human | Q5 |
P8880 | AstroGen ID | 8216 |
P9467 | IAU member ID | 10886 |
P269 | IdRef ID | 074043412 |
P2930 | INSPIRE-HEP author ID | A.M.Koekemoer.1 |
P213 | ISNI | 0000000118200770 |
P244 | Library of Congress authority ID | nb2011008413 |
P8189 | National Library of Israel J9U ID | 987007353473405171 |
P1015 | NORAF ID | 6032916 |
P1207 | NUKAT ID | n2003067424 |
P856 | official website | http://www.stsci.edu/~koekemoer/ |
P496 | ORCID iD | 0000-0002-6610-2048 |
P3829 | Publons author ID | 2528417 |
P1053 | ResearcherID | F-8400-2014 |
P1153 | Scopus author ID | 7004490233 |
P214 | VIAF ID | 169213268 |
P10832 | WorldCat Entities ID | E39PCjxvmMCmm7GbtFtfMWCgfC |
P108 | employer | Space Telescope Science Institute | Q1540619 |
P734 | family name | Koekemoer | Q111986678 |
Koekemoer | Q111986678 | ||
Koekemoer | Q111986678 | ||
P735 | given name | Anton | Q5401576 |
Anton | Q5401576 | ||
P1412 | languages spoken, written or signed | English | Q1860 |
P463 | member of | International Astronomical Union | Q6867 |
P106 | occupation | astrophysicist | Q752129 |
researcher | Q1650915 | ||
P21 | sex or gender | male | Q6581097 |
Q58909173 | Q58909173 |
Q58909141 | 3C 236: Radio Source, Interrupted? |
Q58492573 | 3D-HST+CANDELS: the evolution of the galaxy size-mass distribution since z = 3 |
Q58908673 | A CANDELS WFC3 grism study of emission-line galaxies at z ~ 2: a mix of nuclear activity and low-metallicity star formation |
Q58908452 | A CANDELS-3D-HST synergy: resolved star formation patterns at 0.7 < z < 1.5 |
Q58909108 | A Classic Type 2 QSO |
Q56552903 | A LABOCA survey of the extended Chandra deep field South--Submillimeter properties of near-infrared selected galaxies |
Q57602915 | A Lyman break galaxy in the epoch of reionization from Hubble Space Telescope grism spectroscopy |
Q128177105 | A Milky Way-like barred spiral galaxy at a redshift of 3 |
Q58908068 | A New Stellar Atmosphere Grid and Comparisons withHST/STIS CALSPEC Flux Distributions |
Q58474531 | A Possible New Population of Sources with Extreme X-Ray/Optical Ratios |
Q58908918 | A Potential Galaxy Threshing System in the COSMOS Field |
Q57603001 | A Redshiftz≈ 5.4 Lyα Emitting Galaxy with Linear Morphology in the GRAPES/Hubble Ultra Deep Field |
Q111552290 | A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16 |
Q58474465 | A Strong-Lens Survey in AEGIS: The Influence of Large-Scale Structure |
Q58908652 | A TYPE Ia SUPERNOVA AT REDSHIFT 1.55 INHUBBLE SPACE TELESCOPEINFRARED OBSERVATIONS FROM CANDELS |
Q59765545 | A Two-dimensional Spectroscopic Study of Emission-line Galaxies in the Faint Infrared Grism Survey (FIGS). I. Detection Method and Catalog |
Q58908071 | A Very Large (θE≳ 40″) Strong Gravitational Lens Selected with the Sunyaev–Zel’dovich Effect: PLCK G287.0+32.9 (z= 0.38) |
Q58490163 | A WFC3 grism emission line redshift catalog in the GOODS-South field |
Q56502135 | A brightest cluster galaxy with an extremely large flat core |
Q58908275 | A calibration of NICMOS camera 2 for low count rates |
Q58908717 | A critical analysis of the UV luminosity function at redshift ~7 from deep WFC3 data |
Q58490168 | A critical assessment of photometric redshift methods: a CANDELS investigation |
Q58908262 | A critical assessment of stellar mass measurement methods |
Q58908758 | A detailed study of photometric redshifts for GOODS-south galaxies |
Q58908658 | A detection of weak-lensing magnification using galaxy sizes and magnitudes |
Q34379847 | A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51. |
Q58035501 | A group-galaxy cross-correlation function analysis in zCOSMOS |
Q58908231 | A higher efficiency of converting gas to stars pushes galaxies at z ~ 1.6 well above the star-forming main sequence |
Q58035525 | A journey from the outskirts to the cores of groups |
Q58908633 | A link to the past: using Markov chain Monte Carlo fitting to constrain fundamental parameters of high-redshift galaxies |
Q125898132 | A magnified compact galaxy at redshift 9.51 with strong nebular emission lines |
Q34300921 | A magnified young galaxy from about 500 million years after the Big Bang |
Q58908351 | A mass threshold in the number density of passive galaxies at z ~ 2 |
Q58908813 | A multiwavelength study of a sample of 70 {mu}m selected galaxies in the COSMOS field. I. Spectral energy distributions and luminosities |
Q58908769 | A multiwavelength study of a sample of 70 {mu}m selected galaxies in the COSMOS field. II. The role of mergers in galaxy evolution |
Q58908947 | A multiwavelength study of a sample of Texas Radio Survey steep spectrum sources |
Q58908762 | A new extensive catalog of optically variable active galactic nuclei in the GOODS fields and a new statistical approach to variability selection |
Q58908500 | A new multifield determination of the galaxy luminosity function at z = 7–9 incorporating the 2012 Hubble Ultra-Deep Field imaging |
Q56933607 | A panchromatic catalog of early-type galaxies at intermediate redshift in the Hubble Space Telescope Wide Field Camera 3 Early Release Science field |
Q58908474 | A quasar–galaxy mixing diagram: quasar spectral energy distribution shapes in the optical to near-infrared |
Q58489812 | A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images |
Q58908677 | A robust sample of galaxies at redshifts 6.0 |
Q58908782 | A runaway black hole in COSMOS: gravitational wave or slingshot recoil? |
Q58908363 | A study of massive and evolved galaxies at high redshift |
Q58908114 | A study of the relation between star formation and molecular clumps on subparsec scales in 30 Doradus |
Q56555767 | A submillimetre galaxy atz= 4.76 in the LABOCA survey of the ExtendedChandra Deep Field-South |
Q58909191 | A water-vapour giga-maser in the active galaxy TXFS2226 – 184 |
Q58489776 | A weak lensing study of X-ray groups in the COSMOS survey: form and evolution of the mass-luminosity relation |
Q68399866 | A wide-angle tail galaxy at z = 0.53 in the COSMOS field |
Q58908955 | AEGIS: A Panchromatic Study of IRAC-selected Extremely Red Objects with Confirmed Spectroscopic Redshifts |
Q58908958 | AEGIS: Host Galaxy Morphologies of X-Ray-selected and Infrared-selected Active Galactic Nuclei at 0.2 ≤z< 1.2 |
Q58908960 | AEGIS: The Diversity of Bright Near-IR-selected Distant Red Galaxies |
Q58908740 | AEGIS: demographics of X-ray and optically selected active galactic nuclei |
Q58909017 | AGN Host Galaxies atz ~ 0.4-1.3: Bulge-dominated and Lacking Merger-AGN Connection |
Q60021494 | AGN-enhanced outflows of low-ionization gas in star-forming galaxies at 1.7 < z < 4.6* |
Q114818354 | ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z ≃ 0.5 – 6 |
Q58909151 | ASCA observations of the gigahertz-peaked spectrum radio galaxies 1345+125 and 2352+495 |
Q58908724 | Accretion rate and the physical nature of unobscured active galaxies |
Q58908436 | Active galactic nucleus and quasar science with aperture masking interferometry on the james webb space telescope |
Q58908903 | Active galactic nucleus host galaxy morphologies in COSMOS |
Q57602998 | An Overdensity of Galaxies atz= 5.9 + 0.2 in the Hubble Ultra Deep Field Confirmed Using the ACS Grism |
Q58908212 | An increasing stellar baryon fraction in bright galaxies at high redshift |
Q58035671 | An optical group catalog to z = 1 from the zCOSMOS 10 K sample |
Q60021553 | Analogues of primeval galaxies two billion years after the Big Bang |
Q68729254 | Analogues of primeval galaxies two billion years after the Big Bang |
Q69203229 | Analysis of the SFR-M^*^ plane at z < 3: single fitting versus multi-Gaussian decomposition |
Q58908215 | Are compton-thick AGNs the missing link between mergers and black hole growth? |
Q68521846 | AstroWeb. A database of links to astronomy resources. (Announcement of a database) |
Q58489780 | Bars in early- and late-type discs in COSMOS |
Q58908150 | Beyond spheroids and discs: classifications of CANDELS galaxy structure at 1.4 |
Q58908060 | Black Hole Growth Is Mainly Linked to Host-galaxy Stellar Mass Rather Than Star Formation Rate |
Q58035559 | Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS |
Q58908589 | Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey |
Q58908128 | Breaking the curve with CANDELS: a bayesian approach to reveal the non-universality of the dust-attenuation law at high redshift |
Q58908410 | Bulge growth and quenching since z = 2.5 in CANDELS/3D-HST |
Q58908073 | CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip |
Q58908066 | CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies |
Q58908489 | CANDELS multi-wavelength catalogs: source detection and photometry in the GOODS-south field |
Q58908090 | CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS COSMOS Survey Field |
Q58908519 | CANDELS multiwavelength catalogs: source identification and photometry in the CANDELS UKIDSS ultra-deep survey field |
Q58908522 | CANDELS observations of the environmental dependence of the color-mass-morphology relation at z = 1.6 |
Q58492585 | CANDELS observations of the structural properties of cluster galaxies at z = 1.62 |
Q58908225 | CANDELS visual classifications: scheme, data release, and first results |
Q58908394 | CANDELS+3D-HST: compact SFGs at z ~ 2-3, the progenitors of the first quiescent galaxies |
Q58908354 | CANDELS/GOODS-S, CDFS, and ECDFS : photometric redshifts for normal and X-Ray-detected galaxies |
Q59918515 | CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ∼ 2 |
Q58474370 | CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey |
Q58474373 | CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope observations, imaging data products, and mosaics |
Q58908662 | CANDELS: constraining the AGN-merger connection with host morphologies at z ~ 2 |
Q58908624 | CANDELS: correlations of spectral energy distributions and morphologies with star formation status for massive galaxies at z ~ 2 |
Q58908577 | CANDELS: the contribution of the observed galaxy population to cosmic reionization |
Q58908482 | CANDELS: the correlation between galaxy morphology and star formation activity at z ~ 2 |
Q58908592 | CANDELS: the evolution of galaxy rest-frame ultraviolet colors from z = 8 to 4 |
Q58908544 | CANDELS: the progenitors of compact quiescent galaxies at z ~ 2 |
Q58908175 | CLASH-VLT: A highly precise strong lensing model of the galaxy cluster RXC J2248.7−4431 (Abell S1063) and prospects for cosmography |
Q58908265 | CLASH-VLT: Substructure in the galaxy cluster MACS J1206.2-0847 from kinematics of galaxy populations |
Q58474355 | CLASH-VLT: The mass, velocity-anisotropy, and pseudo-phase-space density profiles of thez= 0.44 galaxy cluster MACS J1206.2-0847 |
Q58908357 | CLASH-VLT: The stellar mass function and stellar mass density profile of thez= 0.44 cluster of galaxies MACS J1206.2-0847 |
Q58474349 | CLASH-VLT: constraints on the dark matter equation of state from accurate measurements of galaxy cluster mass profiles |
Q58908140 | CLASH-VLT: dissecting the frontier fields galaxy cluster MACS J0416.1-2403 with ~800 spectra of member galaxies |
Q58908308 | CLASH-VLT: insights on the mass substructures in the frontier fields cluster MACS J0416.1-2403 through accurate strong lens modeling |
Q58922630 | CLASH-VLT: spectroscopic confirmation of a z = 6.11 quintuply lensed galaxy in the Frontier Fields Cluster RXC J2248.7-4431 (Corrigendum) |
Q58474351 | CLASH-VLT: spectroscopic confirmation of az= 6.11 quintuply lensed galaxy in the Frontier Fields cluster RXC J2248.7-4431 |
Q58908161 | CLASH-VLT: testing the nature of gravity with galaxy cluster mass profiles |
Q57686597 | CLASH-x: a comparison of lensing and X-ray techniques for measuring the mass profiles of galaxy clusters |
Q57686866 | CLASH: PRECISE NEW CONSTRAINTS ON THE MASS PROFILE OF THE GALAXY CLUSTER A2261 |
Q57686691 | CLASH: Photometric redshifts with 16 HST bands in galaxy cluster fields |
Q57686608 | CLASH: a census of magnified star-forming galaxies at z ~ 6-8 |
Q59320356 | CLASH: accurate photometric redshifts with 14 HST bands in massive galaxy cluster cores |
Q57686741 | CLASH: complete lensing analysis of the largest cosmic lens MACS J0717.5+3745 and surrounding structures |
Q57686910 | CLASH: discovery of a bright z =~ 6.2 dwarf galaxy quadruply lensed by MACS J0329.6-0211 |
Q57686658 | CLASH: extending galaxy strong lensing to small physical scales with distant sources highly magnified by galaxy cluster members |
Q57686525 | CLASH: extreme emission-line galaxies and their implication on selection of high-redshift galaxies |
Q57686874 | CLASH: mass distribution in and around MACS J1206.2-0847 from a full cluster lensing analysis |
Q58474366 | CLASH: new multiple images constraining the inner mass profile of MACS J1206.2-0847 |
Q57686471 | CLASH: the concentration-mass relation of galaxy clusters |
Q57686835 | CLASH: the enhanced lensing efficiency of the highly elongated merging cluster MACS J0416.1-2403 |
Q56269231 | CLASH: three strongly lensed images of a candidate z {approx} 11 galaxy |
Q57686586 | CLASH: weak-lensing shear-and-magnification analysis of 20 galaxy clusters |
Q57686697 | CLASH: z ∼ 6 young galaxy candidate quintuply lensed by the frontier field cluster RXC J2248.7−4431 |
Q58908637 | COMMISSION 47: COSMOLOGY |
Q58908921 | COSBO: The MAMBO 1.2 Millimeter Imaging Survey of the COSMOS Field |
Q58489815 | COSMOS 5921+0638: characterization and analysis of a new strong gravitationally lensed AGN |
Q58489880 | COSMOS Morphological Classification with the Zurich Estimator of Structural Types (ZEST) and the Evolution Sincez= 1 of the Luminosity Function of Early, Disk, and Irregular Galaxies |
Q112768100 | COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs |
Q56567288 | COSMOS: Hubble Space Telescope Observations |
Q58489879 | COSMOS: Three‐dimensional Weak Lensing and the Growth of Structure |
Q114822128 | Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift? |
Q56547438 | Caught in the act: gas and stellar velocity dispersions in a fast quenching compact star-forming galaxy at z~1.7 |
Q58908494 | Caught in the act: the assembly of massive cluster galaxies at z = 1.62 |
Q58908627 | Chandra high-resolution observations of CID-42, a candidate recoiling supermassive black hole |
Q58909113 | ChandraDeep Field South: The 1 Ms Catalog |
Q110741299 | Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies |
Q59727483 | Characterization of star-forming dwarf galaxies at 0.1 ≲z ≲ 0.9 in VUDS: probing the low-mass end of the mass-metallicity relation |
Q68292620 | Charge transfer efficiency in the WFPC2 CCD arrays |
Q58908901 | Chasing highly obscured QSOs in the COSMOS field |
Q58908976 | Clues to Active Galactic Nucleus Growth from Optically Variable Objects in the Hubble Ultra Deep Field |
Q58908040 | Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3 |
Q58908311 | Clumpy galaxies in CANDELS. I. The definition of UV clumps and the fraction of clumpy galaxies at 0.5 < z < 3 |
Q58908720 | Color and stellar population gradients in passively evolving galaxies at z ~ 2 from HST/WFC3 deep imaging in the Hubble Ultra Deep Field |
Q58908327 | Compton thick AGN in the XMM-COSMOS survey |
Q59764128 | Concurrent Starbursts in Molecular Gas Disks within a Pair of Colliding Galaxies at z = 1.52 |
Q58908458 | Confirmation of small dynamical and stellar masses for extreme emission line galaxies at z ~ 2 |
Q58908477 | Constraining the assembly of normal and compact passively evolving galaxies from redshift z = 3 to the present with CANDELS |
Q58908313 | Constraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members |
Q58908503 | Constraining the luminosity function of faint undetected i-dropout galaxies★ |
Q58909170 | Constraints on Ultraviolet Absorption in the Intracluster Medium of Abell 1030 |
Q58908595 | Constraints on the faint end of the quasar luminosity function at z ~ 5 in the COSMOS field |
Q58908413 | Constraints on the star-formation rate ofz~ 3 LBGs with measured metallicity in the CANDELS GOODS-South field |
Q58908890 | Cosmic evolution of radio selected active galactic nuclei in the cosmos field |
Q58908101 | Cross-correlation between X-ray and optical/near-infrared background intensity fluctuations |
Q57686291 | Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters |
Q58908859 | DEEPSPITZER24 μm COSMOS IMAGING. I. THE EVOLUTION OF LUMINOUS DUSTY GALAXIES—CONFRONTING THE MODELS |
Q58908242 | DISCOVERY OF A STRONG LENSING GALAXY EMBEDDED IN A CLUSTER AT z = 1.62 |
Q58908153 | Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing |
Q55042909 | Dark matter maps reveal cosmic scaffolding. |
Q58908316 | Deconstructing the galaxy stellar mass function with UKIDSS and CANDELS: the impact of colour, structure and environment |
Q56556554 | Deep ATLAS Radio Observations of the Chandra Deep Field?South/SpitzerWide?Area Infrared Extragalactic Field |
Q58908609 | Deep near-infrared spectroscopy of passively evolving galaxies at z >~ 1.4 |
Q58470100 | DeepGALEXImaging of the COSMOSHSTField: A First Look at the Morphology ofz∼ 0.7 Star‐forming Galaxies |
Q59723335 | Demographics of Star-forming Galaxies since z ∼ 2.5. I. The UVJ Diagram in CANDELS |
Q58489819 | Designing future dark energy space missions |
Q58909188 | Detailed Studies of the Lyman Alpha Kinematics in 2104–242 |
Q58908278 | Detailed shape and evolutionary behavior of the X-ray luminosity function of active galactic nuclei |
Q57630553 | Detection of z ∼ 2.3 Cosmic Voids from 3D Lyα Forest Tomography in the COSMOS Field |
Q58908970 | Did galaxy assembly and supermassive black-hole growth go hand-in-hand? |
Q114823421 | Differential attenuation in star-forming galaxies at 0.3 ≲ z ≲ 1.5 in the SHARDS/CANDELS field |
Q58908733 | Differential morphology between rest-frame optical and ultraviolet emission from 1.5 < z < 3 star-forming galaxies |
Q58909130 | Discovery of Ghost Cavities in the X-Ray Atmosphere of Abell 2597 |
Q58908528 | Discovery of Lyman break galaxies at z ~ 7 from the zFourGE survey |
Q58909116 | Discovery of a Star Formation Region in Abell 2052 |
Q21710640 | Discovery of a quadruple lens in CANDELS with a record lens redshift z = 1.53 |
Q21710631 | Discovery of a strong lensing galaxy embedded in a cluster at z = 1.62 |
Q59765551 | Discovery of a z = 7.452 High Equivalent Width Lyα Emitter from the Hubble Space Telescope Faint Infrared Grism Survey |
Q58908249 | Discovery of massive, mostly star formation quenched galaxies with extremely large Ly{alpha} equivalent widths at z ~ 3 |
Q66649439 | Dissecting photometric redshift for active galactic nucleus using XMM- and Chandra-COSMOS samples |
Q58908117 | Do the most massive black holes at z = 2 grow via major mergers? |
Q58908966 | Dominant Nuclear Outflow Driving Mechanisms in Powerful Radio Galaxies |
Q58908178 | Dust properties of Lyman-break galaxies at z ~ 3 |
Q58909181 | Dynamics and Excitation of Radio Galaxy Emission‐Line Regions. I. PKS 2356−61 |
Q56551112 | EMU: Evolutionary Map of the Universe |
Q58908824 | ERRATUM: "Cosmic evolution of radio selected active galactic nuclei in the COSMOS field" (2009, ApJ, 696, 24) |
Q58908882 | ERRATUM: “PHOTOMETRIC PROPERTIES OF Lyα EMITTERS AT z ≈ 4.86 IN THE COSMOS 2 SQUARE DEGREE FIELD” (2009, ApJ, 696, 546) |
Q58908425 | ERRATUM: “THE FMOS-COSMOS SURVEY OF STAR-FORMING GALAXIES AT z ∼ 1.6. I. Hα-BASED STAR FORMATION RATES AND DUST EXTINCTION” (2013, ApJL, 777, L8) |
Q58909020 | Early Spitzer Detections of Extreme X-ray/Optical Sources (EXOs) |
Q58908345 | Early-type galaxies at intermediate redshift observed with Hubble Space Telescope WFC3: perspectives on recent star formation |
Q58908845 | Early-type galaxies in the PEARS survey: probing the stellar populations at moderate redshift |
Q58908131 | Effect of the star formation histories on the SFR-M∗relation at z ≥ 2 |
Q58909084 | Emission Line Properties of GPS/CSS Galaxies |
Q63374837 | Emission-line Metallicities from the Faint Infrared Grism Survey and VLT/MUSE |
Q57602974 | Emission-line galaxies from the PEARS Hubble ultra deep field: a 2D detection method and first results |
Q105653706 | Enabling new science with MAST community contributed data collections |
Q58908829 | Environment of MAMBO galaxies in the COSMOS field |
Q58035474 | Environmental effects in the interaction and merging of galaxies in zCOSMOS |
Q58908872 | Environmental effects on the star formation activity in galaxies at z =~ 1.2 in the COSMOS field |
Q58908799 | Episodic star formation coupled to reignition of radio activity in 3C 236 |
Q60021504 | Erratum: Corrigendum: Analogues of primeval galaxies two billion years after the Big Bang |
Q58908143 | Erratum: Deconstructing the Galaxy stellar mass function with UKIDSS and CANDELS: the impact of colour, structure and environment |
Q58489845 | Erratum: “First Catalog of Strong Lens Candidates in the COSMOS Field” (ApJS, 176, 19 [2008]) |
Q58474493 | Erratum: “The Hubble Higher z Supernova Search: Supernovae to z≈ 1.6 and Constraints on Type Ia Progenitor Models” (ApJ, 613, 200 [2004]) |
Q58908042 | Evidence for Merger-driven Growth in Luminous, High-z, Obscured AGNs in the CANDELS/COSMOS Field |
Q58474496 | Evidence for a Massive Poststarburst Galaxy at z ∼ 6.5 |
Q58492575 | Evidence for a correlation between the sizes of quiescent galaxies and local environment to z ∼ 2 |
Q58908093 | Evidence for reduced specific star formation rates in the centers of massive galaxies at z = 4 |
Q58908416 | Evidence for two modes of black hole accretion in massive galaxies at z∼2 |
Q57630371 | Evolution in the dust lane fraction of edge-on L*_V_ spiral galaxies since z = 0.8 |
Q58908788 | Evolution of blue E/S0 galaxies fromz~ 1: merger remnants or disk-rebuilding galaxies? |
Q58908228 | Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS) |
Q58908181 | Evolution of intrinsic scatter in the SFR-stellar mass correlation at 0.5 < z < 3 |
Q58908238 | Evolution of star-formation properties of high-redshift cluster galaxies since z = 2 |
Q68344320 | Evolution of structural parameters of galaxies in the GOODS-south field |
Q58908924 | Evolution of the Frequency of Luminous (≥LV٭) Close Galaxy Pairs at z < 1.2 in the COSMOS Field |
Q58908331 | Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation |
Q58908423 | Evolution of the fraction of clumpy galaxies at 0.2 < z < 1.0 in the COSMOS field |
Q58908462 | Evolution of the sizes of galaxies over 7 < z < 12 revealed by the 2012 Hubble ultra deep field campaign |
Q58908615 | Extended X-ray emission from non-thermal sources in the COSMOS field: a detailed study of a large radio galaxy atz= 1.168 |
Q58909195 | Extragalactic Ionized Hydrogen in the Fornax Cluster |
Q58908680 | Extreme emission-line galaxies in CANDELS: broadband-selected, starbursting dwarf galaxies at z > 1 |
Q63375961 | FIGS: spectral fitting constraints on the star formation history of massive galaxies since the cosmic noon |
Q58908055 | FIGS—Faint Infrared Grism Survey: Description and Data Reduction |
Q58907769 | Faint AGNs atz>4 in the CANDELS GOODS-S field: looking for contributors to the reionization of the Universe |
Q58908665 | Faint high-redshift AGN in theChandradeep field south: the evolution of the AGN luminosity function and black hole demography |
Q58908669 | Fe K emission from active galaxies in the COSMOS field |
Q58489848 | First Catalog of Strong Lens Candidates in the COSMOS Field |
Q57630552 | First Data Release of the COSMOS Lyα Mapping and Tomography Observations: 3D Lyα Forest Tomography at 2.05 < z < 2.55 |
Q58908195 | First observational support for overlapping reionized bubbles generated by a galaxy overdensity |
Q56547445 | First results from the Faint Infrared Grism Survey (FIGS): first simultaneous detection of Ly{alpha} emission and Lyman break from a galaxy at z = 7.51 |
Q57710886 | GOODS-Herschel and CANDELS: the morphologies of ultraluminous infrared galaxies at z ~ 2 |
Q57710922 | GOODS–Herschel: an infrared main sequence for star-forming galaxies |
Q57603005 | GRAPES, Grism Spectroscopy of the Hubble Ultra Deep Field: Description and Data Reduction |
Q68300335 | GRB 990123 optical observations |
Q54233017 | Galaxies at z = 6-9 from the WFC3/IR imaging of the Hubble Ultra Deep Field |
Q58908683 | Galaxies in X-ray groups. I. Robust membership assignment and the impact of group environments on quenching |
Q56269200 | Galaxy Zoo: CANDELS barred discs and bar fractions |
Q57310904 | Galaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELS |
Q58474357 | Galaxy halo truncation and giant arc surface brightness reconstruction in the cluster MACSJ1206.2-0847 |
Q58489782 | Galaxy stellar mass assembly between 0.2 < z < 2 from the S-COSMOS survey |
Q58908687 | Galaxy structure and mode of star formation in the SFR-mass plane from z ~ 2.5 to z ~ 0.1 |
Q58909163 | H [CSC]i[/CSC] Absorption toward the Nucleus of the Radio Galaxy PKS 2322−123 in A2597 |
Q68300143 | HST wide field and planetary camera II status update |
Q58909043 | HST/STIS Far-UV observations of the central nebulae in the cooling core cluster A 1795 |
Q58909087 | HST/STIS Spectroscopy of CSS Sources: Kinematics and Ionisation of the Aligned Nebulae |
Q57444876 | HST/STIS low dispersion spectroscopy of three Compact Steep Spectrum sources |
Q58786539 | Heavily obscured AGN in star-forming galaxies at z =~ 2 |
Q58909028 | High-Redshift QSOs in the GOODS |
Q58908052 | High-redshift AGN in the Chandra Deep Fields: the obscured fraction and space density of the sub-L* population |
Q58908832 | High-redshift elliptical galaxies: are they (all) really compact? |
Q58908164 | High-resolution spectroscopy of a young, low-metallicity optically thin L = 0.02L* star-forming galaxy at z = 3.12 |
Q69187302 | Host galaxies of luminous z ~ 0.6 quasars: major mergers are not prevalent at the highest AGN luminosities |
Q68346040 | Host galaxy morphologies in the GOODS-south HST ACS images |
Q58908876 | Host galaxy morphologies of X-ray selected AGN: assessing the significance of different black hole fuelling mechanisms to the accretion density of the Universe atz∼ 1 |
Q58908765 | Hot-dust-poor type 1 active galactic nuclei in the COSMOS survey |
Q58909119 | Hubble Space Telescope STIS Observations of the Kinematics of Emission-Line Nebulae in Three Compact Steep-Spectrum Radio Sources |
Q58908033 | Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts z ∼ 2.3–4.1 |
Q57686533 | Hubble Space Telescope combined strong and weak lensing analysis of the CLASH sample: mass and magnification models and systematic uncertainties |
Q58909135 | Hubble Space TelescopeImaging in the Chandra Deep Field–South. I. Multiple Active Galactic Nucleus Populations |
Q58909100 | Hubble Space TelescopeImaging in the Chandra Deep Field–South. II. WFPC2 Observations of an X‐Ray Flux–limited Sample from the 1 Million Second Chandra Catalog |
Q58909076 | Hubble Space TelescopeImaging in theChandraDeep Field–South. III. Quantitative Morphology of the 1 Million SecondChandraCounterparts and Comparison with the Field Population |
Q58909148 | Hubble Space TelescopeObservations of the Associated Absorption‐Line Systems in Q0122+0338 |
Q58909051 | Hubble Space TelescopeSTIS Far‐Ultraviolet Observations of the Central Nebulae in the Cooling‐Core Clusters A1795 and A2597 |
Q58909008 | Hubble Space TelescopeSTIS Spectroscopy of the Lyα Emission Line in the Central Dominant Galaxies in A426, A1795, and A2597: Constraints on Clouds in the Intracluster Medium |
Q58489100 | Hubble Tarantula Treasury Project. III. Photometric catalog and resulting constraints on the progression of star formation in the 30 Doradus region |
Q56601932 | Hubble Tarantula Treasury Project: unraveling Tarantula's Web. I. Observational overview and first results |
Q58908879 | Hubble space Telescope/Advanced camera for surveys morphology of Ly{alpha} emitters at redshift 5.7 in the COSMOS field |
Q56933833 | Hubble space telescope imaging of Ly{alpha} emission at z {approx} 4.4 |
Q58909058 | Identification of Type Ia Supernovae at Redshift 1.3 and Beyond with the Advanced Camera for Surveys on the Hubble Space Telescope |
Q58908807 | Identifications and photometric redshifts of the 2 Ms Chandra Deep Field-South sources |
Q58908810 | Identifying dynamically young galaxy groups via wide-angle tail galaxies: a case study in the COSMOS field at z = 0.53 |
Q58908640 | Identifying luminous active galactic nuclei in deep surveys: revised IRAC selection criteria |
Q58035504 | Improved constraints on the expansion rate of the Universe up toz∼ 1.1 from the spectroscopic evolution of cosmic chronometers |
Q58908201 | Infrared color selection of massive galaxies at z > 3 |
Q58909092 | Interactions between the Abell 2597 central radio source and dense gas in its host galaxy |
Q57686665 | Intracluster light properties in the CLASH-VLT cluster MACS J1206.2-0847 |
Q58035458 | Investigating the relationship between AGN activity and stellar mass in zCOSMOS galaxies at 0 < z < 1 using emission-line diagnostic diagrams |
Q57444878 | Jet–Cloud Interactions in Compact Steep Spectrum Radio Sources |
Q112768091 | Joint Survey Processing. I. Compact Oddballs in the COSMOS Field—Low-luminosity Quasars at z > 6? |
Q58035644 | K+a galaxies in the zCOSMOS survey |
Q56547473 | Keck-I MOSFIRE spectroscopy of compact star-forming galaxies at z >~ 2: high velocity dispersions in progenitors of compact quiescent galaxies |
Q58908342 | Kiloparsec-scale properties of emission-line galaxies |
Q58908121 | Kinematic downsizing at z ~ 2 |
Q57630642 | LYα FOREST TOMOGRAPHY FROM BACKGROUND GALAXIES: THE FIRST MEGAPARSEC-RESOLUTION LARGE-SCALE STRUCTURE MAP AT z > 2 |
Q58908348 | Late-stage galaxy mergers in cosmos to z ~ 1 |
Q112109267 | Limits to Rest-frame Ultraviolet Emission from Far-infrared-luminous z ≃ 6 Quasar Hosts |
Q58908027 | Linking black hole growth with host galaxies: the accretion–stellar mass relation and its cosmic evolution |
Q58909062 | Lower Mass Black Holes in the Great Observatories Origins Deep Survey? Off-nuclear X-Ray Sources |
Q58908558 | Luminous and high stellar mass candidate galaxies at z {approx} 8 discovered in the cosmic assembly near-infrared deep extragalactic legacy survey |
Q58983750 | Lyman continuum escape fraction of faint galaxies at z ~ 3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC |
Q58908926 | Lyα Emitters at Redshift 5.7 in the COSMOS Field |
Q58908049 | MC2: Subaru and Hubble Space Telescope Weak-lensing Analysis of the Double Radio Relic Galaxy Cluster PLCK G287.0+32.9 |
Q58908786 | MOIRCS deep survey. VI. Near-infrared spectroscopy of K-selected star-forming galaxies at z ~ 2 |
Q58908319 | MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063. I. Data products and redshift identifications |
Q58913309 | Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0 |
Q58035604 | Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the schechter function |
Q58908104 | Mass assembly and morphological transformations sincez∼ 3 from CANDELS |
Q58908839 | Massive galaxies in COSMOS: evolution of black hole versus bulge mass but not versus total stellar mass over the last 9 gyr? |
Q58489740 | Measuring the geometry of the universe from weak gravitational lensing behind galaxy groups in the HST COSMOS survey |
Q58908886 | Mid-IR luminosities and UV/Optical star formation rates at z < 1.4 |
Q59827288 | Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3 Gyr after the Big Bang |
Q58908184 | Morphological properties of Ly{alpha} emitters at redshift 4.86 in the cosmos field: clumpy star formation or merger? |
Q58474538 | Morphologies and Spectral Energy Distributions of Extremely Red Galaxies in the GOODS-South Field |
Q58908428 | Morphologies of z ∼ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity |
Q58908981 | Morphology and Evolution of Emission‐Line Galaxies in the Hubble Ultra Deep Field |
Q58908581 | Multi-wavelength view of kiloparsec-scale clumps in star-forming galaxies at z ~ 2 |
Q58908599 | Near-infrared imaging of a z = 6.42 quasar host galaxy with the Hubble space telescope wide field camera 3 |
Q58909132 | New Results from the X‐Ray and Optical Survey of the Chandra Deep Field–South: The 300 Kilosecond Exposure. II |
Q58908532 | New constraints on cosmic reionization from the 2012 Hubble ultra deep field campaign |
Q60021500 | New constraints on the average escape fraction of Lyman continuum radiation in z ~ 4 galaxies from the VIMOS Ultra Deep Survey (VUDS) |
Q58489741 | New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy-galaxy lensing, clustering, and stellar mass functions from z = 0.2 to z =1 |
Q58908486 | New image statistics for detecting disturbed galaxy morphologies at high redshift |
Q58907771 | New observations of z ~ 7 galaxies: evidence for a patchy reionization |
Q58908367 | No more active galactic nuclei in clumpy disks than in smooth galaxies at z ~ 2 in CANDELS/3D-HST |
Q58908188 | Non-parametric analysis of the rest-frame UV sizes and morphological disturbance amongstL*galaxies at 4 |
Q58908603 | Non-redundant Aperture Masking Interferometry (AMI) and segment phasing with JWST-NIRISS |
Q68643297 | Normal galaxies and mergers: the morphological mix of galaxies to z 1 from GOODS ACS imaging of the Chandra Deep Field-South |
Q58035465 | Obscured AGN at z ~ 1 from the zCOSMOS-Bright Survey |
Q58474521 | Obscured Active Galactic Nuclei and the X‐Ray, Optical, and Far‐Infrared Number Counts of Active Galactic Nuclei in the GOODS Fields |
Q58786439 | Obscured GOODS active galactic nuclei and their host galaxies at z < 1.25: the slow black hole growth phase |
Q58908772 | Obscured star formation and environment in the COSMOS field |
Q58908167 | Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the past 10 Gyr |
Q58908888 | Observational limits on type 1 active galactic nucleus accretion rate in COSMOS |
Q58908709 | On star formation rates and star formation histories of galaxies out to z ~ 3 |
Q58908777 | On the Stellar Populations and Evolution of Star-forming Galaxies at 6.3 < z ⩽ 8.6 |
Q58908022 | On the Transition of the Galaxy Quenching Mode at 0.5 < z < 1 in CANDELS |
Q58908896 | On the contribution of large-scale structure to strong gravitational lensing |
Q58035646 | On the cosmic evolution of the scaling relations between black holes and their host galaxies: broad-line active galactic nuclei in the zCOSMOS survey |
Q58907822 | On the detection of ionizing radiation arising from star-forming galaxies at redshift z ~ 3-4: looking for analogs of "stellar re-ionizers" |
Q58489765 | On the evolution of environmental and mass properties of strong lens galaxies in COSMOS |
Q58908750 | On the evolution of the velocity-mass-size relations of disc-dominated galaxies over the past 10 billion years |
Q58035675 | Ongoing and co-evolving star formation in zCOSMOS galaxies hosting active galactic nuclei |
Q60737237 | Optical Line Emission fromz∼ 6.8 Sources with Deep Constraints on LyαVisibility |
Q58908984 | Optical and X-Ray Identification of Faint Radio Sources in the GOODS CDF-S Advanced Camera for Surveys Field |
Q68641621 | Optical properties of all the X-ray sources within the GOODS HST/ACS survey of the Chandra deep field south |
Q58908403 | Optical-faint, far-infrared-bright Herschel sources in the CANDELS fields: ultra-luminous infrared galaxies at z > 1 and the effect of source blending |
Q58474378 | Oxford SWIFT integral field spectrograph and multiwavelength observations of the Eagle galaxy at z= 0.77 |
Q68634994 | PKS 2250-41 and the role of jet cloud interactions in powerful radio galaxies |
Q58909159 | PKS 2250—41 and the role of jet-cloud interactions in powerful radio galaxies |
Q57602999 | Passively Evolving Early‐Type Galaxies at 1.4 ≲z≲ 2.5 in the Hubble Ultra Deep Field |
Q58908170 | Pathways to quiescence: SHARDS view on the star formation histories of massive quiescent galaxies at 1.0 < z < 1.5 |
Q58908419 | PdBI COLD DUST IMAGING OF TWO EXTREMELY REDH– [4.5] > 4 GALAXIES DISCOVERED WITH SEDS AND CANDELS |
Q58909144 | Peering through the Dust: Evidence for a Supermassive Black Hole at the Nucleus of Centaurus A from VLT Infrared Spectroscopy |
Q58474541 | Photometric Redshifts for Galaxies in the GOODS Southern Field |
Q58908892 | Photometric properties of Ly{alpha} emitters at z~4.86 in the COSMOS 2 square degree field |
Q114819404 | Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85 |
Q58908085 | Physical Properties of Sub-galactic Clumps at 0.5 ≤Z≤ 1.5 in the UVUDF |
Q58908643 | Physical properties ofHerschelselected galaxies in a semi-analytic galaxy formation model |
Q58908284 | Physical properties ofz> 4 submillimeter galaxies in the COSMOS field |
Q58908835 | Pixel-based correction for Charge Transfer Inefficiency in the Hubble Space Telescope Advanced Camera for Surveys |
Q58908949 | Populations of candidate black holes at redshift 7 or above |
Q60021819 | Precise strong lensing mass profile of the CLASH galaxy cluster MACS 2129 |
Q58909073 | Prevalence of X‐Ray Variability in the Chandra Deep Field–South |
Q58909032 | Probing the High Redshift Universe with Extreme X-Ray/Optical Sources (EXOs) |
Q58908747 | Probing the faint end of the quasar luminosity function at z~ 4 in the COSMOS field |
Q58908744 | Probing very bright end of galaxy luminosity function at z >~ 7 using Hubble space telescope pure parallel observations |
Q57686819 | Progress in search for high-redshift galaxies magnified by gravitational lensing |
Q58035636 | Properties and environment of radio-emitting galaxies in the VLA-zCOSMOS survey |
Q58908432 | Properties of submillimeter galaxies in the CANDELS GOODS-South field |
Q56659278 | Proto-groups at 1.8 < z < 3 in the zCOSMOS-deep sample |
Q58908952 | Prototype development for a Hubble Legacy Archive |
Q58908018 | Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey |
Q58908208 | Quenching of Star-formation Activity of High-redshift Galaxies in Clusters and Field |
Q58908568 | Quenching star formation at intermediate redshifts: downsizing of the mass flux density in the green valley |
Q58908507 | Quenching star formation at intermediate redshifts: downsizing of the mass flux density in the green valley |
Q58908802 | Radio galaxy feedback in x-ray-selected groups from COSMOS: the effect on the intracluster medium |
Q58908964 | Radio observations of the Chandra Deep Field South. Exploring the possible link between radio emission and star formation in X-ray selected AGN |
Q58908370 | Rapid decline of Ly{alpha} emission toward the reionization era |
Q58908058 | Recovering the Properties of High-redshift Galaxies with Different JWST Broadband Filters |
Q57602987 | Redshifts of Emission-Line Objects in the Hubble Ultra Deep Field |
Q58908076 | Relations between the Sizes of Galaxies and Their Dark Matter Halos at Redshifts 0 |
Q58909122 | Resolving the Hard X-Ray Background in the Chandra Deep Field South |
Q58909036 | Resolving the Shocks in Radio Galaxy Nebulae:Hubble Space Telescopeand Radio Imaging of 3C 171, 3C 277.3, and PKS 2250-41 |
Q58908648 | Rest-frame UV-optically selected galaxies at 2.3 <~ z <~ 3.5: searching for dusty star-forming and passively evolving galaxies |
Q58908268 | S-CANDELS: the Spitzer-Cosmic Assembly Near-infrared Deep Extragalactic Survey. Survey design, photometry, and deep IRAC source counts |
Q58908536 | SEDS: the Spitzer Extended Deep Survey. Survey design, photometry, and deep IRAC source counts |
Q58908235 | SHARDS: a global view of the star formation activity at z ~ 0.84 and z ~ 1.23 |
Q58908909 | Science with an 8-meter to 16-meter optical/UV space telescope |
Q58908694 | Secular evolution and a non-evolving black-hole-to-galaxy mass ratio in the last 7 gyr |
Q58908987 | Seeing the Sky throughHubble’s Eye: The COSMOS SkyWalker |
Q58908082 | Separating galaxies from the cluster dark matter halo in Abell 611 |
Q58908525 | Serendipitous discovery of a massive cD galaxy at z = 1.096: implications for the early formation and late evolution of cD galaxies |
Q58909095 | Shock ionization of line-emitting gas in the radio galaxy PKS 0349−27 |
Q58908931 | Simulating the Cosmos: The Fraction of Merging Galaxies at High Redshift |
Q58908133 | Size evolution of star-forming galaxies with 2 < z < 4.5 in the VIMOS Ultra-Deep Survey |
Q58908618 | Smooth(er) stellar mass maps in CANDELS: constraints on the longevity of clumps in high-redshift star-forming galaxies |
Q58908555 | Space Telescopes in the Ultraviolet, Optical, and Infrared (UV/O/IR) |
Q68518796 | Spectral energy distributions of X-ray selected sources in the GOODS field: revealing highly-obscured AGN |
Q58908444 | Spectral energy distributions of type 1 AGN in XMM-COSMOS – II. Shape evolution |
Q58908571 | Spectral energy distributions of type 1 active galactic nuclei in the COSMOS survey. I. The XMM-COSMOS sample |
Q58908030 | Spectrophotometric Redshifts in the Faint Infrared Grism Survey: Finding Overdensities of Faint Galaxies |
Q58908727 | Spectropolarimetric evidence for radiatively inefficient accretion in an optically dull active galaxy |
Q58908893 | Spectroscopic confirmation of faint Lyman break galaxies near redshift five in the Hubble Ultra Deep Field |
Q58489769 | Spectroscopy of luminous z > 7 galaxy candidates and sources of contamination in z > 7 galaxy searches |
Q58908848 | Spitzer 70 and 160 {mu}m observations of the COSMOS field |
Q58035439 | Spot the difference |
Q58489833 | Star formation and dust obscuration at z {approx} 2: galaxies at the dawn of downsizing |
Q58908272 | Star formation and quenching among the most massive galaxies at z ∼ 1.7 |
Q58908281 | Star-forming blue ETGs in two newly discovered galaxy overdensities in the HUDF at z=1.84 and 1.9: unveiling the progenitors of passive ETGs in cluster cores |
Q59713055 | Starburst to Quiescent from HST/ALMA: Stars and Dust Unveil Minor Mergers in Submillimeter Galaxies at z ∼ 4.5 |
Q58474512 | Stars in the Hubble Ultra Deep Field |
Q58908862 | Stellar and total baryon mass fractions in groups and clusters since redshift 1 |
Q58035342 | Stellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z ≃ 3 |
Q58908156 | Stellar mass-gas-phase metallicity relation at 0.5 <= z <= 0.7: a power law with increasing scatter toward the low-mass regime |
Q58490164 | Stellar masses from the CANDELS survey: the GOODS-South and UDS fields |
Q56933582 | Stellar populations of Lyman break galaxies at z =~ 1-3 in the HST/WFC3 early release science observations |
Q58492578 | Structural evolution of early-type galaxies to z = 2.5 in CANDELS |
Q58492583 | Structural parameters of galaxies in CANDELS |
Q68319358 | Structure and evolution of disk galaxies in the GOODS fields |
Q58470063 | Studying large- and small-scale environments of ultraviolet luminous galaxies |
Q68302790 | Supermassive black holes in obscured nuclei: the case of Centaurus A |
Q66361878 | Supernova 1998ff in anonymous galaxy |
Q66362418 | Supernovae 2002ez, 2002fv, 2002fw, 2002fx, 2002fy, 2002fz, 2002ga |
Q58908929 | S‐COSMOS: The Spitzer Legacy Survey of the Hubble Space Telescope ACS 2 deg2 COSMOS Field I: Survey Strategy and First Analysis |
Q58035617 | THE 10k zCOSMOS: MORPHOLOGICAL TRANSFORMATION OF GALAXIES IN THE GROUP ENVIRONMENT SINCEz∼1 |
Q58035658 | THE zCOSMOS 10k-BRIGHT SPECTROSCOPIC SAMPLE |
Q58035511 | THE zCOSMOS 20k GROUP CATALOG |
Q58908406 | TYPE Ia SUPERNOVA RATE MEASUREMENTS TO REDSHIFT 2.5 FROM CANDELS: SEARCHING FOR PROMPT EXPLOSIONS IN THE EARLY UNIVERSE |
Q58908439 | TYPE-Ia SUPERNOVA RATES TO REDSHIFT 2.4 FROM CLASH: THE CLUSTER LENSING AND SUPERNOVA SURVEY WITH HUBBLE |
Q58908465 | The 2012 Hubble ultra deep field (UDF12): observational overview |
Q114150775 | The NuSTAR extragalactic survey of the James Webb Space Telescope North Ecliptic Pole time-domain field |
Q58785781 | The ALMA Frontier Fields Survey |
Q58909226 | The ALMA Frontier Fields Survey |
Q112770147 | The ALPINE-ALMA [CII] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements |
Q112768181 | The ALPINE-ALMA [CII] Survey: [CII] 158 μ m Emission Line Luminosity Functions at z ∼ 4–6 |
Q112768240 | The ALPINE-ALMA [CII] survey |
Q112770100 | The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties |
Q112767949 | The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z ∼ 4.4–5.8 |
Q112767925 | The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe |
Q112767851 | The ALPINE-ALMA [CII] survey: Investigation of 10 galaxies at z ∼ 4.5 with [OII] and [CII] line emission − ISM properties and [OII]−SFR relation |
Q112768200 | The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]–SFR relation over the last 13 Gyr |
Q112768212 | The ALPINE-ALMA [CII] survey: Molecular gas budget in the early Universe as traced by [CII] |
Q110205432 | The ALPINE-ALMA [CII] survey: Obscured star formation rate density and main sequence of star-forming galaxies at z > 4 |
Q112768253 | The ALPINE-ALMA [CII] survey: Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6 |
Q108871517 | The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z ∼ 5 |
Q112767973 | The ALPINE-ALMA [CII] survey: The nature, luminosity function, and star formation history of dusty galaxies up to z ≃ 6 |
Q114818306 | The ALPINE–ALMA [C ii] Survey: The Infrared–Radio Correlation and Active Galactic Nucleus Fraction of Star-forming Galaxies at z ∼ 4.4–5.9 |
Q112768000 | The ALPINE–ALMA [CII] survey: Luminosity function of serendipitous [CII] line emitters at z ∼ 5 |
Q112771665 | The ALPINE−ALMA [C ii ] Survey: on the nature of an extremely obscured serendipitous galaxy |
Q58474368 | The Advanced Camera for Surveys General Catalog: structural parameters for approximately half a million galaxies |
Q56556383 | The All-Wavelength Extended Groth Strip International Survey (AEGIS) Data Sets |
Q58908933 | The Angular Correlations of Galaxies in the COSMOS Field |
Q58909001 | The COSMOS 2-degree HST/ACS survey |
Q58489894 | The COSMOS Survey: Hubble Space Telescope Advanced Camera for Surveys Observations and Data Processing |
Q58489794 | The COSMOS-WIRCam near-infrared imaging survey. I. BzK-selected passive and star-forming galaxy candidates at z {>~} 1.4 |
Q58908146 | The COSMOS2015 catalog: exploring the 1 < z < 6 universe with half a million galaxies |
Q59767184 | The Chandra COSMOS Legacy Survey: Compton thick AGN at high redshift |
Q58908865 | The Chandra COSMOS survey. I. Overview and point source catalog |
Q58908612 | The Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sources |
Q56551834 | The Chandra Deep Field-South survey: 4 Ms source catalogs |
Q58908095 | The Chandra Deep Field-South survey: 7 Ms source catalogs |
Q58909104 | The Chandra Deep Field–South: The 1 Million Second Exposure |
Q58909013 | The Chandra deep field South/GOODS survey |
Q68305486 | The Chandra deep field south |
Q58908842 | The Chandra survey of the COSMOS field. II. Source detection and photometry |
Q58908869 | The Clowes-Campusano Large Quasar Group Survey. I. GALEX selected sample of Lyman break galaxies at z ~ 1 |
Q57686901 | The Cluster Lensing And Supernova survey with Hubble: an overview |
Q58489901 | The Cosmic Evolution Survey (COSMOS): A Large‐Scale Structure atz = 0.73 and the Relation of Galaxy Morphologies to Local Environment |
Q58908935 | The Cosmic Evolution Survey (COSMOS): The Morphological Content and Environmental Dependence of the Galaxy Color‐Magnitude Relation atz∼ 0.7 |
Q58908937 | The Effects of Environment on Morphological Evolution at 0 < z < 1.2 in the COSMOS Survey |
Q58908912 | The Evolution of AGN Host Galaxies: From Blue to Red and the Influence of Large‐Scale Structures |
Q58909054 | The Evolution of Disk Galaxies in the GOODS-South Field: Number Densities and Size Distribution |
Q107559636 | The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years |
Q58489903 | The Evolution of the Number Density of Large Disk Galaxies in COSMOS |
Q58909157 | The Extended Blue Continuum and Line Emission around the Central Radio Galaxy in Abell 2597 |
Q58786469 | The Extended Chandra Deep Field-South survey: optical spectroscopy of faint X-ray sources with the VLT and Keck |
Q58909005 | The ExtendedChandraDeep Field–South Survey:ChandraPoint‐Source Catalogs |
Q58908469 | The FMOS-COSMOS survey of star-forming galaxies at z ~ 1.6. I. H{alpha}-based star formation rates and dust extinction |
Q58908386 | The FMOS-COSMOS survey of star-forming galaxies at z ~ 1.6. II. The mass-metallicity relation and the dependence on star formation rate and dust extinction |
Q58908245 | The FMOS-COSMOS survey of star-forming galaxies at z~1.6. III. Survey design, performance, and sample characteristics |
Q58489905 | The First Release COSMOS Optical and Near‐IR Data and Catalog |
Q58908078 | The Frontier Fields: Survey Design and Initial Results |
Q58908852 | The Future of Direct Supermassive Black Hole Mass Estimates |
Q68358664 | The GOODS AGN population and the X-ray background |
Q68359022 | The GOODS on obscured AGN |
Q58909065 | The Great Observatories Origins Deep Survey: Initial Results from Optical and Near-Infrared Imaging |
Q58908373 | The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts |
Q58908297 | The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day |
Q58474523 | The Hubble Higher z Supernova Search: Supernovae to z≈ 1.6 and Constraints on Type Ia Progenitor Models |
Q58474387 | The Hubble Space Telescope GOODS NICMOS Survey: overview and the evolution of massive galaxies at 1.5 < z < 3 |
Q56933885 | The Hubble Space Telescope Wide Field Camera 3 Early Release Science data: panchromatic faint object counts for 0.2-2 {mu}m wavelength |
Q55893552 | The Hubble Ultra Deep Field |
Q68639256 | The Hubble ultra deep field |
Q58908037 | The Intrinsic Characteristics of Galaxies on the SFR–M ∗ Plane at 1.2 < z < 4: I. The Correlation between Stellar Age, Central Density, and Position Relative to the Main Sequence |
Q55950624 | The Isophotal Structure of Star-forming Galaxies at 0.5 < z < 1.8 in CANDELS: Implications for the Evolution of Galaxy Structure |
Q113693161 | The JWST Early Release Observations |
Q56554511 | The LABOCA survey of the Extended Chandra Deep Field South: two modes of star formation in active galactic nucleus hosts? |
Q56555921 | The Large Apex BOlometer Camera survey of the Extended Chandra Deep Field South |
Q58908063 | The Lyman Continuum Escape Fraction of Emission Line-selected z ∼ 2.5 Galaxies Is Less Than 15% |
Q58908204 | The Lyman continuum escape fraction of galaxies at z = 3.3 in the VUDS-LBC/COSMOS field |
Q57686572 | The MUSIC of CLASH: predictions on the concentration-mass relation |
Q58911734 | The Molecular Gas Content and Fuel Efficiency of Starbursts at z ∼ 1.6 with ALMA |
Q58908510 | The Morphologies of Massive Galaxies at 1 |
Q58909068 | The Nature of Near-Ultraviolet-selected Objects in the Chandra Deep Field-South |
Q58909040 | The Nature of UV-Selected Galaxies in the CDFS |
Q58909184 | The Nearest GHz Peaked-Spectrum Radio Galaxy, PKS 1718-649 |
Q59782677 | The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters |
Q58908997 | The Properties and Redshift Evolution of Intermediate-Luminosity Off-Nuclear X-Ray Sources in the Chandra Deep Fields |
Q58489906 | The Redshift Evolution of Early‐Type Galaxies in COSMOS: Do Massive Early‐Type Galaxies Form by Dry Mergers? |
Q58908015 | The SFR–M * Correlation Extends to Low Mass at High Redshift |
Q58786774 | The Space Density of High-Redshift QSOs in the Great Observatories Origins Deep Survey |
Q58489909 | The Stellar Content of the COSMOS Field as Derived from Morphological and SED‐based Star/Galaxy Separation |
Q58474491 | The Structure and Star Formation History of Early‐Type Galaxies in the Ultra Deep Field/GRAPES Survey |
Q58908914 | The UDF05 Follow‐up of the Hubble Ultra Deep Field. I. The Faint‐End Slope of the Lyman Break Galaxy Population atz∼ 5 |
Q58908906 | The UDF05 follow-up of the Hubble Ultra Deep Field. II. Constraints on reionization from z-dropout galaxies |
Q58908713 | The UDF05 follow-up of the Hubble Ultra Deep Field. III. The luminosity function at z ~ 6 |
Q58908540 | The UV Luminosity Function of Star-forming Galaxies via Dropout Selection at Redshifts z ~ 7 and 8 from the 2012 Ultra Deep Field Campaign |
Q58908513 | The UV continua and inferred stellar populations of galaxies at z ≃ 7-9 revealed by the Hubble Ultra-Deep Field 2012 campaign |
Q58908389 | The UV continuum of z > 1 star-forming galaxies in the Hubble ultraviolet UltraDeep field |
Q58922627 | The VANDELS ESO public spectroscopic survey |
Q114822184 | The VANDELS survey: dust attenuation in star-forming galaxies at z = 3-4 |
Q60021493 | The VIMOS Ultra Deep Survey |
Q60021496 | The VIMOS Ultra Deep Survey |
Q58922662 | The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to zspec ~ 6 in CANDELS |
Q58908172 | The VIMOS Ultra Deep Survey: Lyαemission and stellar populations of star-forming galaxies at 2 < z < 2.5 |
Q58035356 | The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-α emitters from z = 2 to z = 6 |
Q60021495 | The VIMOS Ultra-Deep Survey: A major merger origin for the high fraction of galaxies at 2 < z < 6 with two bright clumps |
Q68943274 | The VIMOS Ultra-Deep Survey: Emerging from the dark, a massive proto-cluster at z ~ 4.57 |
Q58909046 | The VLA-COSMOS Survey. I. Radio Identifications from the Pilot Project |
Q58908816 | The VLA-COSMOS perspective on the infrared-radio relation. I. New constraints on selection biases and the non-evolution of the Infrared/Radio properties of star-forming and active galactic nucleus galaxies at intermediate and high redshift |
Q58908793 | The VLA-COSMOS survey. IV. Deep data and joint catalog |
Q58908940 | The VLA‐COSMOS Survey. II. Source Catalog of the Large Project |
Q58908991 | The WFPC2 Archival Pure Parallels Project |
Q58908994 | The X-Ray-to-Optical Properties of Optically Selected Active Galaxies over Wide Luminosity and Redshift Ranges |
Q58035632 | The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS |
Q58035625 | The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei |
Q58908898 | The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue |
Q58908945 | The [Oii] λ3727 Luminosity Function and Star Formation Rate atz ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field |
Q58035639 | The [O iii] emission line luminosity function of optically selected type-2 AGN from zCOSMOS$^{\rm,}$ |
Q56211259 | The abundance of star-forming galaxies in the redshift range 8.5-12: new results from the 2012 Hubble ultra deep field campaign |
Q58908548 | The ages, masses and star formation rates of spectroscopically confirmed z ∼ 6 galaxies in CANDELS |
Q58035562 | The bimodality of the 10k zCOSMOS-bright galaxies up toz ~ 1: a new statistical and portable classification based on optical galaxy properties |
Q58907824 | The blue UV slopes ofz ~ 4 Lyman break galaxies: implications for the corrected star formation rate density |
Q58786386 | The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey |
Q58489801 | The buildup of the Hubble sequence in the cosmos field |
Q58908376 | The bulge–disc decomposed evolution of massive galaxies at 1 < z < 3 in CANDELS |
Q58908754 | The bulk of the black hole growth since z ~ 1 occurs in a secular universe: no Major Merger-AGN connection |
Q58908097 | The bursty star formation histories of low-mass galaxies at 0.4 < z < 1 revealed by star formation rates measured from H{beta} and FUV |
Q58474376 | The cluster lensing and supernova survey with Hubble (CLASH): strong-lensing analysis of A383 from 16-band HST/WFC3/ACS imaging |
Q58035470 | The colors of central and satellite galaxies in zCOSMOS out to z =~ 0.8 and implications for quenching |
Q58908421 | The colour distribution of galaxies at redshift five |
Q58786120 | The composite nature of Dust-Obscured Galaxies (DOGs) atz ∼ 2–3 in the COSMOS field – I. A far-infrared view |
Q57686755 | The contribution of halos with different mass ratios to the overall growth of cluster-sized halos |
Q58908302 | The cosmic growth of the active black hole population at 1 |
Q58908379 | The decomposed bulge and disc size–mass relations of massive galaxies at 1 < z < 3 in CANDELS |
Q58908111 | The deepest X-ray view of high-redshift galaxies: constraints on low-rate black hole accretion |
Q58035647 | The density field of the 10k zCOSMOS galaxies |
Q58035367 | The dependence of galactic outflows on the properties and orientation of zCOSMOS galaxies at z ~ 1 |
Q58908562 | The dependence of quenching upon the inner structure of galaxies at 0.5 <= z < 0.8 in the DEEP2/AEGIS survey |
Q58035681 | The dependence of star formation activity on stellar mass surface density and sersic index in zCOSMOS galaxies at 0.5 < z < 0.9 compared with SDSS galaxies at 0.04 < z < 0.08 |
Q58908198 | The detection and statistics of giant arcs behind CLASH clusters |
Q57602468 | The discovery of the most distant known type Ia supernova at redshift 1.914 |
Q58908382 | The distribution of satellites around massive galaxies at 1 < z < 3 in ZFOURGE/CANDELS: dependence on star formation activity |
Q58035492 | The dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1 |
Q68755901 | The dust and molecular gas in the brightest cluster galaxy in MACS 1931.8-2635 |
Q58908796 | The effects of an active galactic nucleus on host galaxy colour and morphology measurements |
Q58035683 | The environments of active galactic nuclei within the zCOSMOS density field |
Q58908107 | The evolution of star formation histories of quiescent galaxies |
Q68650580 | The evolution of the UV luminosity function of star-forming galaxies at 2.5 |
Q56547458 | The evolution of the galaxy rest-frame ultraviolet luminosity function over the first two billion years |
Q58908821 | The evolution of the hard X-ray luminosity function of AGN |
Q58908655 | The evolving slope of the stellar mass function at 0.6 ≤ z< 4.5 from deep WFC3 data |
Q58035331 | The evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic survey |
Q58922653 | The extended epoch of galaxy formation: Age dating of ~3600 galaxies with 2 < z < 6.5 in the VIMOS Ultra-Deep Survey |
Q58908305 | The galaxy stellar mass function at 3.5 ≤ z ≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields |
Q58908339 | The host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS |
Q58908012 | The host galaxies of luminous type 2 AGN at z ∼0.3-0.4 |
Q58908099 | The impact of JWST broadband filter choice on photometric redshift estimation |
Q58035544 | The impact of galaxy interactions on active galactic nucleus activity in zCOSMOS |
Q58786228 | The incidence of obscuration in active galactic nuclei |
Q58908218 | The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 |
Q58908324 | The interstellar medium and feedback in the progenitors of the compact passive galaxies at z ~ 2 |
Q58908737 | The majority of compact massive galaxies at z ~ 2 are disk dominated |
Q58908360 | The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field |
Q58908192 | The morphologies and alignments of gas, mass, and the central galaxies of CLASH clusters of galaxies |
Q58908565 | The morphologies of massive galaxies at 1 |
Q58474408 | The morphology of passively evolving galaxies at z ~ 2 from Hubble space Telescope/WFC3 deep imaging in the Hubble ultra deep field |
Q58908397 | The nature of extreme emission line galaxies at z = 1-2: kinematics and metallicities from near-infrared spectroscopy |
Q58908630 | The nature of extremely red H - [4.5] > 4 galaxies revealed with SEDS and CANDELS |
Q58908855 | The nature of optically dull active galactic nuclei in COSMOS |
Q58035571 | The nonlinear biasing of the zCOSMOS galaxies up to z ~ 1 from the 10k sample |
Q58489804 | The opacity of galactic disks at z ~ 0.7 |
Q58035653 | The optical spectra of Spitzer 24 {mu}m galaxies in the cosmic evolution survey field. II. Faint infrared sources in the zCOSMOS-bright 10k catalog |
Q58908697 | The population of high-redshift active galactic nuclei in the Chandra-COSMOS survey |
Q58908448 | The progenitors of the compact early-type galaxies at high redshift |
Q59620198 | The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS |
Q58908221 | The projected gravitational potential of the galaxy cluster MACS J1206 derived from galaxy kinematics |
Q58908516 | The properties of (sub-)millimetre-selected galaxies as revealed by CANDELS HST WFC3/IR imaging in GOODS-South |
Q58908254 | The quasar-LBG two-point angular cross-correlation function at z~4 in the COSMOS field |
Q58035548 | The radial and azimuthal profiles of Mg II absorption around 0.5 < z < 0.9 zCOSMOS galaxies of different colors, masses, and environments |
Q58908497 | The redshift and mass dependence on the formation of the Hubble sequence at z > 1 from CANDELS/UDS |
Q58489772 | The redshift and nature of AzTEC/COSMOS 1: a starburst galaxy at z = 4.6 |
Q58908046 | The relationship between galaxy and dark matter halo size from z ∼ 3 to the present |
Q58908088 | The relationship between star formation activity and galaxy structural properties in CANDELS and a semi-analytic model |
Q58908690 | The relative abundance of compact and normal massive early-type galaxies and its evolution from redshift z ~ 2 to the present |
Q58908400 | The rest-frame ultraviolet structure of 0.5 < z < 1.5 galaxies |
Q58908780 | The rise and fall of passive disk galaxies: morphological evolution along the red sequence revealed by COSMOS |
Q58908289 | The role of bulge formation in the homogenization of stellar populations at z~2 as revealed by internal color dispersion in CANDELS |
Q58035534 | The role of galaxy interaction in environmental dependence of the star formation activity at z =~ 1.2 |
Q58908391 | The role of major mergers in the size growth of intermediate-mass spheroids |
Q114823366 | The size and pervasiveness of Ly α–UV spatial offsets in star-forming galaxies at z ∼ 6 |
Q56933737 | The size evolution of passive galaxies: observations from the Wide-Field Camera 3 Early Release Science program |
Q58908574 | The size-luminosity relation at z = 7 in CANDELS and its implication on reionization |
Q58908584 | The spectral energy distributions, host galaxies and environments of variability-selected active galactic nuclei in GOODS-South |
Q58908730 | The star formation history of mass-selected galaxies in the COSMOS field |
Q58908136 | The star formation rate efficiency of neutral atomic-dominated hydrogen gas in the outskirts of star-forming galaxies from z ~ 1 to z ~3 |
Q58908335 | The stellar initial mass function at 0.9 < z < 1.5 |
Q58908972 | The supermassive black hole in Centaurus A: a benchmark for gas kinematical measurements |
Q58908701 | The tumultuous formation of the Hubble sequence at z > 1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep Field |
Q58909079 | The ultra-deep 20 cm Australia telescope survey of the Chandra Deep Field South |
Q58035588 | The zCOSMOS 10k-sample: the role of galaxy stellar mass in the colour-density relation up toz ~ 1 |
Q58035406 | The zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8 |
Q58035648 | The zCOSMOS redshift survey: how group environment alters global downsizing trends |
Q58035667 | The zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1 |
Q58035661 | The zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at $z=0.2$–1 |
Q58035656 | The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types |
Q58035574 | The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z≃ 1 |
Q56556106 | TheChandraDeep Field–South Survey: 2 Ms Source Catalogs |
Q58908942 | TheXMM‐NewtonWide‐Field Survey in the COSMOS Field. IV. X‐Ray Spectral Properties of Active Galactic Nuclei |
Q58489899 | TheXMM‐NewtonWide‐Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies |
Q57686673 | Three gravitationally lensed supernovae behind CLASH galaxy clusters |
Q58197051 | To stack or not to stack: spectral energy distribution properties of ly{alpha}-emitting galaxies at z = 2.1 |
Q68642362 | Toward a multi-wavelenght geometric distortion solution for WFPC2 |
Q58909271 | Tracing the accretion history of supermassive black holes through X-ray variability: results from the ChandraDeep Field-South |
Q58908125 | Tracing the reionization epoch with ALMA: [C II] emission in z ~ 7 galaxies |
Q58035589 | Tracking the impact of environment on the galaxy stellar mass function up toz ~ 1 in the 10 k zCOSMOS sample |
Q58908705 | Two fossil groups of galaxies at z≈ 0.4 in the Cosmic Evolution Survey: accelerated stellar-mass build-up, different progenitors |
Q56934063 | UV-dropout galaxies in the Goods-South field from WFC3 Early Release Science observations |
Q59762395 | UVUDF: UV Luminosity Functions at the Cosmic High Noon |
Q58908455 | UVUDF: Ultraviolet Imaging of the Hubble Ultra Deep Field with Wide-Field Camera 3 |
Q58908258 | UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field |
Q58035630 | Ultraluminous X-ray sources out to z ~ 0.3 in the COSMOS field |
Q36059307 | Ultraviolet luminosity density of the universe during the epoch of reionization |
Q57686501 | Ultraviolet morphology and unobscured UV star formation rates of CLASH brightest cluster galaxies |
Q58909127 | UltravioletHubble Space TelescopeSnapshot Survey of 3CR Radio Source Counterparts at Low Redshift |
Q58035594 | Understanding the shape of the galaxy two-point correlation function at z ≃ 1 in the COSMOS field |
Q58909153 | Unveiling the Active Nucleus of Centaurus A |
Q58908025 | Unveiling the Dynamical State of Massive Clusters through the ICL Fraction |
Q68636520 | V4334 Sagittarii |
Q58910610 | VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 |
Q62622330 | VLT/FORS2 view at z ~ 6: Lyman-α emitter fraction and galaxy physical properties at the edge of the epoch of cosmic reionization |
Q59766635 | Variability-selected Low-luminosity Active Galactic Nuclei Candidates in the 7 Ms Chandra Deep Field-South |
Q58489912 | Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements |
Q58908471 | Weak lensing calibrated M-T scaling relation of galaxy groups in the COSMOS field^{sstarf}^ |
Q58908621 | What turns galaxies off? the different morphologies of star-forming and quiescent galaxies since z ~ 2 from CANDELS |
Q58035522 | X-Ray Groups of Galaxies at 0.5 1 in zCOSMOS: Increased AGN Activities in High Redshift Groups |
Q58474514 | X-Ray Properties of Lyman Break Galaxies in the Great Observatories Origins Deep Survey |
Q58909234 | X-Ray Spectral Analyses of AGNs from the 7Ms Chandra Deep Field-South Survey: The Distribution, Variability, and Evolutions of AGN Obscuration |
Q58908552 | X-ray selected AGN host galaxies are similar to inactive galaxies out to z = 3: results from CANDELS/CDF-s |
Q58909167 | X‐Ray Properties of B2 1028+313: A Quasar at the Center of the Abell Cluster A1030 |
Q58908292 | ZFOURGE/CANDELS: on the evolution of M* galaxy progenitors from z = 3 to 0.5 |
Q58035597 | zCOSMOS 10k-bright spectroscopic sample |
Q58035425 | zCOSMOS 20k: satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z ∼ 0.7 |
Q58035602 | zCOSMOS – 10k-bright spectroscopic sample |
Q56556487 | zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 |