Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures

Abstract

The Universe at the present epoch is found to be a network of matter over-dense and under-dense regions. To date, this picture of the Universe is best revealed through cosmological large-volume simulations and large-scale galaxy redshift surveys, in which, the most important step is the appropriate identification of structures. So far, these structures are identified using various group finding codes, mostly based on the friends-of-friends (FoF) or spherical over-density (SO) algorithms. Although, the main purpose is to identify gravitationally bound structures, surprisingly, the mass information has hardly been used effectively by these codes. Moreover, the methods used so far either constrain the over-density or use the real unstructured geometry only. Even though these are key factors in the accurate determination of structures-mass information, hardly any attempt has been made as yet to consider these important parameters together while formulating the grouping algorithms. In this paper, we present our proposed algorithm which takes care of all the above-mentioned relevant features and ensures the bound structures by means of physical quantities, mainly mass and the total energy information. We introduced a novel concept of physically relevant arm-length for each element depending on their individual gravity leading to a distinct linking length for each unique pair of elements. This proposed algorithm is thus fundamentally new that, not only able to catch the gravitationally bound, real unstructured geometry, it does identify it roughly within a predefined physically motivated density threshold. Such a thing could not be simultaneously achieved before by any of the usual FoF or SO-based methods. We also demonstrate the unique ability of the code in the appropriate identification of structures, both from large volume cosmological simulations as well as from galaxy redshift surveys.

28 pages, 13 figures, published in the Physical Review D

References in corpus (15)

• The NumPy array: a structure for efficient numerical computation
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• The 2.5 m Telescope of the Sloan Digital Sky Survey
• K-corrections and filter transformations in the ultraviolet, optical, and near infrared
• Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
• The stellar masses of 25000 galaxies at 0.2<z<1.0 estimated by the COMBO-17 survey
• SubHaloes going Notts: The SubHalo-Finder Comparison Project
• Asymmetries in the inner regions of LCDM haloes
• On the definition of superclusters
• The Limits of Bound Structures in the Accelerating Universe
• Subhaloes gone Notts: Spin across subhaloes and finders
• Understanding `galaxy groups' as a unique structure in the universe
• Saraswati: An Extremely Massive ~ 200 Megaparsec Scale Supercluster