Dictionary of Nomenclature of Celestial Objects
(Last update: 10-Sep-2021)

Result of query: info cati VFK98]$

Details on Acronym:   H
   H (HST) ***** Avoid the usage of H, prefer [VFK98] Originof the Acronym: L (2007ApJ...661..750T)
Details on Acronym:   Keck
   Keck (Keck telescope) ***** Avoid the usage of Keck, prefer [VFK98] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   [VFK98]
   [VFK98] (Van Dokkum+Franx+Kelson+, 1998)= (H) = (Keck) Write:<<[VFK98] NNNN>> Object:G in ClG  (SIMBAD class: GinCl = Galaxy in Cluster of Galaxies) Note:HST WFPC2 and Keck observations.
Galaxies in the ClG 1E 1054.4-0321.
See also [VFF2000], [FFF98], [KVF97], [VFK2001]. in source:1E 1054.4-0321 = ClG 1054-0321 Ref:=1998ApJ...504L..17V byVAN DOKKUM P.G. , FRANX M., KELSON D.D., ILLINGWORTH G.D. Astrophys. J., 504, 17-22 (1998) Luminosity evolution of early-type galaxies to z = 0.83: constraints on formation epoch and Ω. oIn the text + fig.3 : MS 2053+03 misprint for MS 2053-03 = ClG 2053-04 oTable 1: <[VFK98] NNNN> N=8 among (Nos 1294-1583). Ref:=1999ApJ...520L..95V byVAN DOKKUM P.G. , FRANX M., FABRICANT D., KELSON D.D., ILLINGWORTH G.D. Astrophys. J., 520, 95-98 (1999) A high merger fraction in the rich cluster MS 1054-03 at z = 0.83: direct evidence for hierarchical formation of massive galaxies. oFig.1: <[VFK98] NNNN> N=22 added among (Nos 514-2011). Ref:=1999ApJ...522...39T byTRAN K.-V. , KELSON D.D., VAN DOKKUM P., FRANX M., ILLINGWORTH G.D., MAGEE D. Astrophys. J., 522, 39-45 (1999) The velocity dispersion of MS 1054-03: a massive galaxy cluster at high redshift. oMS 1054-03 = ClG 1054-03 = 1E 1054.4-0321. T.1: objects 1st created as [TKV99], but they are objects from the same catalogue of 1998ApJ...504L..17V. oTable 1: <[VFK98] NNNN> N=24 among (Nos 696-1986). Ref:=2000ApJ...541...95V byVAN DOKKUM P.G. , FRANX M., FABRICANT D., ILLINGWORTH G.D., KELSON D.D. Astrophys. J., 541, 95-111 (2000) Hubble space telescope photometry and Keck spectroscopy of the rich cluster MS 1054-03: morphologies, Butcher-Oemler effect, and the color-magnitude relation at z = 0.83. op. 100 : 1604+43 = ClG 1603+43 (=ClG J1604+4304) oTables 2, 3: <[VFK98] NNNN> N=85 among (Nos 514-2174), 77 are new. Tables 2, 3: <[VFF2000] HES N> (Nos 1-2). Ref:=2007ApJ...661..750T byTRAN K.-V.H. , FRANX M., ILLINGWORTH G.D., VAN DOKKUM P., KELSON D.D., BLAKESLEE J.P., POSTMAN M. Astrophys. J., 661, 750-767 (2007) A Keck spectroscopic survey of MS 1054-03 (z = 0.83): forming the red sequence. oTable 1, col(2): <[VFK98] NNNN> N=153 added among (Nos 159-8001). =E=Catalogue in electronic form as J/ApJ/661/750 Originof the Acronym: S = Created by Simbad, the CDS Database

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