Details on Acronym: [SDK96] | |
[SDK96] | (Smail+Dressler+Kneib+, 1996) |
Write: | <<[SDK96] {A370} {R|P}N>> |
N: | 1+5 |
Object: | Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image) |
Stat: | is completely incorporated in Simbad |
Note: | HST observations of giant arcs. In ACO 370: N=1 new image 'R', separated in (Nos R1-R2), and N=5 peaks (Nos P1-P5). See also [FPM88], [KMF94], [MSQ99]. |
in source: | ACO 370 |
Ref: | =1996ApJ...469..508S |
by | SMAIL I. , DRESSLER A., KNEIB J., ELLIS R.S., COUCH W.J., SHARPLES R.M., OEMLER A.Jr |
Astrophys. J., 469, 508-518 (1996) | |
Hubble Space Telescope observations of giant arcs: high-resolution imaging of distant field galaxies. | |
o | MS 2137-23 = 1E 2137.3-2353. Arcs 'AN' in ACO 370 = [KMF94]. Arcs in ClG 2244-02 = [HLJ89]. Arcs in ACO 2218 = LPS. |
o | Fig1(b): <[KKF92] AN> (Nos B3, D2-D3) added. Fig.2, text: <[SDK96] A370 R> N=1, <[SDK96] A370 PN> (Nos P1-P5). |
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 |