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[PDF] Top 20 RCSLenS: The Red Cluster Sequence Lensing Survey

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RCSLenS: The Red Cluster Sequence Lensing Survey

RCSLenS: The Red Cluster Sequence Lensing Survey

... the RCSLenS lensing data set can be used for cross- correlation studies: the requirement for cross-correlation studies is far less restrictive than for auto-correlation ...Galaxy–galaxy lensing ... See full document

20

Cluster Cosmology Constraints from the 2500 deg^2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope

Cluster Cosmology Constraints from the 2500 deg^2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope

... SZ cluster sample, we have obtained approximately uni- form PISCO imaging for the majority of the previously confirmed SPT-SZ ...optical red-sequence tech- niques for a significant number of clusters ... See full document

41

Galaxies in X ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red Sequence Galaxy Luminosity Function

Galaxies in X ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red Sequence Galaxy Luminosity Function

... faint red sequence galaxies with increasing redshift (De Lucia et ...faint red sequence galaxies compared to the bright (and massive) ...the red sequence luminosity distribution ... See full document

16

RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey

RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey

... the lensing magnification derived from such models may be biased (Johnson & Sharon ...this survey have no redshift constraints, some have only a spectroscopic redshift of only one lensed galaxy, and ... See full document

20

Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more

Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more

... (2005) red-sequence cluster-finding ...candidate cluster overdensity is de- termined from a count of (colour-selected) galaxies within a cir- cle with a radius of ...the cluster and ... See full document

22

Discovery of a Rich Cluster at z = 1.63 Using the Rest-frame 1.6 μm ''Stellar Bump Sequence'' Method

Discovery of a Rich Cluster at z = 1.63 Using the Rest-frame 1.6 μm ''Stellar Bump Sequence'' Method

... μm red- sequence method and have extensive spectroscopy from the GCLASS ...as red squares, those with spectroscopic redshifts inconsistent with being clusters members are shown as green ...The ... See full document

11

MC2: A Deeper Look at ZwCl 2341.1+0000 with Bayesian Galaxy Clustering and Weak Lensing Analyses

MC2: A Deeper Look at ZwCl 2341.1+0000 with Bayesian Galaxy Clustering and Weak Lensing Analyses

... weak lensing catalog using the method of Fischer & Tyson (1997) on the Subaru image of ZwCl ...the cluster with the largest mass peak in the ...confirmed red sequence galaxies in the ... See full document

63

The formation history of massive cluster galaxies as revealed by CARLA

The formation history of massive cluster galaxies as revealed by CARLA

... early-type cluster galaxies at z > 1 is low and consistent with passive evolution for z ...full cluster population, it is no longer possible to model the galaxy formation history with a single formation ... See full document

19

MUSE spectroscopy and deep observations of a unique compact JWST target, lensing cluster CLIO

MUSE spectroscopy and deep observations of a unique compact JWST target, lensing cluster CLIO

... Spitzer survey of a unique compact lensing cluster CLIO at z = ...GAMA survey using spectroscopic ...CLIO cluster was identified for follow-up observations due to its almost unique ... See full document

17

Weak gravitational lensing in the red-sequence cluster survey 2

Weak gravitational lensing in the red-sequence cluster survey 2

... Another change of our world view was initiated in the 1930s by the work of Fritz Zwicky on groups of galaxies (galaxy clusters), but only became widely known after the work of Vera Rubin and her collaborators in the ... See full document

209

Simultaneous Gravitational and Refractive Lensing

Simultaneous Gravitational and Refractive Lensing

... avitational lensing produces non-unique solutions, see e.g. the Appendix in [3]; where additional effects are taken into account, such as refraction or limb darkening of an extended luminous source, the number of ... See full document

5

Testing New Weak Lensing Measurement Techniques With The Dark Energy Survey

Testing New Weak Lensing Measurement Techniques With The Dark Energy Survey

... Dark Energy Survey Collaboration, T. Abbott, F. B. Abdalla, J. Aleksi´c, S. Allam, A. Amara, D. Bacon, E. Balbinot, M. Banerji, K. Bechtol, A. Benoit-Lévy, G. M. Bernstein, E. Bertin, J. Blazek, C. Bonnett, S. ... See full document

168

The SAMI galaxy survey : the cluster redshift survey, target selection and cluster properties

The SAMI galaxy survey : the cluster redshift survey, target selection and cluster properties

... As noted in Section 3.2, the archived AAOmega data targeted galaxies with fainter magnitudes (in particular the Bou´e et al. 2008 observations) and therefore have no existing object in the SAMI- CRS input catalogue. Of ... See full document

26

Rau, Markus Michael
  

(2017):


	Photometric redshift estimation for precision cosmology.


Dissertation, LMU München: Fakultät für Physik

Rau, Markus Michael (2017): Photometric redshift estimation for precision cosmology. Dissertation, LMU München: Fakultät für Physik

... photometric redshift information (e.g. Newman, 2008; Ménard et al., 2013; Morrison et al., 2017) are already an integral part of modern photometric redshift strategies (Hildebrandt et al., 2017; Hoyle et al., 2017). As ... See full document

185

Planck 2015 results  XIII  Cosmological parameters

Planck 2015 results XIII Cosmological parameters

... ing COBE and WMAP, dedicated to measurements of the CMB anisotropies. The first cosmological results from Planck were reported in a series of papers (for an overview see Planck Collaboration I 2014, and references ... See full document

63

Formal description of sequence-based voucherless Fungi: promises and pitfalls, and how to resolve them

Formal description of sequence-based voucherless Fungi: promises and pitfalls, and how to resolve them

... of sequence-based, voucherless Fungi, given that environmental sequencing has accumulated more than one billion fungal ITS reads in the Sequence Read Archive, about 1,000 times as many as fungal ITS ... See full document

24

The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses

The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses

... We thank Monique Arnaud, Gabriel Pratt, Keiichi Umetsu, James Jee, Edo van Uitert, Anja von der Linden, Doug Applegate, Ken Rines and Douglas Scott for useful discussions. We are also grateful to Keiichi Umetsu and James ... See full document

30

Weak Lensing Calibrated M-T Scaling Relation of Galaxy Groups in the COSMOS Field

Weak Lensing Calibrated M-T Scaling Relation of Galaxy Groups in the COSMOS Field

... Simulations indicate that HSE masses may be biased low due to non-thermal pressure support and kinetic pressure from gas motion (e.g., Nagai et al. 2007; Shaw et al. 2010; Rasia et al. 2012). Furthermore, the deviation ... See full document

11

Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey

Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey

... TS, DA, and FR acknowledge support from the German Federal Ministry of Economics and Technology (BMWi) pro- vided through DLR under projects 50 OR 1210, 50 OR 1308, 50 OR 1407, and 50 OR 1610. TS also acknowledges sup- ... See full document

49

Optimising cluster survey design for planning schistosomiasis preventive chemotherapy

Optimising cluster survey design for planning schistosomiasis preventive chemotherapy

... Two-stage cluster surveys aiming to provide treatment guidelines for both types of infection should therefore optimise sample size for schistosomiasis, and STH prevalence estimates of sufficient accuracy will ... See full document

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