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

Result of query: info cati KMF94]$

Details on Acronym:   [KMF94]
  
[KMF94] (Kneib+Mathez+Fort+, 1994)
Write:<<[KMF94] A>>
<<[KMF94] ANN>>
N: 4+44
Object:Arc + Arclet  (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:Study of arclets candidates in ACO 370.
N=4 system arcs: (Nos A-D).
N=34 arclets candidates in the A system, among (Nos A0-A59).
N=7 arclets (Nos B1-B3, C1-C2, D1-D2).
In the 2nd ref. 'A1' is separated in 2 images (Nos S1-S2) and 'A13' in 2 images (Nos Q1-Q2).
Objects with the same format are identical to the [FPM88] ones, except the inversions: [FPM88] A1 = [KMF94] A2, [FPM88] A2 = [KMF94] A1, [FPM88] B2 = [KMF94] B3, [FPM88] B3 = [KMF94] B2. See also [FPM88], [SDK96], [MSQ99]
in source:ACO 370
Ref:=1994A&A...286..701K
byKNEIB J.-P. , MATHEZ G., FORT B., MELLIER Y., SOUCAIL G., LONGARETTI P.-Y.
 Astron. Astrophys., 286, 701-717 (1994)
  "Redshift survey" up to b_{J}=27: distance of gravitational arclets behind Abell 370.
o<[KMF94] A> (Nos A-D). Table 1: <[KMF94] AN> N=34 among (Nos A0-A59), (Nos C1-C2, D1-D2).
Ref:=1998MNRAS.294..734A
byABDELSALAM H.M. , SAHA P., WILLIAMS L.L.R.
 Mon. Not. R. Astron. Soc., 294, 734-746 (1998)
  Non-parametric reconstruction of cluster mass distribution from strong lensing: modelling Abell 370.
oTable 1: <[KMF94] SN> (Nos S1-S2), <[KMF94] QN> (Nos Q1-Q2). Table 1: <[SDK96] A370 RN> (Nos R1-R2).
Originof the Acronym: S = Created by Simbad, the CDS Database