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J131145.1+220206.0

Link to XCS-DR1 entry

Fig. 1: The SDSS optical image with the XCS X-ray contours overlaid. Fig. 2: The colour-magnitude diagram used to determine the magnitude gap. Green triangles are spectroscopic cluster members and circles are photometric cluster members. Red triangles are spectroscopic non-members. Only cluster members within ±0.2 mag of the r-i colour of the fossil galaxy (dotted lines) are used to calculate the gap. The two diamonds denote the second and the fourth brightest galaxy.

Notes

This z=0.1715 system is located at 13:11:45.1 +22:02:06.0. The CMD shows an obvious RS, which all spectroscopic members lie on, and the magnitude gap is 2.7 based on SDSS photometric data. The rejected galaxy is ~50000$ km s-1 away from the FG. The X-ray temperature of the system is TX=3.4 keV and the X-ray emission peak lies ~95.3 kpc from the FG. The X-ray source is extended with R200=1.16 Mpc or ~25R90. The system has a velocity dispersion of 362 km s-1 based on 10 galaxies. This system is also known as MaxBCG J197.94248+22.02702.

Fossil System

XCS IDΔm14R200LXTXLtotΣL24
XMMXCS J131145.1+220206.02.71.161.573.410.971.39

Fossil Galaxy

SDSS IDzMAgeZlog(SSFR)Lgal
J131146.19+220137.20.17150.979.50.027-12.134.36
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