The 6dF Galaxy Survey: Samples, Observational Techniques and the First Data Release

Autor: D. H. Jones, W. Saunders, M. Colless, M. A. Read, Q. A. Parker, F. G. Watson, L. A. Campbell, D. Burkey, T. Mauch, L. Moore, M. Hartley, P. Cass, D. James, K. Russell, K. Fiegert, J. Dawe, J. Huchra, T. Jarrett, O. Lahav, J. Lucey, G. A. Mamon, D. Proust, E. M. Sadler, K.-i. Wakamatsu
Přispěvatelé: Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Departement d'Astrophysique Extragalactique et de Cosmologie (DAEC), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Jazyk: angličtina
Rok vydání: 2004
Předmět:
Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2004, 355 (3), pp.747. ⟨10.1111/j.1365-2966.2004.08353.x⟩
Monthly Notices of the Royal Astronomical Society, 2004, 355 (3), pp.747. ⟨10.1111/j.1365-2966.2004.08353.x⟩
ISSN: 0035-8711
1365-2966
DOI: 10.1111/j.1365-2966.2004.08353.x⟩
Popis: The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150,000 galaxies, and the peculiar velocities of a 15,000-member sub-sample, over almost the entire southern sky. When complete, it will be the largest redshift survey of the nearby universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K_tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J, r_F, b_J) = (13.05, 13.75, 15.6, 16.75). Central to the survey is the Six-Degree Field (6dF) multi-fibre spectrograph, an instrument able to record 150 simultaneous spectra over the 5.7-degree field of the UK Schmidt Telescope. An adaptive tiling algorithm has been employed to ensure around 95% fibering completeness over the 17046 sq.deg of the southern sky with | b | > 10 deg. Spectra are obtained in two observations using separate V and R gratings, that together give R ~ 1000 over at least 4000 -- 7500 Angstroms and signal-to-noise ratio ~10 per pixel. The 6dFGS database is available at http://www-wfau.roe.ac.uk/6dFGS/, with public data releases occuring after the completion of each third of the survey.
17 pages, 10 figures, submitted to MNRAS. Full resolution version of the paper available at http://www-wfau.roe.ac.uk/6dFGS/ and http://www.mso.anu.edu.au/6dFGS/
Databáze: OpenAIRE