CL 0016+16 and the Hubble constant M. Birkinshaw 1 Department of Physics 2 , University of Bristol, Tyndall Avenue, Bristol BS8 1TL, U.K. J.P. Hughes 3 Department of Physics & Astronomy, Rutgers University, PO Box 849, Piscataway, NJ 08855­0849, U.S.A. Rich cluster CL 0016+16 lies in a large­scale dynamical structure at redshift 0:55, and has a strong Sunyaev­Zel'dovich effect. ... Finally, a strong Sunyaev­Zel'dovich effect is associated with the cluster. ... ApJ, submitted. ... ApJ, 251, L69. ...

... Nikolaev 2.8 USNO 104 Italy, San 0.40 21 x 21' 2.5 10 32 0.253 0.436 Marccello 2.0 GSC 106 Slovenia, 0.36 36 x 36' 2.0 2235 9264 0.307 0.295 Crni vrh 2.4 USNO 113 Germany , 0.50 13 x 10' 2 42 283 0.260 0.319 Schonbrunn 2.3 USNO 114 213 1172 0.260 0.222 118 Slovakia, 0.57 14 x 10' 1.7 7 42 0.165 0.077 Modra 3.3 USNO 130 Italy, 0.4 15 x 10' 1.0 9 36 0.284 0.275 Lumezzane 1.8 ... 1.8 UCAC A24 New Millennium 0.36 12 x 12' 1.4 86 399 0.341 0.284 Obs., ... 3.5 UCAC H15 ISON-NM Obs., ...

... T ayl or seri es gives: B= 2kT c 2 A A A = 2kT 2 2 2kT A e · Sourc e flux i n Rayl eigh J eans lim it: 2k S= 2 sT(, )d 2kT 2 Tem perat ure: TA = (Ae/ 2) Tsrc(, )Pn(, )d = (r/ A) Tsrc(, )Pn(, )d · If brightness tem perat ure i s c onst ant across sourc e: S= S 16 B= Brightnes s, = frequenc y ; h = 6.626 x 10- J s; k = 1.380 x 10-23 J K-1 ;T = temperature A = area; = Solid angle ... 1 GAIN Blank S ky or other Theoretic al, or Observati onal From di odes, Hot/ Col d loads, etc. ...

... Table 1. ... The list of objects is given in Table 2. ... 12 10.45 86.67 0.29 JS JU JN JE JT S SU SN SE ST U UN UE UT N NE Post E SP I L N 247.24 5.24 144.25 1.88 1.35 5.48 323.20 61.89 0.01 36.99 0.08 0.01 0.03 0.10 0.14 3.88 1063.87 0.04 0.07 0.15 49.43 0.01 2.22 156.10 0.28 0.02 96.93 45.80 0.01 0.01 0.14 430.55 102.28 0.01 187.82 1.08 0.01 106.75 1.94 107.07 0.38 0.03 0.03 0.02 0.03 0.10 0.50 193.99 1.84 16.19 0.06 55.36 521.23 0.15 24.33 251.13 0.08 4.89 1711.44 ...

... Printed in the U.S.A. PROBING THE BALANCE OF AGN AND STAR-FORMING ACTIVITY IN THE LOCAL UNIVERSE WITH ChaMP Anca Constantin1 , Paul Green1 , Tom Aldcroft1 , Dong-Woo Kim1 , Daryl Haggard2 , Wayne Barkhouse3 ,and Scott F. Anderson2 3 Harvard ... published 2009 October 20 1 ABSTRACT The combination of the Sloan Digital Sky Survey (SDSS) and the Chandra Multiwavelength Project ( ChaMP ) currently offers the largest and most homogeneously selected sample of nearby ... 2004; Ho 2008). ... 2004). ...

... 5-GHz total flux density . ... EW position (mas) . ... 0.2 .. ... Other VLBI references . 2.3 and/or 8.4 GHz: multiple epoch VLBI images are available in the USNO Radio Reference Frame Image Database (RRFID, Fey & Charlot 2000, ApJS 128, 17) . 15 GHz: multiple epoch VLBI images are available in the USNO Radio Reference Frame Image Database (RRFID, Fey & Charlot 2000, ApJS 128, 17) . 15 GHz: multiple epoch VLBI images are available in the VLBA 2-cm survey (Kellermann et al. ...

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