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WiggleZ Dark Energy Survey Baryon Acoustic Oscillation Random Catalogues

Blake, Chris; Kazin, Eyal; Buetler, Florian; Davis, Tamara M.; Parkinson, David; Brough, Sarah; Colless, Matthew; Couch, Warrick; Croom, Scott; Croton, Darren; Drinkwater, Michael J.; Forster, Karl; Gilbank, David; Gladders, Michael; Glazebrook, Karl; Jelliffe, Ben; Jurek, Russell J.; Li, I-hui; Madore, Barry; Martin, D. Christopher; Pimbblet, Kevin J.; Poole, Gregory B.; Pracy, Michael; Sharp, Rob; Wisnioski, Emily; Woods, David ; Wyder, Ted K.; Yee, H. K. C


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  <dc:creator>Blake, Chris</dc:creator>
  <dc:creator>Kazin, Eyal</dc:creator>
  <dc:creator>Buetler, Florian</dc:creator>
  <dc:creator>Davis, Tamara M.</dc:creator>
  <dc:creator>Parkinson, David</dc:creator>
  <dc:creator>Brough, Sarah</dc:creator>
  <dc:creator>Colless, Matthew</dc:creator>
  <dc:creator>Couch, Warrick</dc:creator>
  <dc:creator>Croom, Scott</dc:creator>
  <dc:creator>Croton, Darren</dc:creator>
  <dc:creator>Drinkwater, Michael J.</dc:creator>
  <dc:creator>Forster, Karl</dc:creator>
  <dc:creator>Gilbank, David</dc:creator>
  <dc:creator>Gladders, Michael</dc:creator>
  <dc:creator>Glazebrook, Karl</dc:creator>
  <dc:creator>Jelliffe, Ben</dc:creator>
  <dc:creator>Jurek, Russell J.</dc:creator>
  <dc:creator>Li, I-hui</dc:creator>
  <dc:creator>Madore, Barry</dc:creator>
  <dc:creator>Martin, D. Christopher</dc:creator>
  <dc:creator>Pimbblet, Kevin J.</dc:creator>
  <dc:creator>Poole, Gregory B.</dc:creator>
  <dc:creator>Pracy, Michael</dc:creator>
  <dc:creator>Sharp, Rob</dc:creator>
  <dc:creator>Wisnioski, Emily</dc:creator>
  <dc:creator>Woods, David </dc:creator>
  <dc:creator>Wyder, Ted K.</dc:creator>
  <dc:creator>Yee, H. K. C</dc:creator>
  <dc:date>2012-09-07</dc:date>
  <dc:description>Data products associated with the WiggleZ Dark Energy survey measurement of the Baryon Acoustic Oscillations (BAO), as described in Blake et al. arXiv:1108.2635 (2011, MNRAS, 418, 1707)

Data is given for 6 WiggleZ regions (01, 03, 09, 11, 15, 22 hrs) in 3 different overlapping redshift slices (z=0.2-0.6, 0.4-0.8, 0.6-1.0), matching the datasets analyzed in the final WiggleZ baryon acoustic peak paper Blake et al. (2011, MNRAS, 418, 1707). For each sub-region the following files are given:

Correlation function: xi_**hr*.dat - correlation function measurement and covariance matrix for each sub-region. Format of the file:


	1st line: nbin, ngalaxy
	nbin lines: mean separation [Mpc/h], xi(s), sqrt[Cov(i,i)]
	nbin x nbin lines: i, j, Cov(i,j)


The covariance matrix is from lognormal realizations, not jack-knife regions.

Combined correlation function: xi_combined*.dat - correlation function measurement for each redshift range combining the measurements in each sub-region, in the same format as above.

Integral constant: wigglez_ic.dat - integral constraint correction which should be added to the measured correlation function, format of the file is:


	Region [hr],
	zmin,
	zmax,
	integral constraint delta-xi


We are considering adding another 90 random catalogues in the near future. For now the random catalogues used in the previous analysis are available below.</dc:description>
  <dc:identifier>https://zenodo.org/record/33470</dc:identifier>
  <dc:identifier>10.5281/zenodo.33470</dc:identifier>
  <dc:identifier>oai:zenodo.org:33470</dc:identifier>
  <dc:relation>doi:10.5281/zenodo.618907</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://creativecommons.org/publicdomain/zero/1.0/legalcode</dc:rights>
  <dc:source>Monthly Notices of the Royal Astronomical Society 418 1707 (2012)</dc:source>
  <dc:subject>cosmology</dc:subject>
  <dc:subject>wigglez</dc:subject>
  <dc:subject>baryon acoustic oscillation</dc:subject>
  <dc:subject>galaxy redshift survey</dc:subject>
  <dc:title>WiggleZ Dark Energy Survey Baryon Acoustic Oscillation Random Catalogues</dc:title>
  <dc:type>info:eu-repo/semantics/other</dc:type>
  <dc:type>dataset</dc:type>
</oai_dc:dc>
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