VIAF

Virtual International Authority File

Search

Leader     00000nz a2200037n 45 0
001     WKP|Q56555840  (VIAF cluster)  (Authority/Source Record)
003     WKP
005     20241121000048.0
008     241121nneanz||abbn n and d
035 ‎‡a  (WKP)Q56555840‏
024 ‎‡a  0000-0003-4494-8277‏ ‎‡2  orcid‏
024 ‎‡a  7406740762‏ ‎‡2  scopus‏
035 ‎‡a  (OCoLC)Q56555840‏
100 0 ‎‡a  Graham P. Smith‏ ‎‡c  astronome‏ ‎‡9  fr‏
375 ‎‡a  1‏ ‎‡2  iso5218‏
400 0 ‎‡a  Graham P. Smith‏ ‎‡c  researcher‏ ‎‡9  en‏
400 0 ‎‡a  Graham P. Smith‏ ‎‡c  wetenschapper‏ ‎‡9  nl‏
400 0 ‎‡a  Graham P. Smith‏ ‎‡c  investigador‏ ‎‡9  ast‏
400 0 ‎‡a  Graham P. Smith‏ ‎‡c  Astronom‏ ‎‡9  de‏
400 0 ‎‡a  Graham P. Smith‏ ‎‡c  astronomo‏ ‎‡9  it‏
400 0 ‎‡a  Graham P. Smith‏ ‎‡c  astrónomo‏ ‎‡9  es‏
670 ‎‡a  Author's A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773‏
670 ‎‡a  Author's A CFH12k lensing survey of X-ray luminous galaxy clusters‏
670 ‎‡a  Author's A CFH12k lensing survey of X-ray luminous galaxy clusters. I. Weak lensing methodology‏
670 ‎‡a  Author's A CFH12k lensing survey of X-ray luminous galaxy clusters. II. Weak lensing analysis and global correlations‏
670 ‎‡a  Author's A Hubble Space Telescope lensing survey of X-ray-luminous galaxy clusters — II. A search for gravitationally lensed EROs⋆‏
670 ‎‡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 ‎‡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 ‎‡a  Author's A Unique Small-Scale Gravitational Arc in A1201‏
670 ‎‡a  Author's A Very Bright, Highly Magnified Lyman Break Galaxy atz= 3.07‏
670 ‎‡a  Author's A weak-lensing and near-infrared study of A3192: disassembling a richness class 3 Abell cluster‏
670 ‎‡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 ‎‡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 ‎‡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 ‎‡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 ‎‡a  Author's AHubble Space TelescopeLensing Survey of X‐Ray Luminous Galaxy Clusters. I. A383‏
670 ‎‡a  Author's AHubble Space Telescopelensing survey of X-ray luminous galaxy clusters - III. A multiply imaged extremely red galaxy atz=1.6‏
670 ‎‡a  Author's AHubbleandSpitzerSpace Telescope Survey for Gravitationally Lensed Galaxies: Further Evidence for a Significant Population of Low‐Luminosity Galaxies beyond $z=7$‏
670 ‎‡a  Author's BUDHIES – III: the fate of H i and the quenching of galaxies in evolving environments‏
670 ‎‡a  Author's BUDHIES - III: the fate of HI and the quenching of galaxies in evolving environments‏
670 ‎‡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 ‎‡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 ‎‡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 ‎‡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 ‎‡a  Author's LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters‏
670 ‎‡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 ‎‡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 ‎‡a  Author's LoCuSS: the near-infrared luminosity and weak-lensing mass scaling relation of galaxy clusters‏
670 ‎‡a  Author's LoCuSS: The Splashback Radius of Massive Galaxy Clusters and Its Dependence on Cluster Merger History‏
670 ‎‡a  Author's LoCuSS: THE SUNYAEV–ZEL'DOVICH EFFECT AND WEAK-LENSING MASS SCALING RELATION‏
670 ‎‡a  Author's Measuring8with Cluster Lensing: Biases from Unrelaxed Clusters‏
670 ‎‡a  Author's Near‐Infrared Spectroscopy andHubble Space TelescopeImaging of a Dusty Starburst Extremely Red Object‏
670 ‎‡a  Author's Optical and Infrared Nondetection of thez= 10 Galaxy behind Abell 1835‏
670 ‎‡a  Author's Resolved spectroscopy of a gravitationally lensed L* Lyman-break galaxy at z∼ 5‏
670 ‎‡a  Author's Scientific Synergy between LSST and Euclid‏
670 ‎‡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 ‎‡a  Author's Strong lensing by a node of the cosmic web‏
670 ‎‡a  Author's The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole‏
670 ‎‡a  Author's The BUFFALO HST Survey‏
670 ‎‡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 ‎‡a  (orcid) 0000000344948277‏ ‎‡9  1‏
909 ‎‡a  (scopus) 7406740762‏ ‎‡9  1‏
912 ‎‡a  buffalohstsurvey‏ ‎‡A  The BUFFALO HST Survey‏ ‎‡9  1‏
919 ‎‡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 ‎‡a  birthofarelativisticjetfollowingthedisruptionofastarbyacosmologicalblackhole‏ ‎‡A  The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole‏ ‎‡9  1‏
919 ‎‡a  stronglensingbyanodeofthecosmicweb‏ ‎‡A  Strong lensing by a node of the cosmic web‏ ‎‡9  1‏
919 ‎‡a  brightz52lensedsubmillimetergalaxyinthefieldofabell773‏ ‎‡A  A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773‏ ‎‡9  1‏
919 ‎‡a  cfh12klensingsurveyof10rayluminousgalaxyclusters‏ ‎‡A  A CFH12k lensing survey of X-ray luminous galaxy clusters‏ ‎‡9  1‏
919 ‎‡a  cfh12klensingsurveyof10rayluminousgalaxyclusters1weaklensingmethodology‏ ‎‡A  A CFH12k lensing survey of X-ray luminous galaxy clusters. I. Weak lensing methodology‏ ‎‡9  1‏
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
919 ‎‡a  uniquesmallscalegravitationalarcin‏ ‎‡A  A Unique Small-Scale Gravitational Arc in A1201‏ ‎‡9  1‏
919 ‎‡a  verybrighthighlymagnifiedlymanbreakgalaxyatz307‏ ‎‡A  A Very Bright, Highly Magnified Lyman Break Galaxy atz= 3.07‏ ‎‡9  1‏
919 ‎‡a  weaklensingandnearinfraredstudyofa3192disassemblingarichnessclass3abellcluster‏ ‎‡A  A weak-lensing and near-infrared study of A3192: disassembling a richness class 3 Abell cluster‏ ‎‡9  1‏
919 ‎‡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
919 ‎‡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
919 ‎‡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
919 ‎‡a  ahubblespacetelescopelensingsurveyof10rayluminousgalaxyclusters1a383‏ ‎‡A  AHubble Space TelescopeLensing Survey of X‐Ray Luminous Galaxy Clusters. I. A383‏ ‎‡9  1‏
919 ‎‡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
919 ‎‡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
919 ‎‡a  budhies3thefateofh1andthequenchingofgalaxiesinevolvingenvironments‏ ‎‡A  BUDHIES – III: the fate of H i and the quenching of galaxies in evolving environments‏ ‎‡9  1‏
919 ‎‡a  budhies3thefateofhiandthequenchingofgalaxiesinevolvingenvironments‏ ‎‡A  BUDHIES - III: the fate of HI and the quenching of galaxies in evolving environments‏ ‎‡9  1‏
919 ‎‡a  combiningstrongandweakgravitationallensinginabell‏ ‎‡A  Combining Strong and Weak Gravitational Lensing in Abell 1689‏ ‎‡9  1‏
919 ‎‡a  deepherschelviewofobscuredstarformationinthebulletcluster‏ ‎‡A  DeepHerschelview of obscured star formation in the Bullet cluster‏ ‎‡9  1‏
919 ‎‡a  detectionofanticorrelationofhotandcoldbaryonsingalaxyclusters‏ ‎‡A  Detection of anti-correlation of hot and cold baryons in galaxy clusters‏ ‎‡9  1‏
919 ‎‡a  discoveryofthegalaxycounterpartofhdf8501thebrightestsubmillimetresourceinthehubbledeepfield‏ ‎‡A  Discovery of the galaxy counterpart of HDF 850.1, the brightest submillimetre source in the Hubble Deep Field‏ ‎‡9  2‏
919 ‎‡a  1detectionofthesunyaevzeldovicheffectincrementatλ650μm‏ ‎‡A  First detection of the Sunyaev Zel'dovich effect increment atλ< 650 μm‏ ‎‡9  1‏
919 ‎‡a  galaxiesunderthecosmicmicroscopeageminimultiobjectspectrographstudyoflenseddiskgalaxy289in‏ ‎‡A  Galaxies under the Cosmic Microscope: A Gemini Multiobject Spectrograph Study of Lensed Disk Galaxy 289 in A2218‏ ‎‡9  1‏
919 ‎‡a  galaxiesunderthecosmicmicroscoperesolvedspectroscopyandnewconstraintsonthez1tullyfisherrelation‏ ‎‡A  Galaxies under the cosmic microscope: resolved spectroscopy and new constraints on the z = 1 Tully-Fisher relation‏ ‎‡9  1‏
919 ‎‡a  galexobservationsofpassivespiralsinthecluster1500024+17cluestotheformationofs0galaxies‏ ‎‡A  GALEX Observations of "Passive Spirals" in the Cluster Cl 0024+17: Clues to the Formation of S0 Galaxies‏ ‎‡9  1‏
919 ‎‡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
919 ‎‡a  improvingtheidentificationofhighzherschelsourceswithpositionpriorsandopticalnirandfir2000photometricredshifts‏ ‎‡A  Improving the identification of high-zHerschelsources with position priors and optical/NIR and FIR/mm photometric redshifts‏ ‎‡9  1‏
919 ‎‡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 ‎‡a  whatifligosgravitationalwavedetectionsarestronglylensedbymassivegalaxyclusters‏ ‎‡A  What if LIGO’s gravitational wave detections are strongly lensed by massive galaxy clusters?‏ ‎‡9  1‏
919 ‎‡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 ‎‡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
919 ‎‡a  truncationofgalaxydarkmatterhalosinhighdensityenvironments‏ ‎‡A  Truncation of galaxy dark matter halos in high density environments‏ ‎‡9  1‏
919 ‎‡a  locussacomparisonofsunyaevzeldovicheffectandgravitationallensingmeasurementsofgalaxyclusters‏ ‎‡A  LoCuSS: A COMPARISON OF SUNYAEV-ZEL'DOVICH EFFECT AND GRAVITATIONAL-LENSING MEASUREMENTS OF GALAXY CLUSTERS‏ ‎‡9  1‏
919 ‎‡a  theherschellensingsurvey‏ ‎‡A  TheHerschelLensing Survey‏ ‎‡9  1‏
919 ‎‡a  natureofagravitationallylensedsubmillimetrearcinms0451603052interactinggalaxiesatz29‏ ‎‡A  The nature of a gravitationally lensed submillimetre arc in MS0451.6−0305: two interacting galaxies at z∼ 2.9?‏ ‎‡9  1‏
919 ‎‡a  intrinsicpropertiesofsmmj14011‏ ‎‡A  The Intrinsic Properties of SMM J14011+0252‏ ‎‡9  1‏
919 ‎‡a  locussconnectingthedominanceandshapeofbrightestclustergalaxieswiththeassemblyhistoryofmassiveclusters‏ ‎‡A  LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters‏ ‎‡9  1‏
919 ‎‡a  herschellensingsurveyhlsoverview‏ ‎‡A  The Herschel Lensing Survey (HLS): Overview‏ ‎‡9  1‏
919 ‎‡a  farinfraredsubmillimeterpropertiesofgalaxieslocatedbehindthebulletcluster‏ ‎‡A  The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster‏ ‎‡9  1‏
919 ‎‡a  locuss1resultsfromstronglensinganalysisof20massivegalaxyclustersatz02‏ ‎‡A  LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters atz= 0.2‏ ‎‡9  1‏
919 ‎‡a  distributionofdarkmatterandgasspanning6mpcaroundthepostmergergalaxyclusterms045103‏ ‎‡A  The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451−03‏ ‎‡9  1‏
919 ‎‡a  discoveryofamassivesuperclusteratz09intheukidssdeepextragalacticsurvey‏ ‎‡A  The discovery of a massive supercluster at z= 0.9 in the UKIDSS Deep eXtragalactic Survey‏ ‎‡9  1‏
919 ‎‡a  locusshydrostaticmassmeasurementsofthehigh60clustersamplecrosscalibrationofchandraandxmmnewton‏ ‎‡A  LoCuSS: hydrostatic mass measurements of the high-LX cluster sample – cross-calibration of Chandra and XMM–Newton‏ ‎‡9  1‏
919 ‎‡a  locussscalingrelationsbetweengalaxyclustermassgasandstellarcontent‏ ‎‡A  LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content‏ ‎‡9  1‏
919 ‎‡a  locusssubaruweaklensingstudyof30galaxyclusters‏ ‎‡A  LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters‏ ‎‡9  1‏
919 ‎‡a  locusstheconnectionbetweenbrightestclustergalaxyactivitygascoolinganddynamicaldisturbanceof10rayclustercores‏ ‎‡A  LoCuSS: the connection between brightest cluster galaxy activity, gas cooling and dynamical disturbance of X-ray cluster cores‏ ‎‡9  1‏
919 ‎‡a  locussthemassdensityprofileofmassivegalaxyclustersatz02‏ ‎‡A  LoCuSS: THE MASS DENSITY PROFILE OF MASSIVE GALAXY CLUSTERS ATz= 0.2,‏ ‎‡9  1‏
919 ‎‡a  locussthenearinfraredluminosityandweaklensingmassscalingrelationofgalaxyclusters‏ ‎‡A  LoCuSS: the near-infrared luminosity and weak-lensing mass scaling relation of galaxy clusters‏ ‎‡9  1‏
919 ‎‡a  locussthesplashbackradiusofmassivegalaxyclustersanditsdependenceonclustermergerhistory‏ ‎‡A  LoCuSS: The Splashback Radius of Massive Galaxy Clusters and Its Dependence on Cluster Merger History‏ ‎‡9  1‏
919 ‎‡a  locussthesunyaevzeldovicheffectandweaklensingmassscalingrelation‏ ‎‡A  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 ‎‡a  168x‏ ‎‡A  1689‏ ‎‡9  1‏
943 ‎‡a  025x‏ ‎‡A  0252‏ ‎‡9  1‏
943 ‎‡a  183x‏ ‎‡A  1835‏ ‎‡9  1‏
946 ‎‡a  b‏ ‎‡9  1‏
996 ‎‡2  LC|no2019009591
996 ‎‡2  CAOONL|ncf10396204
996 ‎‡2  ISNI|0000000393640658
996 ‎‡2  NTA|29430116X
996 ‎‡2  RERO|A028525853
996 ‎‡2  JPG|500086583
996 ‎‡2  BNF|13324552
996 ‎‡2  ISNI|0000000442748834
996 ‎‡2  LC|n 86846404
996 ‎‡2  SUDOC|162614179
996 ‎‡2  BIBSYS|15031324
996 ‎‡2  BNF|13598981
996 ‎‡2  ISNI|0000000068744293
996 ‎‡2  LC|nb2018003890
996 ‎‡2  BIBSYS|90876359
996 ‎‡2  NKC|xx0021299
996 ‎‡2  ISNI|0000000047987552
996 ‎‡2  ISNI|0000000373292713
996 ‎‡2  CAOONL|ncf10080616
996 ‎‡2  BNC|981060957839906706
996 ‎‡2  NTA|092836534
996 ‎‡2  ISNI|0000000003206312
996 ‎‡2  J9U|987007439186105171
996 ‎‡2  RERO|A003455214
996 ‎‡2  ISNI|0000000114505032
996 ‎‡2  RERO|A025911021
996 ‎‡2  LC|n 91067509
996 ‎‡2  LC|nr 93048114
996 ‎‡2  BNE|XX945016
996 ‎‡2  NUKAT|n 2009154107
996 ‎‡2  NUKAT|n 94300932
996 ‎‡2  BIBSYS|90218083
996 ‎‡2  J9U|987007390555505171
996 ‎‡2  DNB|1020416637
996 ‎‡2  J9U|987007429010705171
996 ‎‡2  LC|n 98059265
996 ‎‡2  ISNI|000000002168844X
996 ‎‡2  BNF|15068739
996 ‎‡2  ISNI|0000000079799214
996 ‎‡2  LC|n 85114779
996 ‎‡2  CAOONL|ncf12104977
996 ‎‡2  SUDOC|031166261
996 ‎‡2  ISNI|0000000496357222
996 ‎‡2  BNC|981060957839506706
996 ‎‡2  RERO|A028525257
996 ‎‡2  SUDOC|273008102
996 ‎‡2  J9U|987009347792905171
996 ‎‡2  NII|DA00696889
996 ‎‡2  BIBSYS|37452
996 ‎‡2  LC|no2004106688
996 ‎‡2  NII|DA03261168
996 ‎‡2  DNB|1149161957
996 ‎‡2  NTA|371384451
996 ‎‡2  BNF|15600882
996 ‎‡2  LC|n 96039135
996 ‎‡2  NUKAT|n 2007122992
996 ‎‡2  LC|n 86042356
996 ‎‡2  CAOONL|ncf12111628
996 ‎‡2  ISNI|0000000102642670
996 ‎‡2  SUDOC|031365981
996 ‎‡2  LC|nb2011009573
996 ‎‡2  LC|n 90637375
996 ‎‡2  LC|no2005067552
996 ‎‡2  BIBSYS|13021998
996 ‎‡2  NTA|105445886
996 ‎‡2  LC|n 87151932
996 ‎‡2  BIBSYS|99045618
996 ‎‡2  CAOONL|ncf11491304
996 ‎‡2  JPG|500101934
996 ‎‡2  BNF|15151236
996 ‎‡2  ISNI|0000000050282705
996 ‎‡2  LC|nb2010019370
996 ‎‡2  LC|no2002084966
996 ‎‡2  PLWABN|9810646890905606
996 ‎‡2  SUDOC|080180426
996 ‎‡2  J9U|987007460155105171
996 ‎‡2  NUKAT|n 2008094123
996 ‎‡2  BNF|12470016
996 ‎‡2  LC|n 82019887
996 ‎‡2  LC|n 80086970
996 ‎‡2  ISNI|0000000080232020
996 ‎‡2  LC|nb2007004380
996 ‎‡2  BNF|12202121
996 ‎‡2  LC|no2008040526
996 ‎‡2  NII|DA02447819
996 ‎‡2  NUKAT|n 2017086729
996 ‎‡2  ISNI|0000000100327845
996 ‎‡2  LC|n 2017000463
996 ‎‡2  LC|n 92114297
996 ‎‡2  ISNI|0000000035453609
996 ‎‡2  ISNI|0000000117713144
996 ‎‡2  NII|DA18378318
996 ‎‡2  DNB|1224699246
996 ‎‡2  ISNI|0000000045675790
996 ‎‡2  J9U|987007327500805171
996 ‎‡2  BNE|XX1136147
996 ‎‡2  BNF|12259500
996 ‎‡2  SUDOC|161012388
996 ‎‡2  SUDOC|100531598
996 ‎‡2  NII|DA0660301X
996 ‎‡2  RERO|A003839289
996 ‎‡2  BIBSYS|90336746
996 ‎‡2  ISNI|0000000054722317
996 ‎‡2  ISNI|0000000497015750
996 ‎‡2  ISNI|0000000116952485
996 ‎‡2  ISNI|0000000107956273
996 ‎‡2  LC|nb 99082743
996 ‎‡2  NTA|08751754X
996 ‎‡2  JPG|500055785
996 ‎‡2  J9U|987008729784405171
996 ‎‡2  BIBSYS|5094128
996 ‎‡2  ISNI|0000000031668717
996 ‎‡2  ISNI|0000000463376996
996 ‎‡2  PLWABN|9810536147005606
996 ‎‡2  BIBSYS|1695616271874
996 ‎‡2  RERO|A009017587
996 ‎‡2  BIBSYS|90700123
996 ‎‡2  LC|nb2016001684
996 ‎‡2  NLA|000035062564
996 ‎‡2  NLA|000035703596
996 ‎‡2  BIBSYS|5066746
996 ‎‡2  NUKAT|n 2018127843
996 ‎‡2  ISNI|0000000038841404
996 ‎‡2  LNB|LNC10-000012399
996 ‎‡2  N6I|vtls000096875
996 ‎‡2  LC|n 85139199
996 ‎‡2  BNF|12148772
996 ‎‡2  LC|no2011003199
996 ‎‡2  CAOONL|ncf12096818
996 ‎‡2  ISNI|0000000067507907
996 ‎‡2  SUDOC|244944245
996 ‎‡2  BNF|16717599
996 ‎‡2  DNB|1061852423
996 ‎‡2  SUDOC|085878723
996 ‎‡2  PLWABN|9810623073805606
996 ‎‡2  LC|no2014058456
996 ‎‡2  ISNI|0000000082337010
996 ‎‡2  ISNI|0000000114615741
996 ‎‡2  BNF|13487427
996 ‎‡2  NTA|069970408
996 ‎‡2  LC|n 97033142
996 ‎‡2  NUKAT|n 2020213013
996 ‎‡2  LC|no2009081710
996 ‎‡2  LC|nb2008022428
996 ‎‡2  NKC|vut2012706328
996 ‎‡2  LC|nb2007023233
996 ‎‡2  NSK|000318380
996 ‎‡2  NII|DA08619688
996 ‎‡2  DNB|1070807095
996 ‎‡2  N6I|vtls000073618
996 ‎‡2  RERO|A006084999
996 ‎‡2  ISNI|0000000115111684
996 ‎‡2  J9U|987007421391605171
996 ‎‡2  BIBSYS|98034302
996 ‎‡2  LC|no2019125806
996 ‎‡2  LIH|LNB:C___l_9;=BY
996 ‎‡2  RERO|A028525662
996 ‎‡2  LC|n 94056285
996 ‎‡2  LC|nr 96006601
996 ‎‡2  LC|n 86846415
996 ‎‡2  SUDOC|079004105
996 ‎‡2  DNB|139392424
996 ‎‡2  BNF|13614185
996 ‎‡2  NKC|mzk2015890888
996 ‎‡2  NSK|000547677
996 ‎‡2  LC|nr 98006382
996 ‎‡2  CAOONL|ncf11910680
996 ‎‡2  LC|no2019145479
996 ‎‡2  DNB|1026882664
996 ‎‡2  LC|n 99256472
996 ‎‡2  RERO|A028525163
996 ‎‡2  LC|n 87912952
996 ‎‡2  LC|n 90632401
996 ‎‡2  PLWABN|9810681534805606
996 ‎‡2  LC|nb2003080977
996 ‎‡2  LC|n 82237419
996 ‎‡2  LC|n 82158834
996 ‎‡2  NTA|073503096
996 ‎‡2  RERO|A028525427
996 ‎‡2  LIH|LNB:V-145142;=BD
996 ‎‡2  LC|nb2022011521
996 ‎‡2  SUDOC|086864440
996 ‎‡2  LNB|LNC10-000229654
996 ‎‡2  ISNI|0000000458796304
996 ‎‡2  ISNI|0000000050448541
996 ‎‡2  ISNI|0000000035400996
996 ‎‡2  ISNI|0000000044927546
996 ‎‡2  BNC|981060950311106706
996 ‎‡2  SUDOC|030646316
996 ‎‡2  LC|no2015011509
996 ‎‡2  CAOONL|ncf10313290
996 ‎‡2  J9U|987007318838205171
996 ‎‡2  ISNI|0000000037172763
996 ‎‡2  ERRR|12061827
996 ‎‡2  BNE|XX5568068
996 ‎‡2  NTA|074617303
996 ‎‡2  BNF|14517608
996 ‎‡2  NTA|069516685
996 ‎‡2  DNB|1214200125
996 ‎‡2  SUDOC|18762500X
996 ‎‡2  LC|n 84032384
996 ‎‡2  BIBSYS|4091152
996 ‎‡2  NKC|kup20030000092440
996 ‎‡2  LC|nb2001067967
996 ‎‡2  DNB|1214256686
996 ‎‡2  BIBSYS|4040354
996 ‎‡2  DNB|139979557
996 ‎‡2  RERO|A024726719
996 ‎‡2  NII|DA03795060
996 ‎‡2  CAOONL|ncf11600799
996 ‎‡2  CAOONL|ncf11284426
996 ‎‡2  NII|DA12033958
996 ‎‡2  LNB|LNC10-000112438
996 ‎‡2  LC|no2017108344
996 ‎‡2  ISNI|0000000032130636
996 ‎‡2  ISNI|0000000054896245
996 ‎‡2  RERO|A003839224
996 ‎‡2  RERO|A003839220
996 ‎‡2  J9U|987007378668705171
996 ‎‡2  SUDOC|08596705X
996 ‎‡2  NUKAT|n 2006096143
996 ‎‡2  SUDOC|056528205
996 ‎‡2  LC|n 95050606
996 ‎‡2  LC|no2014092353
996 ‎‡2  NTA|068973896
996 ‎‡2  ISNI|000000007111206X
996 ‎‡2  NLA|000035805834
996 ‎‡2  LC|no2015019556
996 ‎‡2  DNB|1276402538
996 ‎‡2  BNF|12254079
996 ‎‡2  JPG|500091660
996 ‎‡2  LC|nb2001038628
996 ‎‡2  DBC|87097969700195
996 ‎‡2  LC|n 00121585
996 ‎‡2  J9U|987007429249605171
996 ‎‡2  SUDOC|253982154
996 ‎‡2  NII|DA01579257
996 ‎‡2  SIMACOB|30922083
996 ‎‡2  LC|no2018100604
996 ‎‡2  LIH|LNB:CPF_y_;=B_o_
996 ‎‡2  NTA|147810884
996 ‎‡2  RERO|A028525622
996 ‎‡2  CAOONL|ncf11527500
996 ‎‡2  DNB|1026016517
996 ‎‡2  NUKAT|n 2009033916
996 ‎‡2  NUKAT|n 2004078636
996 ‎‡2  ISNI|0000000045437071
996 ‎‡2  LC|nb2009018887
996 ‎‡2  SUDOC|272533858
996 ‎‡2  NTA|191797847
997 ‎‡a  0 0 lived 0 0‏ ‎‡9  1‏