... signal in stellar mass bins split by morphology Signal on small scales reflects halo mass Signal on large scales reflects fraction in group/cluster Plot from Mandelbaum et al. 2005, astro-ph/0511164 Early types Late types 100 1000 r [kpc/h] Results, cont ...
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Ссылки http://www.stsci.edu/institute/itsd/information/streaming/archive/HubbleFellowsSymposium2008/RachelMandelbaum031108Hi_supporting/RachelMandelbaum031108.pdf -- 1949.4 Кб -- 12.03.2008 Похожие документы
... we note that R=26.9 is within 0.1 mag of the value for 3.9 April 2000 predicted by the fit to earlier R band data in Rhoads and Fruchter (astro-ph/0004057) and this provides some further confidence that our best estimate of the OT strength is not far off ...
... that the decay of the optical transient steepened to at least t ^ -1.75 to -2 at late times, in agreement with the result obtainted primarily from radio data by Berger et al (20001, astro-ph/0102278). 27.4 on the magnitude of the OT 47 days after outburst ...
... Given that a much redder color of B - V = +0.91 ± 0.15 was reported for S/2005 P 2 (Buie et al. 2006, http://xxx.lanl.gov/abs/astro-ph/?0512491), additional observations are solicited. ...
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Ссылки http://www.stsci.edu/~mutchler/documents/IAU_Circular_8686.pdf -- 93.6 Кб -- 10.03.2006 Похожие документы
... The full paper is available from the Astro-Ph archive, maintained at the Los Alamos National Laboratory. Click here for our entry in the archive. ...