[MSG2014] 8a , the SIMBAD biblio

[MSG2014] 8a , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:51:03


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Title First 3 Authors
2014MNRAS.438.1417M 15       D               1 51 43 CLASH: z ∼ 6 young galaxy candidate quintuply lensed by the frontier field cluster RXC J2248.7-4431. MONNA A., SEITZ S., GREISEL N., et al.
2014MNRAS.444..268R viz 15       D               1 267 190 Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high-redshift studies. RICHARD J., JAUZAC M., LIMOUSIN M., et al.
2014ApJ...797...48J 15       D               1 253 178 Lens models and magnification maps of the six Hubble frontier fields clusters. JOHNSON T.L., SHARON K., BAYLISS M.B., et al.
2015ApJ...801...44Z viz 16       D               1 444 215 Hubble Space Telescope combined strong and weak lensing analysis of the CLASH sample: mass and magnification models and systematic uncertainties. ZITRIN A., FABRIS A., MERTEN J., et al.
2016A&A...587A..80C 16       D               2 53 99 CLASH-VLT: A highly precise strong lensing model of the galaxy cluster RXC J2248.7-4431 (Abell S1063) and prospects for cosmography. CAMINHA G.B., GRILLO C., ROSATI P., et al.
2016MNRAS.459.3447D 16       D               1 46 17 A free-form mass model of the Hubble Frontier Fields cluster AS1063 (RXC J2248.7-4431) with over one hundred constraints. DIEGO J.M., BROADHURST T., WONG J., et al.
2017A&A...599A..28K 16       D               1 197 48 MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063. II. Properties of low luminosity Lyman α emitters at z> 3. KARMAN W., CAPUTI K.I., CAMINHA G.B., et al.
2018ApJ...855....4K viz 16       D               1 1029 127 Size-luminosity relations and UV luminosity functions at z = 6-9 simultaneously derived from the complete Hubble Frontier Fields data. KAWAMATA R., ISHIGAKI M., SHIMASAKU K., et al.
2020PASP..132d4501T                     1 11 ~ Comparison of multi-class and binary classification machine learning models in identifying strong gravitational lenses. TEIMOORINIA H., TOYONAGA R.D., FABBRO S., et al.

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