Peter Melchior researcher
Melchior, Peter
VIAF ID: 122254578 (Personal)
Permalink: http://viaf.org/viaf/122254578
Preferred Forms
- 100 1 _ ‡a Melchior, Peter
- 100 1 _ ‡a Melchior, Peter
- 100 0 _ ‡a Peter Melchior ‡c researcher
4xx's: Alternate Name Forms (1)
5xx's: Related Names (3)
- 551 _ _ ‡a Heidelberg ‡4 ortw ‡4 https://d-nb.info/standards/elementset/gnd#placeOfActivity
- 551 _ _ ‡a Ingolstadt ‡4 ortg ‡4 https://d-nb.info/standards/elementset/gnd#placeOfBirth
- 510 2 _ ‡a Universität Heidelberg ‡b Fakultät für Physik und Astronomie ‡4 affi ‡4 https://d-nb.info/standards/elementset/gnd#affiliation ‡e Affiliation
Works
Title | Sources |
---|---|
CLASH: a census of magnified star-forming galaxies at z ~ 6-8 | |
CLASH-VLT: spectroscopic confirmation of a z = 6.11 quintuply lensed galaxy in the Frontier Fields Cluster RXC J2248.7-4431 | |
The cluster lensing and supernova survey with Hubble (CLASH): strong-lensing analysis of A383 from 16-band HST/WFC3/ACS imaging | |
Comparing Dark Energy Survey andHST–CLASH observations of the galaxy cluster RXC J2248.7−4431: implications for stellar mass versus dark matter | |
Constraints on the richness–mass relation and the optical-SZE positional offset distribution for SZE-selected clusters | |
The contribution of halos with different mass ratios to the overall growth of cluster-sized halos | |
Core or Cusps: The Central Dark Matter Profile of a Strong Lensing Cluster with a Bright Central Image at Redshift 1 | |
Cosmological constraints from the convergence 1-point probability distribution | |
Cross-correlation redshift calibration without spectroscopic calibration samples in DES Science Verification Data | |
Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters | |
Crowdsourcing quality control for Dark Energy Survey images | |
The dark energy survey and operations: years 1 to 3 | |
Dark Energy Survey Year 1 results: the impact of galaxy neighbours on weak lensing cosmology with im3shape | |
Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog | |
Deconvolution with shapelets | |
Density mapping with weak lensing and phase information | |
Density split statistics: Joint model of counts and lensing in cells | |
The DES Science Verification weak lensing shear catalogues | |
Detecting galaxy-filament alignments in the Sloan Digital Sky Survey III | |
Detection of the kinematic Sunyaev–Zel'dovich effect with DES Year 1 and SPT | |
Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data | |
Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using deep generative models | |
Evidence for ubiquitous high-equivalent-width nebular emission in z ~ 7 galaxies: toward a clean measurement of the specific star-formation rate using a sample of bright, magnified galaxies | |
The evolution of active galactic nuclei in clusters of galaxies from the Dark Energy Survey | |
Filling the gaps: Gaussian mixture models from noisy, truncated or incomplete samples | |
Forward Global Photometric Calibration of the Dark Energy Survey | |
Galaxy halo truncation and giant arc surface brightness reconstruction in the cluster MACSJ1206.2-0847 | |
GalSim : The modular galaxy image simulation toolkit | |
Graph neural network-based resource allocation strategies for multi-object spectroscopy | |
Hubble Space Telescope combined strong and weak lensing analysis of the CLASH sample: mass and magnification models and systematic uncertainties | |
Image analysis for cosmology: results from the GREAT10 Galaxy Challenge | |
Imprint of DES superstructures on the cosmic microwave background | |
Improving weak lensing mass map reconstructions using Gaussian and sparsity priors: application to DES SV | |
In the Crosshair: Astrometric Exoplanet Detection with WFIRST's Diffraction Spikes | |
Inference from the small scales of cosmic shear with current and future Dark Energy Survey data | |
Intracluster light properties in the CLASH-VLT cluster MACS J1206.2-0847 | |
Joint measurement of lensing–galaxy correlations using SPT and DES SV data | |
Mapping and simulating systematics due to spatially varying observing conditions in DES science verification data | |
Models of the strongly lensed quasar DES J0408−5354 | |
A multicomponent matched filter cluster confirmation tool for eROSITA: initial application to the RASS and DES-SV data sets | |
The MUSIC of CLASH: predictions on the concentration-mass relation | |
No galaxy left behind: accurate measurements with the faintest objects in the Dark Energy Survey | |
Parametrizing arbitrary galaxy morphologies: potentials and pitfalls | |
The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters | |
Quantifying galaxy shapes: sérsiclets and beyond | |
Realistic simulations of gravitational lensing by galaxy clusters: extracting arc parameters from mock DUNE images | |
redMaGiC: selecting luminous red galaxies from the DES Science Verification data | |
Reliable shapelet image analysis | |
scarlet : Source separation in multi-band images by Constrained Matrix Factorization | |
DES science portal: Computing photometric redshifts | |
Scientific Synergy between LSST and Euclid | |
Shapelets for gravitational lensing and galaxy morphology studies | |
Shear-flexion cross-talk in weak-lensing measurements | |
Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13) | |
Unveiling the Dynamical State of Massive Clusters through the ICL Fraction | |
VDES J2325−5229 az= 2.7 gravitationally lensed quasar discovered using morphology-independent supervised machine learning | |
Weak gravitational lensing with deimos | |
Wide-field lensing mass maps from Dark Energy Survey science verification data: Methodology and detailed analysis |