What determines the shape of the local (z < 0.1) infrared galaxy luminosity function?

Author:

Symeonidis M1,Page M J1

Affiliation:

1. Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. On the dust properties of the UV galaxies in the redshift range z ∼ 0.6–1.2;Monthly Notices of the Royal Astronomical Society;2024-01-12

2. The star formation rates of QSOs;Monthly Notices of the Royal Astronomical Society;2022-05-18

3. A Flexible Method for Estimating Luminosity Functions via Kernel Density Estimation. II. Generalization and Python Implementation;The Astrophysical Journal Supplement Series;2022-05-01

4. AGN and star formation across cosmic time;Monthly Notices of the Royal Astronomical Society;2021-03-03

5. Subaru/HSC deep optical imaging of infrared sources in the AKARI North Ecliptic Pole-Wide field;Monthly Notices of the Royal Astronomical Society;2020-10-20

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