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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; +21 Authors
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;
WiggleZ Dark Energy Survey Baryon Acoustic Oscillation Random Catalogues
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.
galaxy redshift survey, wigglez, cosmology, baryon acoustic oscillation
galaxy redshift survey, wigglez, cosmology, baryon acoustic oscillation
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).0 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Average influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Average impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Average views 783 downloads 472 citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).0 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Average influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Average impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Average - 783views472downloads
popularity
Popularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP!influenceInfluence provided by BIP!
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Influence provided by BIP!impulseImpulse provided by BIP!
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
Impulse provided by BIP!viewsViews provided by UsageCounts
Views provided by UsageCountsdownloadsDownloads provided by UsageCounts
Downloads provided by UsageCounts Average
Average
Average
783
472
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.