Topology of luminous red galaxy in the sdss
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Topology of Luminous Red Galaxy in the SDSS. Yun-Young Choi, Changbom Park, & Juhan Kim KIAS. Introduction to SDSS LRGs. Eisenstein et al. 2001. SDSS uses color to target luminous, early-type galaxies at 0.2< z <0.5. Fainter than MAIN ( r <19.5) About 15/sq deg

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Topology of Luminous Red Galaxy in the SDSS

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Topology of luminous red galaxy in the sdss

Topology of Luminous Red Galaxy in the SDSS

Yun-Young Choi, Changbom Park, & Juhan Kim

KIAS

SDSS-KSG Meeting


Topology of luminous red galaxy in the sdss

Introduction to SDSS LRGs

Eisenstein et al. 2001

  • SDSS uses color to target luminous, early-type galaxies at 0.2<z<0.5.

    • Fainter than MAIN (r<19.5)

    • About 15/sq deg

    • Excellent redshift success rate

  • Science Goals:

    • Clustering on largest scales

    • Galaxy clusters to z~0.5

    • Evolution of massive galaxies


Topology of luminous red galaxy in the sdss

Max Tegmark


Acoustic oscillation

Acoustic Oscillation

SDSS-LRG

http://sdss.org


Large scale correlation

Acoustic series in P(k) becomes a single peak in x(r)!

Pure CDM model has no peak.

Large Scale Correlation

Galaxy bias

Non-linear structure evolution

Redshift distortion


Topology of luminous red galaxy in the sdss

30°

45°

60°

12h

8h

11h

9h

10h

Dr4+ LRG sample: ~80k galaxies


Topology of luminous red galaxy in the sdss

Blanton et al.


Topology of lrg

Topology of LRG

Genus – Measure of Topology

(Gott, Dickinson, and Melott 1986)

A measure of the degree of connectivity of the smoothed galaxy # density field

High 50%

High 8%


Topology of luminous red galaxy in the sdss

MAIN

LRG

Biasedgalaxy formation at lowdensity environments – more connected


Topology of luminous red galaxy in the sdss

Environmental Dependency of LF

LRG

MAIN

MAIN


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