Michele Trenti
0000-0001-9391-305X
133 papers found
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LOWER-LUMINOSITY GALAXIES COULD REIONIZE THE UNIVERSE: VERY STEEP FAINT-END SLOPES TO THEUVLUMINOSITY FUNCTIONS ATz⩾ 5-8 FROM THE HUDF09 WFC3/IR OBSERVATIONS
GAMMA-RAY BURST HOST GALAXY SURVEYS AT REDSHIFTz≳ 4: PROBES OF STAR FORMATION RATE AND COSMIC REIONIZATION
CRITICAL STAR FORMATION RATES FOR REIONIZATION: FULL REIONIZATION OCCURS AT REDSHIFTz≈ 7
INFERENCES ON THE DISTRIBUTION OF Lyα EMISSION OFz∼ 7 ANDz∼ 8 GALAXIES
OVERDENSITIES OFY-DROPOUT GALAXIES FROM THE BRIGHTEST-OF-REIONIZING GALAXIES SURVEY: A CANDIDATE PROTOCLUSTER AT REDSHIFTz≈ 8
EXPANDED SEARCH FORz∼ 10 GALAXIES FROM HUDF09, ERS, AND CANDELS DATA: EVIDENCE FOR ACCELERATED EVOLUTION ATz> 8?
The Brightest of Reionizing Galaxies (BoRG) survey
ACTIVE AND PASSIVE GALAXIES ATz∼ 2: REST-FRAME OPTICAL MORPHOLOGIES WITH WFC3
The UDF05 FOLLOW-UP OF THE HUBBLE ULTRA DEEP FIELD. III. THE LUMINOSITY FUNCTION ATz∼ 6
GALAXY FORMATION IN HEAVILY OVERDENSE REGIONS ATz∼ 10: THE PREVALENCE OF DISKS IN MASSIVE HALOS
ULTRAVIOLET LUMINOSITY FUNCTIONS FROM 132z∼ 7 ANDz∼ 8 LYMAN-BREAK GALAXIES IN THE ULTRA-DEEP HUDF09 AND WIDE-AREA EARLY RELEASE SCIENCE WFC3/IR OBSERVATIONS
The Dark Side of Qso Formation at High Redshifts
MORPHOLOGICAL EVOLUTION OF GALAXIES FROM ULTRA-DEEPHUBBLE SPACE TELESCOPEWIDE FIELD CAMERA 3 IMAGING: THE HUBBLE SEQUENCE ATz∼ 2
The Brightest of Reionizing Galaxies Survey: Design and Preliminary Results
A candidate redshift z ≈ 10 galaxy and rapid changes in that population at an age of 500 Myr
The EVOLUTION OF THE ULTRAVIOLET LUMINOSITY FUNCTION FROMz∼ 0.75 TOz∼ 2.5 USINGHSTERS WFC3/UVIS OBSERVATIONS
Galaxy sets distance mark
Widespread Presence of Shallow Cusps in the Surface-Brightness Profile of Globular Clusters
The Clustering Properties of the First Galaxies
CONFIRMATION OF THE COMPACTNESS OF Az= 1.91 QUIESCENT GALAXY WITHHUBBLE SPACE TELESCOPE’S WIDE FIELD CAMERA 3
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