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Oliver Krause

Researcher at Max Planck Society

Publications -  165
Citations -  14831

Oliver Krause is an academic researcher from Max Planck Society. The author has contributed to research in topics: Star formation & Galaxy. The author has an hindex of 48, co-authored 162 publications receiving 13695 citations. Previous affiliations of Oliver Krause include University of Arizona.

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NIP - The Near Infrared Imaging Photometer for Euclid

TL;DR: The Euclid Imaging Consortium (EIC) as mentioned in this paper performed a near infrared imaging photometer for the Euclid space mission in the context of ESA's 2015 Cosmic Vision program, where the NIP channel was used to determine the photometric redshifts of over 2 billion galaxies collected over a wide survey area of 20 000 deg 2.
Posted Content

Bringing high spatial resolution to the Far-infrared -- A giant leap for astrophysics

TL;DR: In this paper, the authors trace the role of water in proto-planetary disks, to advance our understanding of the planet formation process and, intimately related to that, the pathways to habitable planets and the emergence of life.
Journal ArticleDOI

The molecular hydrogen explorer H2EX

F. Boulanger, +77 more
TL;DR: The Molecular Hydrogen Explorer (H2EX) as mentioned in this paper was designed to observe the first rotational lines of the H2 molecule (28.2, 17.0, 12.3 and 9.7 μm) over a wide field, and at high spectral resolution.
Journal ArticleDOI

The ISOPHOT 170 ${\mathsf \mu}$m Serendipity Survey - IV. The far-infrared sky atlas

TL;DR: In this article, a sky atlas with ≈ 15% sky coverage in the hitherto unobserved far-infrared wavelength band around 170 μ m was assembled to further increase the scientific utilization of the strip scanning measurements of the ISOPHOT Serendipity Survey (ISOSS).
Proceedings ArticleDOI

Development of a Si:As blocked impurity band detector for far IR detection

TL;DR: In this article, a linear array of blocked impurity band (BIB) far infrared detectors and the related Cryogenic Readout Electronics (CRE) were fabricated for the study of exoplanets by means of null interferometry.