Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

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: GtowardsCl = Galaxy towards a 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