D
Dietrich Lemke
Researcher at Max Planck Society
Publications - 229
Citations - 8449
Dietrich Lemke is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 39, co-authored 229 publications receiving 8095 citations. Previous affiliations of Dietrich Lemke include University of Arizona.
Papers
More filters
Journal ArticleDOI
Small-scale structure of the galactic cirrus emission
TL;DR: In this paper, the Fourier power spectrum characteristics of cirrus structures in 13 sky fields with faint to bright cirrus emission observed with ISOPHOT in the 90-200µm wavelength range were examined.
Journal ArticleDOI
The Small Magellanic Cloud in the far infrared - I. ISO's 170 $\mu$m map and revisit of the IRAS 12–100 $\mu$m data
TL;DR: In this article, the ISOPHOT experiment onboard the ISO satellite generated a complete view of the Small Magellanic Cloud (SMC) at 170 µm with 1.5 arcmin resolution.
Journal ArticleDOI
A far infrared view of low mass star formation in the Cederblad 110 nebula of Chamaeleon I
TL;DR: The Cederblad 110 reflection nebula as mentioned in this paper contains several young stellar objects previously discovered by IRAS and sub-mm observations and was revisited with ISO's FIR cameras and mapped with higher spatial resolution.
Journal ArticleDOI
Isophot - photometric calibration of point sources
Benjamin L. Schulz,S. Huth,R. J. Laureijs,J. A. Acosta-Pulido,J. A. Acosta-Pulido,M. Braun,Héctor O. Castañeda,Héctor O. Castañeda,Martin Cohen,L. Cornwall,C. Gabriel,Peter Hammersley,I. Heinrichsen,I. Heinrichsen,Ulrich Klaas,Dietrich Lemke,Th. Müller,David J. Osip,David J. Osip,P. Roman-Fernandez,Charles M. Telesco +20 more
TL;DR: In this paper, the authors present the calibration concept for point sources within a flux-range from 60 mJy up to 4500 Jy for staring and raster observations in standard configurations and discuss the requisite measurements and uncertainties involved.
Journal ArticleDOI
Unidentified Infrared Bands in the Interstellar Medium across the Galaxy
TL;DR: In this article, a set of 6-12 micron ISOPHOT-S spectra of the general interstellar medium of the Milky Way is presented, which is dominated by a series of strong, wide emission features commonly called the Unidentified Infrared Bands.