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Hiddo S B

As seen in: arXiv, Oxford Academic
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Articles by Hiddo S B

Astrophysics > Astrophysics of Galaxies

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By Hiddo S B, da Cunha, van der Werf
| arXiv
arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.
Open in Who Shared View Duplicates (15) Issue with article?

Astrophysics > Astrophysics of Galaxies

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By Hiddo S B, Sarah E I
| arXiv
arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.
Open in Who Shared View Duplicates (351) Issue with article?

Astrophysics > Astrophysics of Galaxies

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By Hiddo S B
| arXiv
arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.
Open in Who Shared View Duplicates (641) Issue with article?

Astrophysics > Astrophysics of Galaxies

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By Martinez III, Hiddo S B, Henry Joy
| arXiv
arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.
Open in Who Shared View Duplicates (686) Issue with article?

Accurate simultaneous constraints on the dust mass, temperature, and emissivity index of a galaxy at redshift 7.31

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By De Looze, Sterrenkundig Observatorium, Academia Sinica, Hiddo S B
| Oxford Academic Verified
A thorough understanding of both the formation and properties of cosmic dust at high redshift is crucial for our understanding of the evolution of galaxies as a whole. The presence of dust can be indirectly inferred by observing the attenuated rest-frame UV and optical emission of galaxies, or directly through observing its signature infrared emission (e.g. Galliano, Galametz & Jones 2018).
Open in Who Shared Issue with article?
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