about
The Spatially Resolved Dust-to-metals Ratio in M101SMASH: Survey of the MAgellanic Stellar HistoryThe Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE): The Dust Extinction Curve from Red Clump StarsA New Approach to Convective Core Overshooting: Probabilistic Constraints from Color–Magnitude Diagrams of LMC ClustersPanchromatic Hubble Andromeda Treasury. XVIII. The High-mass Truncation of the Star Cluster Mass FunctionDDO 216-A1: A Central Globular Cluster in a Low-luminosity Transition-type GalaxyPanchromatic Hubble Andromeda treasury. XVI. Star cluster formation efficiency and the clustered fraction of young starsPanchromatic Hubble Andromeda treasury. XIV. The period-age relationship of cepheid variables in M31 star clustersThe high-mass stellar initial mass function in M31 clustersPHAT stellar cluster survey. II. Andromeda project cluster catalogThe panchromatic Hubble Andromeda treasury. V. Ages and masses of the year 1 stellar clustersThe Panchromatic Hubble Andromeda Treasury. IV. A probabilistic approach to inferring the high-mass stellar initial mass function and other power-law functionsThe 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 treasuryModeling the effects of star formation histories on h{alpha} and ultraviolet fluxes in nearby dwarf galaxiesThe wyoming survey for h{alpha}. II. H{alpha} luminosity functions at z ~~ 0.16, 0.24, 0.32, and 0.40The Wyoming survey for H{alpha}. I. Initial results at z ~ 0.16 and 0.24SMASHing the LMC: A Tidally Induced Warp in the Outer LMC and a Large-scale Reddening MapSMASHing the LMC: Mapping a Ring-like Stellar Overdensity in the LMC Disk
P50
Q57524248-870B1208-41DB-4392-A8DD-3645A2FF41D4Q57524251-77759DC7-FD39-4078-8D71-BBE7D3DDE96EQ57524253-BCC4AF32-80DB-4548-B402-09ECD8A66B3DQ57524256-407087BE-D6D0-47F8-801C-C0C2268852FEQ57524257-4753D948-FEA9-46D0-940C-1E08D4BC0EB9Q57524258-E19957EE-012D-482D-B062-499A8B2990B2Q57524262-AD2D42F0-36C6-4683-9E3F-269046B626AEQ57524266-1A105706-6569-469D-84EA-1821E0C00A5AQ57524268-6A3822FF-6793-46A8-998B-AB2BF911ACECQ57524271-67F4616A-527A-44DC-B258-8F4E10D55C2EQ57524276-F1A2C7FD-3437-42AA-9F15-27A2A0A16FD7Q57524283-E9CAD086-2F0E-4658-8845-36B1228658DEQ57524286-EB567021-FF91-440C-8C8A-0CF6B14F55E6Q57524287-C2C7D0FF-CF64-4AAE-B847-5125A3BD0779Q57524291-806AA1A2-5534-4F90-A3E0-DADDCAF97602Q57524293-C3655A08-E60D-4B06-A2F5-9DC508FB1444Q57524295-4995E0B8-4F8B-41EC-9F14-F4E7B4C745E3Q57524297-9A2DD665-CD1E-4752-878C-885F9C08444BQ57524299-1AA47DAB-EB66-419C-976D-78704D7AD839Q57524313-46B6B0AC-1012-4EC6-9CD8-F4979E5BF032Q57524323-EA676CBF-45C4-4F6E-94B0-8EA236BAA213Q59822128-BBDF64FC-567E-4540-945A-DF33FD3BA97EQ60368238-CF5D2770-EF09-4231-976D-2E272F05291E
P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
Lent Johnson
@ast
Lent Johnson
@en
Lent Johnson
@es
Lent Johnson
@nl
type
label
Lent Johnson
@ast
Lent Johnson
@en
Lent Johnson
@es
Lent Johnson
@nl
altLabel
Cliff Johnson
@en
Clifton Johnson
@en
L.C. Johnson
@en
prefLabel
Lent Johnson
@ast
Lent Johnson
@en
Lent Johnson
@es
Lent Johnson
@nl
P244
P106
P214
65146936621813780605
P244
no2016086303
P31
P496
0000-0001-6421-0953
P734
P7859
lccn-no2016086303