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A catalogue of the voids in the IRAS 1.2- Jy survey
Author(s) -
Hagai ElAd,
Tsvi Piran,
L. N. da Costa
Publication year - 1997
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/287.4.790
Subject(s) - physics , galaxy , void (composites) , astrophysics , smoothing , universe , sample (material) , astronomy , statistics , materials science , mathematics , composite material , thermodynamics
Using the Void-Finder algorithm we have compiled a catalogue of voids in the IRAS 1.2 Jy sample. The positions of the voids correspond well to the under dense regions seen in the IRAS smoothed density map. However, since in our analysis no smoothing is used, all structures appear much sharper: walls are not smeared and the voids are not artificially reduced by them. Therefore the current method based on the point distribution of galaxies is better suited to determine the diameter of voids in the galaxy distribution. We have identified 24 voids, covering more than 30% of the volume considered. By comparing the results with equivalent random catalogues we have determined that twelve voids are significant at a 0.95 confidence level, having an average diameter of 40 the nearby universe, but also to give support to the results recently obtained with the SSRS2 survey, suggesting a void-filled universe. Moreover, our results indicate that the voids detected have a similar scale, demonstrating that both optically and IRAS selected galaxies delineate the same large-scale structures

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