SHUFFLE: A New Statistical Bootstrap Method: Applied to Cosmological Filaments

Details SHUFFLE: A New Statistical Bootstrap Method: Applied to Cosmological Filaments SHUFFLE: A New Statistical Bootstrap Method: Applied to Cosmological Filaments

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..666..303b&link_type=abstract

THE EMERGENCE OF COSMIC STRUCTURE: Thirteenth Astrophysics Conference. AIP Conference Proceedings, Volume 666, pp. 303-306 (200

Astronomy and Astrophysics

Astrophysics

1

Origin And Formation Of The Universe

Scientific paper

We introduce Shuffle, a powerful statistical procedure devised by Bhavsar and Ling [1] to determine the true physical extent of the filaments in the Las Campanas Redshift Survey [LCRS]. At its heart, Shuffle falls in the category of bootstrap like methods [2]. We find that the longest physical filamentary structures in 5 of the 6 LCRS slices are longer than 50 h-1 Mpc but not quite extending to 70 h-1 Mpc. The -3 degree slice contains filamentary structure longer than 70 h-1 Mpc.

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