Steward Observatory

to reduce this thermal distortion by improvements in the panel design

Steward Observatory, Dietmar Scheulen, William F. Hoffmann, 2017 .

PypeIt: The Python Spectroscopic Data Reduction Pipeline

Steward Observatory, University of Arizona, J. Xavier Prochaska, 2019, J. Open Source Softw..

than the shortest wavelength in order to assure a diffraction limited beam and hence a good overall efficiency.

Steward Observatory, 2017 .

The architecture of the LkCa 15 transitional disk revealed by high-contrast imaging⋆

National Astronomical Observatory of Japan, Steward Observatory, Tucson, 2014, 1402.1766.

Accretion Disk Evolution with Wind Infall. II. Results of Three-dimensional Hydrodynamical Simulations with an Illustrative Application to Sagittarius A*

Steward Observatory, Max-Planck-Institut fur Radioastronomie, Fulvio Melia, 1999 .

“TNOs are Cool”: a survey of the trans-Neptunian region - VII. Size and surface characteristics of (90377) Sedna and 2010 EK139

Steward Observatory, Paul Hartogh, Michael Mommert, 2012, 1204.0899.

GAPS IN THE HD 169142 PROTOPLANETARY DISK REVEALED BY POLARIMETRIC IMAGING: SIGNS OF ONGOING PLANET FORMATION?

Steward Observatory, Sascha P. Quanz, Esther Buenzli, 2013, 1302.3029.

The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts

Steward Observatory, Tucson, AZ, 2014, 1409.7082.