Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high-redshift studies

By J. Richard, M. Jauzac, M. Limousin, E. Jullo, B. Clément, H. Ebeling, Jean-Paul Kneib, H. Atek, P. Natarajan, E. Egami and 2 more. 2014

138 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/a9e3c3d6fd864263869a6a2a8ea17a099806ef66

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In Astronomy and Astrophysics

1. Richard S. Ellis
2. R. Bouwens
3. P. Oesch
4. G. Illingworth
5. J. Dunlop
6. M. Franx
7. M. Ouchi
8. P. V. van Dokkum

In Instrumentation

1. Richard S. Ellis
2. R. Bouwens
3. P. Oesch
4. G. Illingworth
5. J. Dunlop
6. M. Franx
7. P. V. van Dokkum
8. Brant Robertson

Citations in the corpus

• The extreme faint end of the UV luminosity function at z ∼ 6 through gravitational telescopes: a comprehensive assessment of strong lensing uncertainties (2018, background): “…cosmic telescopes, magnifying background galaxies in the strong gravitational lensing regime, and as such offer a viable route to reach beyond the current observational limit (Maizy et al. 2010; Kneib & Natarajan 2011; Sharon et al. 2012; Postman et al. 2012; Richard et al. 2014b; Coe et al. 2015).”
• HUBBLE FRONTIER FIELDS FIRST COMPLETE CLUSTER DATA: FAINT GALAXIES AT z ∼ 5–10 FOR UV LUMINOSITY FUNCTIONS AND COSMIC REIONIZATION (2014, methodology): “…Mass Models Mass models of Abell 2744 are also made by the five independent groups: M. Bradač (PI), The Clusters As TelescopeS (CATS) team (Co-PI’s J.P Kneib, P. Natarajan; see Richard et al. 2014), J. Merten & A. Zitrin (CoPI’s), K. Sharon (PI; see Johnson et al. 2014), and L. Williams (PI).”
• The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: the z = 9 luminosity function and further evidence for a smooth decline in ultraviolet luminosity density at z≥ 8 (2016, methodology): “For the HFF fields analysed here, we have employed the CATS (Richard et al. 2014) and Zitrin LTM (Zitrin et al. 2013) lensing maps.”
• HUBBLE SPACE TELESCOPE COMBINED STRONG AND WEAK LENSING ANALYSIS OF THE CLASH SAMPLE: MASS AND MAGNIFICATION MODELS AND SYSTEMATIC UNCERTAINTIES (2014, methodology): “Other mass models for this cluster were published, both in the SL and WL regimes (e.g., Jauzac et al. 2012; Limousin et al. 2012; Diego et al. 2014; Richard et al. 2014; Johnson et al. 2014; Medezinski et al. 2013).”
• The Frontier Fields: Survey Design and Initial Results (2016, methodology): “…and new ground-based spectroscopic campaigns have greatly increased the number and accuracy of the redshifts for the background lensed FF galaxies (Wang et al. 2015, Hoag et al. 2015; Johnson et al. 2014; Richard et al. 2014; Ebeling et al. 2014; Grillo et al. 2015; Balestra et al. 2015).”
• The z ∼ 6 Luminosity Function Fainter than −15 mag from the Hubble Frontier Fields: The Impact of Magnification Uncertainties (2016, methodology): “For our magnification estimates for individual sources, we take the median of the model magnifications from the CATS (Jullo & Kneib 2009; Richard et al. 2014; Jauzac et al. 2015a,b),GLAFIC (Oguri 2010; Ishigaki et al. 2015; Kawamata et al. 2016), Sharon/Johnson (John- 5 son et al. 2014), and Zitrin…”
• Dust in the Reionization Era: ALMA Observations of a z = 8.38 Gravitationally Lensed Galaxy (2017, methodology): “Moreover a web tool11 enables us to estimate the magnification for Abell2744 YD4 from parametric high resolution models, i.e. version 3.1 of the CATS model (Richard et al. 2014), version 3 of Johnson et al. (2014), version 3 of Merten et al. (2011) and version 3 of GLAFIC (Ishigaki et al. 2015).”
• LENS MODELS AND MAGNIFICATION MAPS OF THE SIX HUBBLE FRONTIER FIELDS CLUSTERS (2014, methodology): “We fix the redshifts of image systems # 4 and 6 to the spectroscopic redshifts obtained by Richard et al. (2014).”
• New redshift z ≃ 9 galaxies in the Hubble Frontier Fields: implications for early evolution of the UV luminosity density (2014, methodology): “To derive these we have utilised the magnification map at z ' 9 produced by the CATS team3 (e.g. Richard et al. 2014) and have con- 2 www.cfht.hawaii.edu/ arnouts/LEPHARE/lephare.html 3 http://archive.stsci.edu/prepds/frontier/lensmodels c© 0000 RAS, MNRAS 000, 000–000 c© 0000 RAS, MNRAS 000,…”