hsim: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT

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Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph

P2860

Q56817989-D2D06250-0784-45FB-92D5-F1E4A790D0B0

P2860

hsim: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT

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http://www.wikidata.org/entity/Q56818019

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im September 2015 veröffentlichter wissenschaftlicher Artikel

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wetenschappelijk artikel

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наукова стаття, опублікована у вересні 2015

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hsim: a simulation pipeline fo ...... ectrograph on the European ELT

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hsim: a simulation pipeline fo ...... ectrograph on the European ELT

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hsim: a simulation pipeline fo ...... ectrograph on the European ELT

@en

hsim: a simulation pipeline fo ...... ectrograph on the European ELT

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hsim: a simulation pipeline fo ...... ectrograph on the European ELT

@en

hsim: a simulation pipeline fo ...... ectrograph on the European ELT

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P1476

hsim: a simulation pipeline fo ...... ectrograph on the European ELT

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P2093

F. Clarke

http://www.w3.org/2001/XMLSchema#string

M. Tecza

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N. Thatte

http://www.w3.org/2001/XMLSchema#string

R. C. W. Houghton

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S. Zieleniewski

http://www.w3.org/2001/XMLSchema#string

T. Fusco

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P2860

Galactic Stellar and Substellar Initial Mass Function

The Global Schmidt Law in Star‐forming Galaxies

Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4

Hubble Space TelescopeHα imaging of star-forming galaxies atz≃ 1–1.5: evolution in the size and luminosity of giant H iiregions

The properties of the star-forming interstellar medium at z = 0.8-2.2 from HiZELS: star formation and clump scaling laws in gas-rich, turbulent disks

The properties of the star-forming interstellar medium atz = 0.84-2.23 from HiZELS: mapping the internal dynamics and metallicity gradients in high-redshift disc galaxies

Astropy: A community Python package for astronomy

GOALS: The Great Observatories All-Sky LIRG Survey

The SINS survey: SINFONI integral field spectroscopy of z ~ 2 star-forming galaxies

The rapid formation of a large rotating disk galaxy three billion years after the Big Bang

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3754–3765

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scholarly article

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10.1093/MNRAS/STV1860

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English

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http://www.w3.org/2001/XMLSchema#string

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453

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A. M. Swinbank

Sarah Kendrew

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2015-09-10T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

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1508.04441

http://www.w3.org/2001/XMLSchema#string

P819

2015MNRAS.453.3754Z

http://www.w3.org/2001/XMLSchema#string

hsim: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT

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P2860

P2860

hsim: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT

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name

type

label

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P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819

P356

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819