaxy Redshift Survey
1206720
184288617
2008-01-14T17:34:37Z
122.126.37.169
[[Image:2dfgrs.png|right|thumb|300px|Rendering of the 2dFGRS data]]
In [[astronomy]], the '''2dF Galaxy Redshift Survey''' (Two-degree-Field Galaxy Redshift Survey), '''2dF''' or '''2dFGRS''' is a [[redshift survey]] conducted by the [[Anglo-Australian Observatory]] (AAO) with the 3.9[[metre|m]] [[Anglo-Australian Telescope]] between [[1997]] and [[11 April]] [[2002]].<ref>[http://www2.aao.gov.au/~TDFgg/Public/Survey/Overview/sld013.htm Final Status of Survey Observations]</ref> The data from this survey were made public on [[30 June]] [[2003]]. The survey determined the large-scale structure in one section of the local Universe. As of January 2007, it is the second largest redshift survey next to the [[Sloan Digital Sky Survey]] which began in 2000. Steve Maddox and John Peacock were in charge of the project.
== Description ==
The 2dF survey covered an area of about 1500 [[square degree]]s, surveying regions in both the north and the south [[galactic pole]]s.<ref name="AAO's 2dF Intro">[http://www2.aao.gov.au/~TDFgg/Public/Survey/description.html 2dFGRS − An Introduction]</ref> The name derives from the fact that the survey instrument covers an area of approximately two square degrees.
The areas selected for observation were previously surveyed by the massive [[APM Galaxy Survey]] (on which Steve Maddox also worked).<ref name="AAO's 2dF Intro" /> The regions surveyed cover roughly 75 degrees of [[right ascension]] for both bands, and the [[declination]] of the North Polar band was about 7.5 degrees while the declination of the South Polar band was about 15 degrees. Hundreds of isolated two degree fields near the South Polar band were also surveyed (see [http://www2.aao.gov.au/~TDFgg/Public/Survey/Overview/img009.GIF this illustration], where black circles represent survey fields, and the red grid represents the earlier APM survey).
In total, the [[photometry (astronomy)|photometry]] of 382,323 objects were measured, which includes [[spectrum|spectra]] for 245,591 objects, of which 232,155 were [[galaxies]] (221,414 with good quality spectra), 12,311 are [[stars]], and 125 are [[quasi-stellar object]]s (quasars).<ref>[http://www2.aao.gov.au/~TDFgg/Public/Survey/statusfinal.html 2dFGRS Summary Statistics]</ref> The survey necessitated 272 required nights of observation, spread over 5 years.
The survey was carried out with the 4 metre [[Anglo-Australian Telescope]], with the 2dF instrument installed at the primary focus permitting the observation of a field of 2 degrees per pointing. The instrument possesses a [[spectrograph]] equipped with two banks each of 200 optical fibres, permitting the simultaneous measurement of 400 spectra. The limiting apparent magnitude of the survey is 19.5, covering objects with a [[redshift]] mostly within less than z=0.3 and a median [[redshift]] of 0.11. The volume of the Universe covered by the survey is approximately 10<sup>8</sup> ''h''<sup>-1</sup> [[Megaparsec|Mpc]]<sup>3</sup>, where ''h'' corresponds to the value of the [[Hubble constant]], ''H''<sub>0</sub>, divided by 100. ''H''<sub>0</sub> is approximately 70 km/s/Mpc. The largest [[redshift]] observed by the survey corresponds to a distance of 600 ''h''<sup>-1</sup> Mpc.
== Survey Results ==
The principal results obtained for the field of [[cosmology]] by the 2dF survey are:
* The measurement of the [[density parameter]] of [[non-relativistic matter]] ([[baryonic matter]] plus [[dark matter]] plus massive [[neutrinos]])
* The detection of acoustic oscillations of baryons, and as a consequence the relationship between the density of baryonic matter and dark matter
* Limits on the contribution of massive neutrinos to dark matter, putting a limit on the sum of the masses of the three families of neutrinos at 1.8 eV.
All these results are in agreement with the measurements of other experiments, notably those of [[WMAP]]. They confirm the [[Lambda-CDM model|standard cosmological model]].
[[Image:2dfdtfe.gif|thumb|300px|right|[[Dtfe|DTFE]] reconstruction of the inner parts of the 2dF Galaxy Redshift Survey.]]
The 2dF survey also yields a unique view on our local cosmic environment. In the figure a 3-D reconstruction of the inner parts of the survey is shown, revealing an impressive view on the cosmic structures in the nearby universe. Several [[superclusters]] stand out, such as the [[Sloan Great Wall]], the largest structure in the universe known to date.
== See also ==
* [[Lambda-CDM model]]
* [[Acoustic oscillations of Baryons]]
* [[Dark matter]]
== Notes ==
<references />
== External links ==
* [http://www2.aao.gov.au/2dFGRS/ Official site] of the 2dF Galaxy Redshift Survey
* [http://www2.aao.gov.au/2dFGRS/Public/Publications/colless_specz.pdf ''The 2dF Galaxy Redshift Survey: spectra and redshifts''] − 2001 [[Royal Astronomical Society]] paper describing the survey
* [http://www.aao.gov.au/2df/ Official site] of the Two Degree Field instrument system
[[Category:Astronomical surveys]]
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