about
The densest galaxyTwo stellar-mass black holes in the globular cluster M22.A supermassive black hole in an ultra-compact dwarf galaxy.A deeper look at Leo IV: star formation history and extended structureDetection of Supermassive Black Holes in Two Virgo Ultracompact Dwarf GalaxiesThe star formation history and extended structure of the Hercules Milky Way satelliteTidal signatures in the faintest Milky Way satellites: the detailed properties of Leo V, Pisces II, and Canes venatici IIThe NGC 404 nucleus: star cluster and possible intermediate-mass black holeDetection of Enhanced Central Mass-to-light Ratios in Low-mass Early-type Galaxies: Evidence for Black Holes?The ACS nearby galaxy survey treasuryThe MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular ClustersA radio-selected black hole X-ray binary candidate in the Milky Way globular cluster M62No evidence for intermediate-mass black holes in globular clusters: strong constraints from the JVLAPanchromatic Hubble Andromeda Treasury. XVIII. The High-mass Truncation of the Star Cluster Mass FunctionPanchromatic Hubble Andromeda treasury. XVI. Star cluster formation efficiency and the clustered fraction of young starsPanchromatic Hubble Andromeda treasury. XII. Mapping stellar metallicity distributions in M31The high-mass stellar initial mass function in M31 clustersThe panchromatic Hubble Andromeda treasury. XI. The spatially resolved recent star formation history of M31PHAT stellar cluster survey. II. Andromeda project cluster catalogThe Panchromatic Hubble Andromeda Treasury. X. Ultraviolet to infrared photometry of 117 million equidistant starsThe panchromatic Hubble Andromeda treasury. V. Ages and masses of the year 1 stellar clustersThe panchromatic Hubble Andromeda treasury. III. Measuring ages and masses of partially resolved stellar clustersM31 Planetary nebulae as seen by the Panchromatic Hubble Andromeda TreasuryThe panchromatic Hubble Andromeda treasury. I. Bright UV stars in the bulge of M31PHAT stellar cluster survey. I. Year 1 catalog and integrated photometryThe ACS nearby galaxy survey treasury. X. Quantifying the star cluster formation efficiency of nearby dwarf galaxiesThe panchromatic Hubble Andromeda treasuryThe history of star formation in galaxy disks in the local volume as measured by the Advanced Camera for Surveys Nearby Galaxy Survey TreasuryThe Assembly History of the Milky Way Nuclear Star ClusterKMOS view of the Galactic centre. I. Young stars are centrally concentratedLarge scale kinematics and dynamical modelling of the Milky Way nuclear star clusterThe Milky Way nuclear star cluster beyond 1 pcThe SPLASH survey: kinematics of Andromeda's inner spheroidThe panchromatic Hubble Andromeda treasury. VIII. A wide-area, high-resolution map of dust extinction in M31Tracing the metal-poor M31 stellar halo with blue horizontal branch starsThe panchromatic Hubble Andromeda treasury. II. Tracing the inner M31 halo with blue horizontal branch starsM94 as a Unique Testbed for Black Hole Mass Estimates and AGN Activity at Low LuminositiesThe M81 group dwarf irregular galaxy DDO 165. I. High-velocity neutral gas in a post-starburst systemThe M81 group dwarf irregular galaxy DDO 165. II. Connecting recent star formation with interstellar medium structures and kinematicsThe HST/ACS Coma Cluster Survey – X. Nuclear star clusters in low-mass early-type galaxies: scaling relations
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description
researcher, ORCID id # 0000-0003-0248-5470
@en
wetenschapper
@nl
name
Anil Seth
@ast
Anil Seth
@en
Anil Seth
@es
Anil Seth
@nl
type
label
Anil Seth
@ast
Anil Seth
@en
Anil Seth
@es
Anil Seth
@nl
prefLabel
Anil Seth
@ast
Anil Seth
@en
Anil Seth
@es
Anil Seth
@nl
P106
P1412
P21
P31
P496
0000-0003-0248-5470