173,155 research outputs found
Percival, C R, 5714980
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/410362Surname: PERCIVAL. Given Name(s) or Initials: C R. Military Service Number or Last Known Location: 5714980. Missing, Wounded and Prisoner of War Enquiry Card Index Number: SEA-2650.226078
Item: [2016.0049.42631] "Percival, C R, 5714980
Bigelow (C-Henry Waugh & Co Penang), Norman Percival, Singapore
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/371753Surname: BIGELOW (C-HENRY WAUGH & CO PENANG)
Given Name(s) or Initials: NORMAN PERCIVAL
Military Service Number or Last Known Location: SINGAPORE
Missing, Wounded and Prisoner of War Enquiry Card Index Number: 15004182673
Item: [2016.0049.04080] "Bigelow (C-Henry Waugh & Co Penang), Norman Percival, Singapore
Jennings, Mr Percival John, C-O Caltex Corp Shanghai China
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/395202Surname: JENNINGS. Given Name(s) or Initials: MR PERCIVAL JOHN. Military Service Number or Last Known Location: C-O CALTEX CORP SHANGHAI CHINA. Missing, Wounded and Prisoner of War Enquiry Card Index Number: 55839.229021
Item: [2016.0049.27495] "Jennings, Mr Percival John, C-O Caltex Corp Shanghai China
Come hither thou beautiful rover, thou wand'rer of earth and of air [first line]
No full textstrophicpiano and voiceJohns Hopkins University, Levy Sheet Music Collection, Box
174, Item 048The Words by Percival. The Music by P.K. Moran
In the forest [music] : flute solo with piano accompaniment /
No full textCover title.; Also available online http://nla.gov.au/nla.mus-vn1617835; MUS: N, --
Come hither thou beautiful rover, thou wand'rer of earth and of air [first line]
No full textstrophicpiano and voiceJohns Hopkins University, Levy Sheet Music Collection, Box
174, Item 048The Words by Percival. The Music by P.K. Moran
Oh, that I had wings [music] : anthem /
No full textPl. no.: B. 1093.; For SATB with organ.; Also available online http://nla.gov.au/nla.mus-vn2100067
Sweet content [music] : flute solo : op. 5 with pianoforte accompaniment /
No full textW.H.P. & Co.,1391 (Publisher number). Cover title.; "To my friend and master Mr. John Lemmoné."; Pl. no.: W.H.P. & Co. 1391.; Printed in England.; NLA's NL copy has inscribed to George Wane by the composer, dated 7-3-27. ANL; Also available online http://nla.gov.au/nla.mus-vn95380; NLA's NL copy from the collection of George Wane
The shepherds [music] /
No full textB.1257 (Publisher number). For voices (SATB) and piano.; Caption title.; Pl. no.: B.1257.; Also available online http://nla.gov.au/nla.mus-vn2432675
Interpreting large-scale redshift-space distortion measurements
No full textThe simplest theory describing large-scale redshift-space distortions (RSD), based on linear theory and distant galaxies, depends on the growth of cosmological structure, suggesting that strong tests of general relativity can be constructed from galaxy surveys. As data sets become larger and the expected constraints more precise, the extent to which the RSD follow the simple theory needs to be assessed in order that we do not introduce systematic errors into the tests by introducing inaccurate simplifying assumptions. We study the impact of the sample geometry, non-linear processes and biases induced by our lack of understanding of the radial galaxy distribution on RSD measurements. Using Large Suite of Dark Matter Simulations of the Sloan Digital Sky Survey II (SDSS-II) luminous red galaxy data, these effects are shown to be important at the level of 20per cent. Including them, we can accurately model the recovered clustering in these mock catalogues on scales 30-200h -1Mpc. Applying this analysis to robustly measure parameters describing the growth history of the Universe from the SDSS-II data gives f(z= 0.25)σ 8(z= 0.25) = 0.3512 ± 0.0583 and f(z= 0.37)σ 8(z= 0.37) = 0.4602 ± 0.0378 when no prior is imposed on the growth rate, and the background geometry is assumed to follow a Λ cold dark matter (ΛCDM) model with the Wilkinson Microwave Anisotropy Probe (WMAP)+Type Ia supernova priors. The standard WMAP constrained ΛCDM model with general relativity predicts f(z= 0.25)σ 8(z= 0.25) = 0.4260 ± 0.0141 and f(z= 0.37)σ 8(z= 0.37) = 0.4367 ± 0.0136, which is fully consistent with these measurements. © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
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