about
sameAs
CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy SurveyCANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope observations, imaging data products, and mosaicsThe Hubble Space Telescope GOODS NICMOS Survey: overview and the evolution of massive galaxies at 1.5 < z < 3Erratum: “The Hubble Higher z Supernova Search: Supernovae to z≈ 1.6 and Constraints on Type Ia Progenitor Models” (ApJ, 613, 200 [2004])The Hubble Higher z Supernova Search: Supernovae to z≈ 1.6 and Constraints on Type Ia Progenitor ModelsColor-selected Galaxies at z ≈ 6 in the Great Observatories Origins Deep SurveyThe Rest-Frame Ultraviolet Luminosity Density of Star-forming Galaxies at Redshifts z > 3.5The Size Evolution of High-Redshift GalaxiesBar Evolution over the Last 8 Billion Years: A Constant Fraction of Strong Bars in the GEMS SurveyEvolution and Impact of Bars over the Last Nine Gyr: Early Results from GEMSClumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3Physical Properties of Sub-galactic Clumps at 0.5 ≤Z≤ 1.5 in the UVUDFThe bursty star formation histories of low-mass galaxies at 0.4 < z < 1 revealed by star formation rates measured from H{beta} and FUVUVUDF: ultraviolet through near-infrared catalog and photometric redshifts of galaxies in the Hubble Ultra Deep FieldClumpy galaxies in CANDELS. I. The definition of UV clumps and the fraction of clumpy galaxies at 0.5 < z < 3The interstellar medium and feedback in the progenitors of the compact passive galaxies at z ~ 2The rest-frame ultraviolet structure of 0.5 < z < 1.5 galaxiesThe progenitors of the compact early-type galaxies at high redshiftUVUDF: ultraviolet imaging of the Hubble Ultra Deep Field with Wide-Field Camera 3The tumultuous formation of the Hubble sequence at z > 1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep FieldBL Lac identification for the ultraluminous X-ray source observed in the direction of NGC 4698AGN Host Galaxies atz ~ 0.4-1.3: Bulge-dominated and Lacking Merger-AGN ConnectionThe Evolution of Disk Galaxies in the GOODS-South Field: Number Densities and Size DistributionLower Mass Black Holes in the Great Observatories Origins Deep Survey? Off-nuclear X-Ray SourcesThe Great Observatories Origins Deep Survey: Initial Results from Optical and Near-Infrared ImagingMultiwavelength Study of Massive Galaxies at z ∼ 2. II. Widespread Compton‐thick Active Galactic Nuclei and the Concurrent Growth of Black Holes and BulgesThe Morphological Diversities among Star‐forming Galaxies at High Redshifts in the Great Observatories Origins Deep SurveyVigorous Star Formation with Low Efficiency in Massive Disk Galaxies at z = 1.5Pandeia: a multi-mission exposure time calculator for JWST and WFIRSTPhotoionization models for the semi-forbidden C III] 1909 emission in star-forming galaxiesWide-Field Slitless Spectroscopy with JWST's NIRISSA multiwavelength study of tadpole galaxies in the Hubble ultra deep fieldThe rate of core collapse supernovae to redshift 2.5 from the CANDELS and CLASH supernova surveysUpdated point spread function simulations for JWST with WebbPSFDOTIFS: a new multi-IFU optical spectrograph for the 3.6-m Devasthal optical telescopeMid-infrared and X-ray luminosity correlations of X-ray point sources in NGC 1399Generation of a Near Infra-Red Guide Star Catalog for Thirty-Meter Telescope ObservationsThe bivariate size-luminosity relations for Lyman break galaxies at z ~ 4-5Hα survey of nearby dwarf galaxiesFilamentary infall of cold gas and escape of Lyα and hydrogen ionizing radiation from an interacting high-redshift galaxy★
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description
onderzoeker
@nl
researcher ORCID ID = 0000-0002-5269-6527
@en
name
Swara Ravindranath
@ast
Swara Ravindranath
@en
Swara Ravindranath
@es
Swara Ravindranath
@nl
type
label
Swara Ravindranath
@ast
Swara Ravindranath
@en
Swara Ravindranath
@es
Swara Ravindranath
@nl
prefLabel
Swara Ravindranath
@ast
Swara Ravindranath
@en
Swara Ravindranath
@es
Swara Ravindranath
@nl
P106
P21
P31
P496
0000-0002-5269-6527