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Disambiguation of "Menten, Karl"

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An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: Spectroscopic redshifts

, , , , , , , , , , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1705.03503Comment: 26 pages; 15 figures. Accepted for publication in ApJ. Redshift catalogs, spectra and SED templates available from: http://astro.dur.ac.uk/~ams/zLESS/.

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Karl Menten

Karl Martin Menten

Wilhelm Menten

Karl

Rosa Karl

 

Other publications of authors with the same name

Revealing a spiral-shaped molecular cloud in our galaxy - Cloud fragmentation under rotation and gravity, , and . Astronomy & Astrophysics, (Oct 24, 2016)An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: Spectroscopic redshifts, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1705.03503Comment: 26 pages; 15 figures. Accepted for publication in ApJ. Redshift catalogs, spectra and SED templates available from: http://astro.dur.ac.uk/~ams/zLESS/.An ALMA survey of Sub-millimetre Galaxies in the Extended Chandra Deep Field South: Detection of C II at z=4.4, , , , , , , , , and 12 other author(s). (2012)cite arxiv:1209.1390Comment: Accepted for publication in MNRAS. 10 pages, 5 figures, 2 tables.Imaging the cold molecular gas in SDSS J1148 + 5251 at z = 6.4, , , , , , , , , and . (2015)cite arxiv:1505.07669Comment: 6 pages, 5 figures, 1 table; accepted by MNRAS.Molecular Cloud-scale Star Formation in NGC 300, , , , and . (2014)cite arxiv:1405.2337Comment: 42 pages, 14 figures, 7 tables. Includes a complete image atlas of our HII region targets. ASCII versions of tables will be available electronically after paper is published. Accepted for publication in the Astrophysical Journal.ALMA and VLA measurements of frequency-dependent time lags in Sagittarius A*: evidence for a relativistic outflow, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1502.03423Comment: 10 pages, 9 figures. Accepted for publication in A&A. Updated acknowledgements.Dense gas in the Galactic central molecular zone is warm and heated by turbulence, , , , , , , , , and 12 other author(s). (2015)cite arxiv:1509.01583Comment: Accepted to A&A. The data (raw & processed) are available from http://doi.org/10.7910/DVN/27601 . The processing pipeline, analysis code, and paper source are available at https://github.com/adamginsburg/APEX_CMZ_H2CO.Constraining Dust and Molecular Gas Properties in Lyman Alpha Blobs at z~3, , , , , , , , , and 7 other author(s). (2011)cite arxiv:1110.1457Comment: Accepted for publication in ApJ, 10 pages, 7 figures.C II radiative cooling of the Galactic diffuse interstellar medium: Insight about the star formation in Damped Lyman-alpha systems, , , , , and . (2016)cite arxiv:1606.04966Comment: 16 pages, 3 tables, 9 figures. Accepted for publication in ApJ. The definitive version will be available at http://iopscience.iop.org/0004-637X.From Poloidal to Toroidal: Detection of Well-ordered Magnetic Field in High-mass Proto-cluster G35.2-0.74N, , , , and . (Nov 4, 2013)