BCS+X-ray+Analysis+Comparison

= = =Links= Telecons [|Paul's WWW] Scaling Comparisons
 * = **Cluster** ||= Temp Comp ||= kT profile notes ||= EM comp ||= EM profile Notes ||= Wiki Link ||= Paul Homepage Link ||
 * = A115 ||= Yes ||= Good agreement ||= Yes ||= Messy EM profile, disagreement at larger radii ||= A115 ||= A115 ||
 * = A1423 ||= Yes ||= Good agreement ||= Yes ||= Davids higher than ours at large radii ||= A1423 ||= A1423 ||
 * = A1576 ||= Yes ||= Good agreement, low S/N profile ||= Yes ||= Davids profile consistently above ours ||= A1576 ||= A1576 ||
 * = A1682 ||= Yes ||= Good agreement ||= Yes ||= Hump in Davids profile differs from ours, could be due to exclusion of extended emission? ||= A1682 ||= A1682 ||
 * = A1758 ||= Yes ||= A hard cluster to analyse, compare notes ||= No ||=  ||=   ||= [|A1758] ||
 * = A1763 ||= Yes ||= Good agreement ||= Yes ||= Very good agreement ||= A1763 ||= A1763 ||
 * = A1835 ||= Yes ||= Very good agreement ||= Yes ||= Davids lower than ours within ~1Mpc ||= A1835 ||= A1835 ||
 * = A1914 ||= Yes ||= Good agrement ||= No ||= Very good agreement ||= A1914 ||= A1914 ||
 * = A2111 ||= Yes ||= Good agreement, large errors on secont to last bin on Paul profile ||= Yes ||= Davids consistently above ours, has shallower slope a large radii. ||= A2111 ||= A2111 ||
 * = A2204 ||= Yes ||= Very good agreement ||= Yes ||= Very good agreement ||= A2204 ||= A2204 ||
 * = A2219 ||= Yes ||= Pauls profile has large temperatures at small radii? ||= Yes ||= Davids profile has shallower slope at large radii leading to disagreement ||= A2219 ||= A2219 ||
 * = A2261 ||= Yes ||= Very good agreement ||= Yes ||= Good agreement, difference at large radii within errors ||= A2261 ||= A2261 ||
 * = A2390 ||= Yes ||= Have agreed to use only last 20ks, finally a good agreement ||= Yes ||= Davids below ours at small radii ||= A2390 ||= A2390 ||
 * = A2552 ||= Yes ||= Good agreement ||= Yes ||= Davids profile has shallower slope at large radii, consistent within errors ||= A2552 ||= A2552 ||
 * = A2631 ||= Yes ||= Good agreement ||= Yes ||= Good agreement ||= A2631 ||= A2631 ||
 * = A267 ||= Yes ||= Very good agreement ||= Yes ||= Davids below ours at small radii ||= A267 ||= A267 ||
 * = A520 ||= Yes ||= Good agreement ||= No ||=  ||= A520 ||= [|A520] ||
 * = A586 ||= Yes ||= Good agreement ||= Yes ||= Agreement consistent within error bars ||= A586 ||= A586 ||
 * = A611 ||= Yes ||= Flared observation, only extracting profiles out to ~150 arcsec ||= No ||=  ||= A611 ||= A611 ||
 * = A665 ||= Yes ||= Good agreement ||= yes ||= Davids consistently below ours at all radii ||= A665 ||= A665 ||
 * = A68 ||= Yes ||= Good agreement ||= Yes ||= Good agreement, david has steeper profile at large radii but consistent within errors ||= A68 ||= A68 ||
 * = A697 ||= Yes ||= Good agreement ||= Yes ||= Good agreement ||= A697 ||= A697 ||
 * = A773 ||= Yes ||= Very good agreement ||= Yes ||= Good agreement ||= A773 ||= A773 ||
 * = A781 ||= Yes ||= Good agreement ||= No ||= Paul to use isothermal model for gas mass calculation ||= A781 ||= [|A781] ||
 * = A963 ||= Yes ||= Very good agreement ||= Yes ||= Good agreement ||= A963 ||= A963 ||
 * = MS1455 ||= Yes ||= Very good agreement ||= Yes ||= Davids consistently below ours at all radii ||= MS1455 ||= MS1455 ||
 * = RXJ0437 ||= Yes ||= Good agreement ||= Yes ||= Good agreement ||= RXJ0437 ||= RXJ0437 ||
 * = RXJ0439 ||= Yes ||= Good agreement ||= Yes ||= Good agreement ||= RXJ0439 ||= [|RXJ0439] ||
 * = RXJ1720 ||= Yes ||= Very good agreement ||= Yes ||= Very good agreement ||= RXJ1720 ||= RXJ1720 ||
 * = RXJ2129 ||= Yes ||= Very good agreement ||= Yes ||= Good agreement ||= RXJ2129 ||= RXJ2129 ||
 * = Zw2089 ||= Yes ||= Very good agreement ||= Yes ||= Good agreement ||= zw2089 ||= [|zw2089] ||
 * = Zw3146 ||= Yes ||= Good agreement ||= Yes ||= good agreement ||= zw3146 ||= Zw3146 ||
 * = Zw5247 ||= Yes ||= Good agreement ||= Yes ||= Very poor agreement ||= zw5247 ||= [|Zw5247] ||
 * = Zw7215 ||= Yes ||= Good agreement, low S/N ||= Yes ||= Very poor agreement ||= zw7215 ||= Zw7215 ||