Summary Page for Probing dark energy using the X-ray gas mass fraction in dynamically relaxed galaxy clusters
Probing dark energy using the X-ray gas mass fraction in dynamically relaxed galaxy clusters

Target: Abell 2204

Chandra
X-ray
Center

PI: Dr Steven Allen 
Seq Num: 800552
Obs ID: 6104
Instrument: ACIS




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Full Field with Sources
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Full Field with Sources
Full Field with Sources



List of the Brighest Sources in the Field
RA[deg] DEC[deg] NET_COUNTS[count] NET_COUNTS_ERR[count] SNR
248.097866 5.429620 141.875000 13.967070 10.157822
248.213868 5.581631 67.714287 11.108340 6.095806
248.255456 5.502183 35.238636 7.713988 4.568148
248.179224 5.654479 30.159090 7.154203 4.215576
248.251122 5.625733 29.318182 7.411719 3.955652
248.033452 5.570781 31.795454 8.437037 3.768557
248.195553 5.575929 102.571426 30.585615 3.353584
248.250792 5.535667 19.000000 5.949306 3.193650
248.372005 5.395283 33.875000 11.055345 3.064129
248.123551 5.431157 22.750000 7.463658 3.048103


Postscript Summary Page