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The 6dF Galaxy Survey (Six-degree-Field Galaxy Survey), 6dF or 6dFGS is a redshift survey conducted by the Anglo-Australian Observatory (AAO) with the 1.2m UK Schmidt Telescope between 2001 and 2009. The data from this survey were made public on 31 March 2009.〔The 6dF Galaxy Survey DR3, Heath Jones et al., (2009)〕 The survey has mapped the nearby universe over nearly half the sky. Its 136 304 spectra have yielded 110 256 new extragalactic redshifts and a new catalog of 125 071 galaxies. For a subsample of 6dF a peculiar velocity survey is measuring mass distribution and bulk motions of the local Universe. As of July 2009, it is the third largest redshift survey next to the Sloan Digital Sky Survey (SDSS) and the 2dF Galaxy Redshift Survey (2dFGRS). ==Description== The 6dF survey covers 17 000 deg2 of the southern sky which is approximately ten times the area of the 2dFGRS〔2dFGRS; Colless et al. 2001〕 and more than twice the spectroscopic areal coverage of the Sloan Digital Sky Survey.〔SDSS DR7; Abazajian et al. 2009〕 All redshifts and spectra are available through the (6dFGS Online Database ), hosted at the Royal Observatory, Edinburgh. An (online 6dFGS atlas ) is available through the University of Cape Town. The survey was carried out with the 1.2 meter UK Schmidt Telescope at Siding Spring Observatory in New South Wales, Australia with the 6dF instrument permitting the observation of a field of 6 degrees per pointing. The instrument possesses a multi-object fiber spectrograph with 150 optical fibers per field plate. One feature of the 6dF Galaxy Survey compared to earlier redshift and peculiar velocity surveys is its near-infrared source selection. The main target catalogs are selected from the Two Micron All Sky Survey.〔2MASS; Jarrett et al. 2000〕 There are several advantages of choosing galaxies in these bands. * The near-infrared spectral energy distributions of galaxies are dominated by the light of their oldest stellar populations, and hence, the bulk of their stellar mass. Traditionally, surveys have selected target galaxies in the optical where galaxies dominated by younger, bluer stars. * The effects of dust extinction are smaller at longer wavelengths. For the target galaxies, this means that the total near-infrared luminosity is not dependent on galaxy orientation and so provides a reliable measure of galaxy mass. Furthermore this means the 6dFGS can map the local Universe nearer to the plane of the Milky Way than would otherwise be possible through optical selection. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「6dF Galaxy Survey」の詳細全文を読む スポンサード リンク
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