Ruprecht-Karls-Universität Heidelberg

Astronomisches Rechen-Institut

Address:

Astronomisches Rechen-Institut
Mönchhofstr. 12-14
69120 Heidelberg
Germany
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The Astronomisches Rechen-Institut (ARI) is part of the newly established Centre for Astronomy of Heidelberg University (Zentrum für Astronomie der Universität Heidelberg or ZAH). The other two institutes in the ZAH are the Institute for Theoretical Astrophysics (Institut für Theoretische Astrophysik or ITA) and the State Observatory Königstuhl (Landessternwarte Königstuhl or LSW).

The scientific activities at the ARI cover a broad range of research areas including cosmology, gravitational lensing, galaxy evolution, star clusters, stellar astrophysics, the interstellar medium, astrometry, satellite missions, and calendrical calculations.

The ARI is involved in various national and international scientific networks and collaborations.  The institute plays a leading role in supporting the Gaia satellite mission of the European Space Agency and participates in the ground-based spectroscopic and photometric SDSS, 4MOST, and LSST surveys.

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Next Astro colloquia
Oct 02
11:00
TBD
Duncan Christie (MPIA)
Königstuhl Kolloquium
Max-Planck-Institut für Astronomie, Level 3 Lecture Hall (301)
Oct 15
11:15
A graveyard of disrupted globular clusters in the Milky Way’s stellar halo
Sarah Kane (Cambridge University)
ARI Institute Colloquium
ARI, Moenchhofstrasse 12-14, Seminarraum 1.OG
Oct 16
11:00
TBA
TBA (TBA)
Königstuhl Kolloquium
Max-Planck-Institut für Astronomie, Level 3 Lecture Hall (301)

More colloquia

Recent ZAH publications
8/2026
Annibali, F.; Ferguson, A. M. N. et al. (inc. Zinchenko, I. A.)
Euclid: Early Release Observations - The extended stellar component of the IC10 dwarf galaxy
A&A 712, A175(2026)

8/2026
Rosu, S.; Sciarini, L. et al. (inc. Josiek, J.)
The beauty of k2: Probing stellar interiors using apsidal motion: I. The benchmark massive binary HD 152248
A&A 712, A42(2026)

9/2026
Budi, Bakuh Danang Setyo; Aoki, Wako et al. (inc. Matsuno, Tadafumi)
Revealing α-element's Past with Subaru/IRD: Oxygen Abundance of 35 Very Metal-poor Stars from Near-IR OH Lines
ApJ 1008, 75(2026)


More publications