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 |
by | KNEIB 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 |
by | ABDELSALAM 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. | |
o | Table 1: <[KMF94] SN> (Nos S1-S2), <[KMF94] QN> (Nos Q1-Q2). Table 1: <[SDK96] A370 RN> (Nos R1-R2). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |