Henry Joy McCracken astrophysicien irlandais
McCracken, Henry Joy, 19..-....
![Sudoc [ABES], France](/viaf/images/flags/SUDOC.png "Sudoc [ABES], France")
VIAF ID: 307509780 (Personal)
Permalink: http://viaf.org/viaf/307509780
Preferred Forms
4xx's: Alternate Name Forms (9)
Works
| Title | Sources |
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| L’amplification par effet de lentillage pour étudier le lien entre les galaxies et les halos de matière noire dans les champs profonds de Euclid. |
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| Baryonic acoustic oscillations with emission line galaxies at intermediate redshift : the large-scale structure of the universe. |
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| THE BIMODAL GALAXY STELLAR MASS FUNCTION IN THE COSMOS SURVEY TOz∼ 1: A STEEP FAINT END AND A NEW GALAXY DICHOTOMY |
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| THE COLORS OF CENTRAL AND SATELLITE GALAXIES IN zCOSMOS OUT TOz≃ 0.8 AND IMPLICATIONS FOR QUENCHING |
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| COSMOS photometric redshifts with 30-Bands for 2-deg^2^ |
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| THE COSMOS-WIRCam NEAR-INFRARED IMAGING SURVEY. I.BzK-SELECTED PASSIVE AND STAR-FORMING GALAXY CANDIDATES ATz≳ 1.4 |
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| Détection de lumière diffuse intra-amas dans les amas de galaxies. |
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| Detection of diffuse intracluster light in galaxy clusters |
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| Dissecting photometric redshift for active galactic nucleus using XMM- and Chandra-COSMOS samples |
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| The emergence of massive quiescent galaxies at z~3 |
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| Environmental effects on the star formation activity in galaxies at z =~ 1.2 in the COSMOS field |
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| Evolution de la distribution des galaxies dans les grands relevés cosmologiques. |
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| THE EVOLUTION OF THE STELLAR MASS FUNCTIONS OF STAR-FORMING AND QUIESCENT GALAXIES TOz= 4 FROM THE COSMOS/UltraVISTA SURVEY |
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| An exponential decline at the bright end of the z = 6 galaxy luminosity function |
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| THE FMOS-COSMOS SURVEY OF STAR-FORMING GALAXIES ATz∼ 1.6. III. SURVEY DESIGN, PERFORMANCE, AND SAMPLE CHARACTERISTICS |
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| Magnifying the galaxy-halo connection in the Euclid Deep fields |
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| NEW CONSTRAINTS ON THE EVOLUTION OF THE STELLAR-TO-DARK MATTER CONNECTION: A COMBINED ANALYSIS OF GALAXY-GALAXY LENSING, CLUSTERING, AND STELLAR MASS FUNCTIONS FROMz= 0.2 toz= 1 |
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| Observation des oscillations baryoniques primordiales des galaxies à raie d’émission à décalage vers le rouge modéré : la structure aux grandes échelles dans l’univers.. |
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| Observational and theoretical constraints on galaxy evolution at high redshift |
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| An optical group catalog to z = 1 from the zCOSMOS 10 K sample |
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| A protocluster at z = 2.45 |
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| THE REDSHIFT AND NATURE OF AzTEC/COSMOS 1: A STARBURST GALAXY ATz= 4.6 |
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| REST-UV ABSORPTION LINES AS METALLICITY ESTIMATOR: THE METAL CONTENT OF STAR-FORMING GALAXIES ATz∼ 5 |
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| S‐COSMOS: TheSpitzerLegacy Survey of theHubble Space TelescopeACS 2 deg2COSMOS Field I: Survey Strategy and First Analysis |
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| THE SINS SURVEY: SINFONI INTEGRAL FIELD SPECTROSCOPY OFz∼ 2 STAR-FORMING GALAXIES |
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| SPECTRAL ENERGY DISTRIBUTIONS OF TYPE 1 ACTIVE GALACTIC NUCLEI IN THE COSMOS SURVEY. I. THEXMM-COSMOS SAMPLE |
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| The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes |
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| SPITZERBRIGHT, ULTRAVISTA FAINT SOURCES IN COSMOS: THE CONTRIBUTION TO THE OVERALL POPULATION OF MASSIVE GALAXIES ATz= 3–7 |
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| A strongly lensed massive ultracompact quiescent galaxy at z ~ 2.4 in the COSMOS/UltraVISTA field |
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| The VIPERS Multi-Lambda Survey. I. UV and near-IR observations, multi-colour catalogues, and photometric redshifts |
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| The VIPERS Multi-Lambda Survey. II. Diving with massive galaxies in 22 square degrees since z = 1.5 |
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| VIPERS view of the star formation history of early-type galaxies |
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| Virmos-VLT deep survey |
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| The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release |
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| The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population |
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| The VLA-COSMOS 3 GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to z ≲ 6 |
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| The VLA-COSMOS Survey – V. 324 MHz continuum observations |
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| The VLA-VIRMOS Deep Field. I. Radio observations probing the {mu}Jy source population |
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| The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface |
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| The VVDS: Early Results on the Large Scale Structure Distribution of Galaxies out to z~1.5 |
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| VVDS-SWIRE |
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| VVDS-SWIRE. Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2 < z < 2.1 selected from Spitzer IRAC 3.6 {mu}m and 4.5 {mu}m photometry |
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| The VVDS type-1 AGN sample: the faint end of the luminosity function |
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| The VVDS-VLA deep field. IV. Radio-optical properties |
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| Weak lensing calibrated M-T scaling relation of galaxy groups in the COSMOS field^{sstarf}^ |
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| Weak lensing measurement of galaxy clusters in the CFHTLS-wide survey |
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| A Wide‐Angle Tail Radio Galaxy in the COSMOS Field: Evidence for Cluster Formation |
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| The WIRCam Deep Survey I. Counts, colours, and mass-functions derived from near-infrared imaging in the CFHTLS deep fields |
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| The WIRCam Deep Survey II. Mass selected clustering |
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| The XMM-LSS survey. Survey design and first results |
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| The XMM‐Newton Wide‐Field Survey in the COSMOS Field. III. Optical Identification and Multiwavelength Properties of a Large Sample of X‐Ray–Selected Sources |
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| The XMM-Newton wide field survey in the COSMOS field: redshift evolution of AGN bias and subdominant role of mergers in triggering moderate-luminosity AGNs at redshifts up to 2.2 |
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| XMM-Newtonsurveys of the Canada-France Redshift Survey fields - II. The X-ray catalogues, the properties of the host galaxies and the redshift distribution |
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| zCOSMOS 10k-bright spectroscopic sample |
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| zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <z< 3 in the COSMOS Field |
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| The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z≃ 1 |
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| The zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8 |
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| The zCOSMOS redshift survey: how group environment alters global downsizing trends |
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| The zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1 |
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| The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties |
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| The zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at $z=0.2$–1 |
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| The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types |
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| The Zurich Extragalactic Bayesian Redshift Analyzer and its first application: COSMOS |
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