2dF Galaxy Redshift Survey

2dF Galaxy Redshift Survey

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 3.9m Anglo-Australian Telescope between 1997 and 11 April 2002. [ [http://www2.aao.gov.au/~TDFgg/Public/Survey/Overview/sld013.htm Final Status of Survey Observations] ] 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 degrees, surveying regions in both the north and the south galactic poles. [http://www2.aao.gov.au/~TDFgg/Public/Survey/description.html 2dFGRS − An Introduction] ] 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). 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.gifthis illustration] , where black circles represent survey fields, and the red grid represents the earlier APM survey).

In total, the photometry of 382,323 objects were measured, which includes 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 objects (quasars). [ [http://www2.aao.gov.au/~TDFgg/Public/Survey/statusfinal.html 2dFGRS Summary Statistics] ] 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 108 "h"-1 Mpc3, where "h" corresponds to the value of the Hubble constant, "H"0, divided by 100. "H"0 is approximately 70 km/s/Mpc. The largest redshift observed by the survey corresponds to a distance of 600 "h"-1 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 standard cosmological model.



thumb|300px|right|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

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


Wikimedia Foundation. 2010.

Игры ⚽ Поможем написать курсовую

Look at other dictionaries:

  • 2dF Galaxy Redshift Survey — Interpretación de la información obtenida con el 2dFGRS. En astronomía, el 2dF Galaxy Redshift Survey (Sondeo de corrimiento al rojo de galaxias en un campo de 2 grados), 2dF o 2dFGRS es un sondeo de corrimiento al rojo de galaxias llevado a cabo …   Wikipedia Español

  • 2dF Galaxy Redshift Survey — Extension du relevé du 2dF 2dFGRS, ou 2dF Galaxy Redshift Survey, pour l’anglais Two degree field (« champ de deux degrés ») est un catalogue de galaxies réalisé par l’observatoire anglo australien (AAO). Il a été réalisé sur une… …   Wikipédia en Français

  • Redshift survey — In astronomy, a redshift survey, or galaxy survey, is a survey of a section of the sky to measure the redshift of astronomical objects. Using Hubble s law, the redshift can be used to calculate the distance of an object from Earth. By combining… …   Wikipedia

  • 2dF — Galaxy Redshift Survey Extension du relevé du 2dF 2dFGRS, ou 2dF Galaxy Redshift Survey, pour l’anglais Two degree field (« champ de deux degrés ») est un catalogue de galaxies réalisé par l’observatoire anglo australien (AAO). Il a été …   Wikipédia en Français

  • Redshift — This article is about the astronomical phenomenon. For other uses, see Redshift (disambiguation). Physical cosmology …   Wikipedia

  • Galaxy formation and evolution — The study of galaxy formation and evolution is concerned with the processes that formed a heterogeneous universe from a homogeneous beginning, the formation of the first galaxies, the way galaxies change over time, and the processes that have… …   Wikipedia

  • Redshift quantization — is the hypothesis that the redshifts of cosmologically distant objects (in particular galaxies) tend to cluster around multiples of some particular value. Since there is a correlation of distance and redshift as expressed in Hubble s Law,… …   Wikipedia

  • 2dFGRS — 2dF Galaxy Redshift Survey Extension du relevé du 2dF 2dFGRS, ou 2dF Galaxy Redshift Survey, pour l’anglais Two degree field (« champ de deux degrés ») est un catalogue de galaxies réalisé par l’observatoire anglo australien (AAO). Il a …   Wikipédia en Français

  • Observable universe — For a general discussion of the universe, see Universe. Visualization of the 93 billion light year – or 28 billion parsec – three dimensional observable universe. The scale is such that the fine grains of light represent collections of large… …   Wikipedia

  • Observational cosmology — Physical cosmology Universe · Big Bang …   Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”