Daniel Weisz astrophysicien américain
Weisz, Dan
VIAF ID: 8591159400279019620008 (Personal)
Permalink: http://viaf.org/viaf/8591159400279019620008
Preferred Forms
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100 0 _
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Daniel Weisz
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astrophysicien américain
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100 1 _
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Weisz, Dan
4xx's: Alternate Name Forms (6)
5xx's: Related Names (2)
Works
| Title | Sources |
|---|---|
| The ACS LCID project: on the origin of dwarf galaxy types--A manifestation of the halo assembly bias? |
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| The ACS nearby galaxy survey treasury. II. Young stars and their relation to h{alpha} and UV emission timescales in the M81 outer disk |
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| The ACS nearby galaxy survey treasury. IX. Constraining asymptotic giant branch evolution with old metal-poor galaxies |
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| The ACS nearby galaxy survey treasury. X. Quantifying the star cluster formation efficiency of nearby dwarf galaxies |
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| AHUBBLE SPACE TELESCOPESTUDY OF THE ENIGMATIC MILKY WAY HALO GLOBULAR CLUSTER CRATER |
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| Chemistry and kinematics of the late-forming dwarf irregular galaxies Leo A, Aquarius, and Sagittarius DIG |
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| A clear age-velocity dispersion correlation in Andromeda's stellar disk |
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| Comparing Chandra and Hubble in the Northern Disk of M31 |
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| Comparing the ancient star formation histories of the Magellanic Clouds★ |
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| Comparison of H{alpha} and UV star formation rates in the local volume: systematic discrepancies for dwarf galaxies |
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| A Complete Census of Luminous Stellar Variability on Day to Decade Timescales |
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| DDO 216-A1: A Central Globular Cluster in a Low-luminosity Transition-type Galaxy |
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| Discovery and characterization of 3000+ main-sequence binaries from APOGEE spectra |
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| DOES STELLAR FEEDBACK CREATE H I HOLES? AHUBBLE SPACE TELESCOPE/VERY LARGE ARRAY STUDY OF HOLMBERG II |
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| An Empirical Measurement of the Initial–Final Mass Relation with Gaia White Dwarfs |
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| fire in the field: simulating the threshold of galaxy formation |
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| The formation and hierarchical assembly of globular cluster populations |
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| The formation of kiloparsec-scale H I holes in dwarf galaxies |
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| Gas kinematics in FIRE simulated galaxies compared to spatially unresolved H i observations |
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| Gas kinematics, morphology and angular momentum in the FIRE simulations |
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| A global star-forming episode in M31 2-4 Gyr ago |
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| The high-mass stellar initial mass function in M31 clusters |
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| The history of star formation in galaxy disks in the local volume as measured by the Advanced Camera for Surveys Nearby Galaxy Survey Treasury |
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| HST/ACS direct ages of the dwarf elliptical galaxies NGC 147 and NGC 185 |
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| HSTIMAGING OF THE LOCAL VOLUME DWARF GALAXIES PISCES A AND B: PROTOTYPES FOR LOCAL GROUP DWARFS |
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| The Hubble Space Telescope Survey of M31 Satellite Galaxies. I. RR Lyrae–based Distances and Refined 3D Geometric Structure |
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| The impact of pre-supernova feedback and its dependence on environment |
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| The ISLANDS project. I. Andromeda XVI, an extremely low mass galaxy not quenched by reionization |
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| The ISLAnds Project. III. Variable Stars in Six Andromeda Dwarf Spheroidal Galaxies |
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| Leo A: A Late-blooming Survivor of the Epoch of Reionization in the Local Group |
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| The Local Group as a time machine: studying the high-redshift Universe with nearby galaxies |
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| The Local Group: the ultimate deep field |
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| The M81 group dwarf irregular galaxy DDO 165. I. High-velocity neutral gas in a post-starburst system |
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| The M81 group dwarf irregular galaxy DDO 165. II. Connecting recent star formation with interstellar medium structures and kinematics |
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| Measuring galaxy star formation rates from integrated photometry: insights from color-magnitude diagrams of resolved stars |
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| Metallicity Distribution Function of the Eridanus II Ultra-faint Dwarf Galaxy from Hubble Space Telescope Narrowband Imaging |
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| Modeling the effects of star formation histories on h{alpha} and ultraviolet fluxes in nearby dwarf galaxies |
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| A New Approach to Convective Core Overshooting: Probabilistic Constraints from Color–Magnitude Diagrams of LMC Clusters |
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| No assembly required: mergers are mostly irrelevant for the growth of low-mass dwarf galaxies |
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| The panchromatic Hubble Andromeda treasury. VIII. A wide-area, high-resolution map of dust extinction in M31 |
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| The Panchromatic Hubble Andromeda Treasury. X. Ultraviolet to infrared photometry of 117 million equidistant stars |
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| THE PANCHROMATICHUBBLEANDROMEDA TREASURY. XI. THE SPATIALLY RESOLVED RECENT STAR FORMATION HISTORY OF M31 |
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| PHAT stellar cluster survey. II. Andromeda project cluster catalog |
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| Push it to the limit: Local Group constraints on high-redshift stellar mass functions forM⋆≥ 105 M⊙ |
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| Rapid environmental quenching of satellite dwarf galaxies in the Local Group |
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| A rogues gallery of Andromeda’s dwarf galaxies – II. Precise distances to 17 faint satellites |
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| Science with the Ultraviolet Explorer (UVEX) |
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| Signatures of unresolved binaries in stellar spectra: implications for spectral fitting |
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| The Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE): The Dust Extinction Curve from Red Clump Stars |
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| A spectroscopic and photometric exploration of the C/M ratio in the disk of M31 |
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| The star formation histories of local group dwarf galaxies. II. Searching for signatures of reionization |
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| THE STAR FORMATION HISTORY OF LEO T FROMHUBBLE SPACE TELESCOPEIMAGING |
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| The statistical challenge of constraining the low-mass IMF in Local Group dwarf galaxies |
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| Stellar clusterings around "isolated" massive YSOs in the LMC |
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| The supernova progenitor mass distributions of M31 and M33: further evidence for an upper mass limit |
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| Testing density wave theory with resolved stellar populations around spiral arms in M81 |
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| Timescales on which star formation affects the neutral interstellar medium |
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| Triggered star formation and the creation of the supergiant H I shell in IC 2574 |
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| The very faint end of the UV luminosity function over cosmic time: constraints from the Local Group fossil record |
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| Where are the most ancient stars in the Milky Way? |
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