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WKP|Q56555840
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(WKP)Q56555840
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0000-0003-4494-8277
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7406740762
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scopus
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(OCoLC)Q56555840
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Graham P. Smith
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astronome
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fr
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Graham P. Smith
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researcher
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Graham P. Smith
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wetenschapper
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Graham P. Smith
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investigador
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Graham P. Smith
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Astronom
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Graham P. Smith
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astronomo
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Graham P. Smith
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astrónomo
‡9
es
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670
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‡a
Author's A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773
|
670
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‡a
Author's A CFH12k lensing survey of X-ray luminous galaxy clusters
|
670
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‡a
Author's A CFH12k lensing survey of X-ray luminous galaxy clusters. I. Weak lensing methodology
|
670
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‡a
Author's A CFH12k lensing survey of X-ray luminous galaxy clusters. II. Weak lensing analysis and global correlations
|
670
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‡a
Author's A Hubble Space Telescope lensing survey of X-ray-luminous galaxy clusters — II. A search for gravitationally lensed EROs⋆
|
670
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‡a
Author's A Hubble Space Telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z = 0.2
|
670
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|
|
‡a
Author's A Keck Survey for Gravitationally Lensed Lyα Emitters in the Redshift Range 8.5 < z < 10.4: New Constraints on the Contribution of Low‐Luminosity Sources to Cosmic Reionization
|
670
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‡a
Author's A Unique Small-Scale Gravitational Arc in A1201
|
670
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|
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‡a
Author's A Very Bright, Highly Magnified Lyman Break Galaxy atz= 3.07
|
670
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|
‡a
Author's A weak-lensing and near-infrared study of A3192: disassembling a richness class 3 Abell cluster
|
670
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‡a
Author's A Wide-Field Hubble Space Telescope Study of the Cluster Cl 0024+1654 at z=0.4. II. The Cluster Mass Distribution
|
670
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‡a
Author's A Wide-Field Hubble Space Telescope Survey of the Cluster Cl 0024+16 at z = 0.4. III. Spectroscopic Signatures of Environmental Evolution in Early-Type Galaxies
|
670
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‡a
Author's A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s
|
670
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‡a
Author's A Wide‐FieldHubble Space TelescopeSurvey of the Cluster Cl 0024+16 atz= 0.4. III. Spectroscopic Signatures of Environmental Evolution in Early‐Type Galaxies
|
670
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‡a
Author's AHubble Space TelescopeLensing Survey of X‐Ray Luminous Galaxy Clusters. I. A383
|
670
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‡a
Author's AHubble Space Telescopelensing survey of X-ray luminous galaxy clusters - III. A multiply imaged extremely red galaxy atz=1.6
|
670
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|
‡a
Author's AHubbleandSpitzerSpace Telescope Survey for Gravitationally Lensed Galaxies: Further Evidence for a Significant Population of Low‐Luminosity Galaxies beyond $z=7$
|
670
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‡a
Author's BUDHIES – III: the fate of H i and the quenching of galaxies in evolving environments
|
670
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‡a
Author's BUDHIES - III: the fate of HI and the quenching of galaxies in evolving environments
|
670
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|
|
‡a
Author's Combining Strong and Weak Gravitational Lensing in Abell 1689
|
670
|
|
|
‡a
Author's DeepHerschelview of obscured star formation in the Bullet cluster
|
670
|
|
|
‡a
Author's Detection of anti-correlation of hot and cold baryons in galaxy clusters
|
670
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|
|
‡a
Author's Discovery of the galaxy counterpart of HDF 850.1, the brightest submillimetre source in the Hubble Deep Field
|
670
|
|
|
‡a
Author's Discovery of the galaxy counterpart of HDF 850.1, the brightest submillimetre source in theHubble Deep Field
|
670
|
|
|
‡a
Author's First detection of the Sunyaev Zel'dovich effect increment atλ< 650 μm
|
670
|
|
|
‡a
Author's Galaxies under the Cosmic Microscope: A Gemini Multiobject Spectrograph Study of Lensed Disk Galaxy 289 in A2218
|
670
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|
‡a
Author's Galaxies under the cosmic microscope: resolved spectroscopy and new constraints on the z = 1 Tully-Fisher relation
|
670
|
|
|
‡a
Author's GALEX Observations of "Passive Spirals" in the Cluster Cl 0024+17: Clues to the Formation of S0 Galaxies
|
670
|
|
|
‡a
Author's Hubble space telescope observations of a spectacular new strong-lensing galaxy cluster: MACS J1149.5+2223 at z = 0.544
|
670
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|
|
‡a
Author's Improving the identification of high-zHerschelsources with position priors and optical/NIR and FIR/mm photometric redshifts
|
670
|
|
|
‡a
Author's LoCuSS: A COMPARISON OF CLUSTER MASS MEASUREMENTS FROMXMM-NEWTONAND SUBARU—TESTING DEVIATION FROM HYDROSTATIC EQUILIBRIUM AND NON-THERMAL PRESSURE SUPPORT
|
670
|
|
|
‡a
Author's LoCuSS: A COMPARISON OF SUNYAEV-ZEL'DOVICH EFFECT AND GRAVITATIONAL-LENSING MEASUREMENTS OF GALAXY CLUSTERS
|
670
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|
‡a
Author's LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
|
670
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|
|
‡a
Author's LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters atz= 0.2
|
670
|
|
|
‡a
Author's LoCuSS: hydrostatic mass measurements of the high-LX cluster sample – cross-calibration of Chandra and XMM–Newton
|
670
|
|
|
‡a
Author's LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
|
670
|
|
|
‡a
Author's LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters
|
670
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|
|
‡a
Author's LoCuSS: the connection between brightest cluster galaxy activity, gas cooling and dynamical disturbance of X-ray cluster cores
|
670
|
|
|
‡a
Author's LoCuSS: THE MASS DENSITY PROFILE OF MASSIVE GALAXY CLUSTERS ATz= 0.2,
|
670
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|
|
‡a
Author's LoCuSS: the near-infrared luminosity and weak-lensing mass scaling relation of galaxy clusters
|
670
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|
‡a
Author's LoCuSS: The Splashback Radius of Massive Galaxy Clusters and Its Dependence on Cluster Merger History
|
670
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‡a
Author's LoCuSS: THE SUNYAEV–ZEL'DOVICH EFFECT AND WEAK-LENSING MASS SCALING RELATION
|
670
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‡a
Author's Measuring8with Cluster Lensing: Biases from Unrelaxed Clusters
|
670
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‡a
Author's Near‐Infrared Spectroscopy andHubble Space TelescopeImaging of a Dusty Starburst Extremely Red Object
|
670
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‡a
Author's Optical and Infrared Nondetection of thez= 10 Galaxy behind Abell 1835
|
670
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‡a
Author's Resolved spectroscopy of a gravitationally lensed L* Lyman-break galaxy at z∼ 5
|
670
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‡a
Author's Scientific Synergy between LSST and Euclid
|
670
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‡a
Author's Separating Baryons and Dark Matter in Cluster Cores: A Full Two‐dimensional Lensing and Dynamic Analysis of Abell 383 and MS 2137−23
|
670
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‡a
Author's Strong lensing by a node of the cosmic web
|
670
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‡a
Author's The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole
|
670
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‡a
Author's The BUFFALO HST Survey
|
670
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|
‡a
Author's The discovery of a massive supercluster at z= 0.9 in the UKIDSS Deep eXtragalactic Survey
|
670
|
|
|
‡a
Author's The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451−03
|
670
|
|
|
‡a
Author's The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster
|
670
|
|
|
‡a
Author's The Herschel Lensing Survey (HLS): Overview
|
670
|
|
|
‡a
Author's The Intrinsic Properties of SMM J14011+0252
|
670
|
|
|
‡a
Author's The nature of a gravitationally lensed submillimetre arc in MS0451.6−0305: two interacting galaxies at z∼ 2.9?
|
670
|
|
|
‡a
Author's TheHerschelLensing Survey
|
670
|
|
|
‡a
Author's Truncation of galaxy dark matter halos in high density environments
|
670
|
|
|
‡a
Author's UV to IR SEDs of UV‐Selected Galaxies in the ELAIS Fields: Evolution of Dust Attenuation and Star Formation Activity from z = 0.7 to 0.2
|
670
|
|
|
‡a
Author's UV to IR SEDs of UV‐Selected Galaxies in the ELAIS Fields: Evolution of Dust Attenuation and Star Formation Activity fromz= 0.7 to 0.2
|
670
|
|
|
‡a
Author's What if LIGO’s gravitational wave detections are strongly lensed by massive galaxy clusters?
|
670
|
|
|
‡a
Author's ഗാലെക്സ് Observations of "Passive Spirals" in the Cluster Cl 0024+17: Clues to the Formation of S0 Galaxies
|
909
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‡a
(orcid) 0000000344948277
‡9
1
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909
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‡a
(scopus) 7406740762
‡9
1
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912
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‡a
buffalohstsurvey
‡A
The BUFFALO HST Survey
‡9
1
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919
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‡a
separatingbaryonsanddarkmatterinclustercoresafull2dimensionallensinganddynamicanalysisofabell383andms213723
‡A
Separating Baryons and Dark Matter in Cluster Cores: A Full Two‐dimensional Lensing and Dynamic Analysis of Abell 383 and MS 2137−23
‡9
1
|
919
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|
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‡a
birthofarelativisticjetfollowingthedisruptionofastarbyacosmologicalblackhole
‡A
The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole
‡9
1
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919
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‡a
stronglensingbyanodeofthecosmicweb
‡A
Strong lensing by a node of the cosmic web
‡9
1
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919
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‡a
brightz52lensedsubmillimetergalaxyinthefieldofabell773
‡A
A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773
‡9
1
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919
|
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‡a
cfh12klensingsurveyof10rayluminousgalaxyclusters
‡A
A CFH12k lensing survey of X-ray luminous galaxy clusters
‡9
1
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919
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‡a
cfh12klensingsurveyof10rayluminousgalaxyclusters1weaklensingmethodology
‡A
A CFH12k lensing survey of X-ray luminous galaxy clusters. I. Weak lensing methodology
‡9
1
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919
|
|
|
‡a
cfh12klensingsurveyof10rayluminousgalaxyclusters2weaklensinganalysisandglobalcorrelations
‡A
A CFH12k lensing survey of X-ray luminous galaxy clusters. II. Weak lensing analysis and global correlations
‡9
1
|
919
|
|
|
‡a
hubblespacetelescopelensingsurveyof10rayluminousgalaxyclusters2asearchforgravitationallylensederos
‡A
A Hubble Space Telescope lensing survey of X-ray-luminous galaxy clusters — II. A search for gravitationally lensed EROs⋆
‡9
1
|
919
|
|
|
‡a
hubblespacetelescopelensingsurveyof10rayluminousgalaxyclusters4massstructureandthermodynamicsofclustercoresatz02
‡A
A Hubble Space Telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z = 0.2
‡9
1
|
919
|
|
|
‡a
kecksurveyforgravitationallylensedlyαemittersintheredshiftrange85z104newconstraintsonthecontributionoflowluminositysourcestocosmicreionization
‡A
A Keck Survey for Gravitationally Lensed Lyα Emitters in the Redshift Range 8.5 < z < 10.4: New Constraints on the Contribution of Low‐Luminosity Sources to Cosmic Reionization
‡9
1
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919
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‡a
uniquesmallscalegravitationalarcin
‡A
A Unique Small-Scale Gravitational Arc in A1201
‡9
1
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919
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‡a
verybrighthighlymagnifiedlymanbreakgalaxyatz307
‡A
A Very Bright, Highly Magnified Lyman Break Galaxy atz= 3.07
‡9
1
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919
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‡a
weaklensingandnearinfraredstudyofa3192disassemblingarichnessclass3abellcluster
‡A
A weak-lensing and near-infrared study of A3192: disassembling a richness class 3 Abell cluster
‡9
1
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919
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‡a
widefieldhubblespacetelescopestudyofthecluster1500024+1654atz042theclustermassdistribution
‡A
A Wide-Field Hubble Space Telescope Study of the Cluster Cl 0024+1654 at z=0.4. II. The Cluster Mass Distribution
‡9
1
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919
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‡a
widefieldhubblespacetelescopesurveyofthecluster1500024+16atz043spectroscopicsignaturesofenvironmentalevolutioninearlytypegalaxies
‡A
A Wide-Field Hubble Space Telescope Survey of the Cluster Cl 0024+16 at z = 0.4. III. Spectroscopic Signatures of Environmental Evolution in Early-Type Galaxies
‡9
2
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919
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‡a
widefieldsurveyoftwoz05galaxyclustersidentifyingthephysicalprocessesresponsiblefortheobservedtransformationofspiralsintos0s
‡A
A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s
‡9
1
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919
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‡a
ahubblespacetelescopelensingsurveyof10rayluminousgalaxyclusters1a383
‡A
AHubble Space TelescopeLensing Survey of X‐Ray Luminous Galaxy Clusters. I. A383
‡9
1
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919
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‡a
ahubblespacetelescopelensingsurveyof10rayluminousgalaxyclusters3amultiplyimagedextremelyredgalaxyatz16
‡A
AHubble Space Telescopelensing survey of X-ray luminous galaxy clusters - III. A multiply imaged extremely red galaxy atz=1.6
‡9
1
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919
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‡a
ahubbleandspitzerspacetelescopesurveyforgravitationallylensedgalaxiesfurtherevidenceforasignificantpopulationoflowluminositygalaxiesbeyond$z7$
‡A
AHubbleandSpitzerSpace Telescope Survey for Gravitationally Lensed Galaxies: Further Evidence for a Significant Population of Low‐Luminosity Galaxies beyond $z=7$
‡9
1
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919
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‡a
budhies3thefateofh1andthequenchingofgalaxiesinevolvingenvironments
‡A
BUDHIES – III: the fate of H i and the quenching of galaxies in evolving environments
‡9
1
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919
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‡a
budhies3thefateofhiandthequenchingofgalaxiesinevolvingenvironments
‡A
BUDHIES - III: the fate of HI and the quenching of galaxies in evolving environments
‡9
1
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919
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‡a
combiningstrongandweakgravitationallensinginabell
‡A
Combining Strong and Weak Gravitational Lensing in Abell 1689
‡9
1
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919
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‡a
deepherschelviewofobscuredstarformationinthebulletcluster
‡A
DeepHerschelview of obscured star formation in the Bullet cluster
‡9
1
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919
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‡a
detectionofanticorrelationofhotandcoldbaryonsingalaxyclusters
‡A
Detection of anti-correlation of hot and cold baryons in galaxy clusters
‡9
1
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919
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‡a
discoveryofthegalaxycounterpartofhdf8501thebrightestsubmillimetresourceinthehubbledeepfield
‡A
Discovery of the galaxy counterpart of HDF 850.1, the brightest submillimetre source in the Hubble Deep Field
‡9
2
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919
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|
‡a
1detectionofthesunyaevzeldovicheffectincrementatλ650μm
‡A
First detection of the Sunyaev Zel'dovich effect increment atλ< 650 μm
‡9
1
|
919
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‡a
galaxiesunderthecosmicmicroscopeageminimultiobjectspectrographstudyoflenseddiskgalaxy289in
‡A
Galaxies under the Cosmic Microscope: A Gemini Multiobject Spectrograph Study of Lensed Disk Galaxy 289 in A2218
‡9
1
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919
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‡a
galaxiesunderthecosmicmicroscoperesolvedspectroscopyandnewconstraintsonthez1tullyfisherrelation
‡A
Galaxies under the cosmic microscope: resolved spectroscopy and new constraints on the z = 1 Tully-Fisher relation
‡9
1
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919
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‡a
galexobservationsofpassivespiralsinthecluster1500024+17cluestotheformationofs0galaxies
‡A
GALEX Observations of "Passive Spirals" in the Cluster Cl 0024+17: Clues to the Formation of S0 Galaxies
‡9
1
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919
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‡a
hubblespacetelescopeobservationsofaspectacularnewstronglensinggalaxyclustermacsj11495+2223atz0544
‡A
Hubble space telescope observations of a spectacular new strong-lensing galaxy cluster: MACS J1149.5+2223 at z = 0.544
‡9
1
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919
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‡a
improvingtheidentificationofhighzherschelsourceswithpositionpriorsandopticalnirandfir2000photometricredshifts
‡A
Improving the identification of high-zHerschelsources with position priors and optical/NIR and FIR/mm photometric redshifts
‡9
1
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919
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‡a
ഗലകസobservationsofpassivespiralsinthecluster1500024+17cluestotheformationofs0galaxies
‡A
ഗാലെക്സ് Observations of "Passive Spirals" in the Cluster Cl 0024+17: Clues to the Formation of S0 Galaxies
‡9
1
|
919
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‡a
whatifligosgravitationalwavedetectionsarestronglylensedbymassivegalaxyclusters
‡A
What if LIGO’s gravitational wave detections are strongly lensed by massive galaxy clusters?
‡9
1
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919
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‡a
locussacomparisonofclustermassmeasurementsfromxmmnewtonandsubarutestingdeviationfromhydrostaticequilibriumandnonthermalpressuresupport
‡A
LoCuSS: A COMPARISON OF CLUSTER MASS MEASUREMENTS FROMXMM-NEWTONAND SUBARU—TESTING DEVIATION FROM HYDROSTATIC EQUILIBRIUM AND NON-THERMAL PRESSURE SUPPORT
‡9
1
|
919
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‡a
uvtoirsedsofuvselectedgalaxiesintheelaisfieldsevolutionofdustattenuationandstarformationactivityfromz07to02
‡A
UV to IR SEDs of UV‐Selected Galaxies in the ELAIS Fields: Evolution of Dust Attenuation and Star Formation Activity fromz= 0.7 to 0.2
‡9
2
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919
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‡a
truncationofgalaxydarkmatterhalosinhighdensityenvironments
‡A
Truncation of galaxy dark matter halos in high density environments
‡9
1
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919
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‡a
locussacomparisonofsunyaevzeldovicheffectandgravitationallensingmeasurementsofgalaxyclusters
‡A
LoCuSS: A COMPARISON OF SUNYAEV-ZEL'DOVICH EFFECT AND GRAVITATIONAL-LENSING MEASUREMENTS OF GALAXY CLUSTERS
‡9
1
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919
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‡a
theherschellensingsurvey
‡A
TheHerschelLensing Survey
‡9
1
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919
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‡a
natureofagravitationallylensedsubmillimetrearcinms0451603052interactinggalaxiesatz29
‡A
The nature of a gravitationally lensed submillimetre arc in MS0451.6−0305: two interacting galaxies at z∼ 2.9?
‡9
1
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919
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‡a
intrinsicpropertiesofsmmj14011
‡A
The Intrinsic Properties of SMM J14011+0252
‡9
1
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919
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‡a
locussconnectingthedominanceandshapeofbrightestclustergalaxieswiththeassemblyhistoryofmassiveclusters
‡A
LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
‡9
1
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919
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‡a
herschellensingsurveyhlsoverview
‡A
The Herschel Lensing Survey (HLS): Overview
‡9
1
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919
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‡a
farinfraredsubmillimeterpropertiesofgalaxieslocatedbehindthebulletcluster
‡A
The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster
‡9
1
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919
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‡a
locuss1resultsfromstronglensinganalysisof20massivegalaxyclustersatz02
‡A
LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters atz= 0.2
‡9
1
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919
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‡a
distributionofdarkmatterandgasspanning6mpcaroundthepostmergergalaxyclusterms045103
‡A
The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451−03
‡9
1
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919
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‡a
discoveryofamassivesuperclusteratz09intheukidssdeepextragalacticsurvey
‡A
The discovery of a massive supercluster at z= 0.9 in the UKIDSS Deep eXtragalactic Survey
‡9
1
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919
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‡a
locusshydrostaticmassmeasurementsofthehigh60clustersamplecrosscalibrationofchandraandxmmnewton
‡A
LoCuSS: hydrostatic mass measurements of the high-LX cluster sample – cross-calibration of Chandra and XMM–Newton
‡9
1
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919
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‡a
locussscalingrelationsbetweengalaxyclustermassgasandstellarcontent
‡A
LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
‡9
1
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919
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‡a
locusssubaruweaklensingstudyof30galaxyclusters
‡A
LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters
‡9
1
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919
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‡a
locusstheconnectionbetweenbrightestclustergalaxyactivitygascoolinganddynamicaldisturbanceof10rayclustercores
‡A
LoCuSS: the connection between brightest cluster galaxy activity, gas cooling and dynamical disturbance of X-ray cluster cores
‡9
1
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919
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|
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‡a
locussthemassdensityprofileofmassivegalaxyclustersatz02
‡A
LoCuSS: THE MASS DENSITY PROFILE OF MASSIVE GALAXY CLUSTERS ATz= 0.2,
‡9
1
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919
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‡a
locussthenearinfraredluminosityandweaklensingmassscalingrelationofgalaxyclusters
‡A
LoCuSS: the near-infrared luminosity and weak-lensing mass scaling relation of galaxy clusters
‡9
1
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919
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‡a
locussthesplashbackradiusofmassivegalaxyclustersanditsdependenceonclustermergerhistory
‡A
LoCuSS: The Splashback Radius of Massive Galaxy Clusters and Its Dependence on Cluster Merger History
‡9
1
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919
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|
‡a
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LoCuSS: THE SUNYAEV–ZEL'DOVICH EFFECT AND WEAK-LENSING MASS SCALING RELATION
‡9
1
|
919
|
|
|
‡a
measuring8withclusterlensingbiasesfromunrelaxedclusters
‡A
Measuring8with Cluster Lensing: Biases from Unrelaxed Clusters
‡9
1
|
919
|
|
|
‡a
nearinfraredspectroscopyandhubblespacetelescopeimagingofadustystarburstextremelyredobject
‡A
Near‐Infrared Spectroscopy andHubble Space TelescopeImaging of a Dusty Starburst Extremely Red Object
‡9
1
|
919
|
|
|
‡a
opticalandinfrarednondetectionofthez10galaxybehindabell
‡A
Optical and Infrared Nondetection of thez= 10 Galaxy behind Abell 1835
‡9
1
|
919
|
|
|
‡a
resolvedspectroscopyofagravitationallylensed50lymanbreakgalaxyatz5
‡A
Resolved spectroscopy of a gravitationally lensed L* Lyman-break galaxy at z∼ 5
‡9
1
|
919
|
|
|
‡a
scientificsynergybetweenlsstandeuclid
‡A
Scientific Synergy between LSST and Euclid
‡9
1
|
943
|
|
|
‡a
120x
‡A
1201
‡9
1
|
943
|
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|
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168x
‡A
1689
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1
|
943
|
|
|
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025x
‡A
0252
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1
|
943
|
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|
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183x
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1835
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|
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LC|nb2022011521
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CAOONL|ncf10313290
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J9U|987007318838205171
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ERRR|12061827
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BNE|XX5568068
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NTA|074617303
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BNF|14517608
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NTA|069516685
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DNB|1214200125
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SUDOC|18762500X
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LC|n 84032384
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BIBSYS|4091152
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BIBSYS|4040354
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0 0 lived 0 0
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1
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