about
An unusually brilliant transient in the galaxy M85.Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission.A massive protocluster of galaxies at a redshift of z ≈ 5.3.Dark matter maps reveal cosmic scaffolding.A Redshift z = 6.56 Galaxy behind the Cluster Abell 370Spectroscopic Confirmation of an Extreme Starburst at Redshift 4.547Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble SequenceKeck/MOSFIRE spectroscopy of z = 7-8 galaxies: Ly{alpha} emission from a galaxy at z = 7.66The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large ArrayCOLDz: KARL G. JANSKY VERY LARGE ARRAY DISCOVERY OF A GAS-RICH GALAXY IN COSMOSA Herschel view of the far-infrared properties of submillimetre galaxieszCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <z< 3 in the COSMOS FieldThe Cosmic Evolution Survey (COSMOS): OverviewCOSMOS: Hubble Space Telescope ObservationsThe Faint‐End Slopes of Galaxy Luminosity Functions in the COSMOS FieldThe Hyper Suprime-Cam SSP Survey: Overview and survey designA Dark Core in Abell 520A study of the dark core in A520 with the Hubble space telescope: the mystery deepensScientific Synergy between LSST and EuclidISM masses and the star formation law at z = 1 to 6: ALMA observations of dust continuum in 145 galaxies in the COSMOS survey fieldA massive, distant proto-cluster at z = 2.47 caught in a phase of rapid formation?A turnover in the galaxy main sequence of star formation at M_*_~ 10^10^ M_{sun}_ for redshifts z < 1.3Are dusty galaxies blue? insights on UV attenuation from dust-selected galaxiesCharacterization of Scuba-2 450 μm and 850 μm selected galaxies in the COSMOS fieldMulti-wavelength SEDs of Herschel-selected galaxies in the COSMOS fieldThe role of galaxy interaction in the SFR-M_*_Relation: characterizing morphological properties of herschel-selected galaxies at 0.2 < z < 1.5Optical Selection of Faint Active Galactic Nuclei in the COSMOS FieldAutomated Selection and Characterization of Emission-Line Sources in Advanced Camera for Surveys Wide Field Camera Grism DataThe evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic surveyStellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z ≃ 3The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-α emitters from z = 2 to z = 6VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster atz~ 3.3Discovery of a rich proto-cluster atz= 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)Discovering extremely compact and metal-poor, star-forming dwarf galaxies out toz~ 0.9 in the VIMOS Ultra-Deep SurveyMass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTAThe dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1Black hole accretion and host galaxies of obscured quasars in XMM-COSMOSThe bimodality of the 10k zCOSMOS-bright galaxies up toz ~ 1: a new statistical and portable classification based on optical galaxy propertiesThe evolution of quiescent galaxies at high redshifts (z≥ 1.4)
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description
astrofysicus
@nl
researcher
@en
հետազոտող
@hy
name
Peter Capak
@ast
Peter Capak
@en
Peter Capak
@es
Peter Capak
@fr
Peter Capak
@nl
type
label
Peter Capak
@ast
Peter Capak
@en
Peter Capak
@es
Peter Capak
@fr
Peter Capak
@nl
prefLabel
Peter Capak
@ast
Peter Capak
@en
Peter Capak
@es
Peter Capak
@fr
Peter Capak
@nl
P1960
gaUTOEwAAAAJ
P21
P31
P496
0000-0003-3578-6843