Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA

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Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA

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im Jahr 2017 veröffentlichter wissenschaftlicher Artikel

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wetenschappelijk artikel

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наукова стаття, опублікована у 2017

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Tracing the Evolution of Dust ...... Reionisation Epoch with SPICA

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Tracing the Evolution of Dust ...... Reionisation Epoch with SPICA

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Tracing the Evolution of Dust ...... Reionisation Epoch with SPICA

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Tracing the Evolution of Dust ...... Reionisation Epoch with SPICA

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Tracing the Evolution of Dust ...... Reionisation Epoch with SPICA

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Tracing the Evolution of Dust ...... Reionisation Epoch with SPICA

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P1476

Tracing the Evolution of Dust ...... Reionisation Epoch with SPICA

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P2093

A. Efstathiou

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A. Papadopoulos

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C. Pearson

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C. Vignali

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D. Scott

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D.L. Clements

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E. Egami

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E. González-Alfonso

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E. Hatziminaoglou

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F. Fontanot

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P2860

A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34.

Energy input from quasars regulates the growth and activity of black holes and their host galaxies.

Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission.

A massive protocluster of galaxies at a redshift of z ≈ 5.3.

High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey

Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies

Observations of the Hubble Deep Field with the Infrared Space Observatory - V. Spectral energy distributions, starburst models and star formation history

An Observational Determination of the Bolometric Quasar Luminosity Function

TheHerschel-SPIRE instrument and its in-flight performance

The Photodetector Array Camera and Spectrometer (PACS) on the HerschelSpace Observatory

P31

scholarly article

P356

10.1017/PASA.2017.49

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P478

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Mattia Vaccari

Luigi Spinoglio

Maarten Baes

Vassilis Charmandaris

P577

2017-01-01T00:00:00Z

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P818

1710.02353

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