ClG J1621+0607 , the SIMBAD biblio

ClG J1621+0607 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST09:04:16


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Title First 3 Authors
2011ApJS..193....8B viz 525 63 Gemini/GMOS spectroscopy of 26 strong-lensing-selected galaxy cluster cores. BAYLISS M.B., HENNAWI J.F., GLADDERS M.D., et al.
2012MNRAS.420.3213O 172       D       C F     6 34 203 Combined strong and weak lensing analysis of 28 clusters from the Sloan giant arcs survey. OGURI M., BAYLISS M.B., DAHLE H., et al.
2011RAA....11.1185W 15       D               1 39 13 Lensing clusters of galaxies in the SDSS-III. WEN Z.-L., HAN J.-L. and JIANG Y.-Y.
2015MNRAS.449.2024S 16       D               1 106 30 The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects. SERENO M., GIOCOLI C., ETTORI S., et al.
2015MNRAS.450.3665S viz 16       D               1 430 35 CoMaLit - III. Literature catalogues of weak lensing clusters of galaxies (LC2). SERENO M.
2016MNRAS.455..892G viz 16       D               3 353 14 The galaxy cluster concentration-mass scaling relation. GROENER A.M., GOLDBERG D.M. and SERENO M.
2020ApJS..247...12S viz 17       D               1 845 43 Strong lens models for 37 clusters of galaxies from the SDSS giant Arcs Survey. SHARON K., BAYLISS M.B., DAHLE H., et al.
2021ApJ...911...82C viz 17       D               1 388 ~ Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data. CORASANITI P.-S., SERENO M. and ETTORI S.
2021ApJ...920...98R 17       D               1 73 ~ Core mass estimates in strong lensing galaxy clusters: a comparison between masses obtained from detailed lens models, single-halo lens models, and Einstein radii. REMOLINA GONZALEZ J.D., SHARON K., MAHLER G., et al.
2022ApJ...928...87F viz 108       D       C       2 75 12 The Strongest Cluster Lenses: An Analysis of the Relation between Strong Gravitational Lensing Strength and the Physical Properties of Galaxy Clusters. FOX C., MAHLER G., SHARON K., et al.

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