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Weitere Publikationen von Autoren mit dem selben Namen

The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold, , , , , , , , , und 2 andere Autor(en). (2015)cite arxiv:1504.02479Comment: Submitted to ApJ.A submillimeter galaxy illuminating its circumgalactic medium: Ly-alpha scattering in a cold, clumpy outflow, , , , , , , , , und 10 andere Autor(en). (2014)cite arxiv:1402.6335Comment: Submitted to ApJ.A deep ALMA image of the Hubble Ultra Deep Field, , , , , , , , , und 26 andere Autor(en). (2016)cite arxiv:1606.00227Comment: 25 pages, 14 figures, submitted to MNRAS.VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA, , , , , , , , , und 11 andere Autor(en). (2016)cite arxiv:1611.05867Comment: Accepted for publication in A&A. Abstract abridged for arXiv. 13 pages, including 5 figures and 2 tables.Witnessing the birth of the red sequence: the physical scale and morphology of dust emission in hyper-luminous starbursts in the early Universe, , , , , , , , , und 15 andere Autor(en). (2017)cite arxiv:1709.04191Comment: Submitted to ApJ. Comments welcome.The average submillimetre properties of Lyman-alpha Blobs at z=3, , , , , , , , , und 4 andere Autor(en). (2016)cite arxiv:1605.04912v1.pdfComment: Accepted MNRAS 16 May 2016.A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time, , , , , , , und . (2019)cite arxiv:1902.09172Comment: 21 pages, 10 figures, 8 table, accepted for publication in A&A.Witnessing the birth of the red sequence: ALMA high-resolution imaging of CII and dust in two interacting ultra-red starbursts at z = 4.425, , , , , , , , , und 12 andere Autor(en). (2016)cite arxiv:1601.07549Comment: Submitted to ApJ.The evolving far-IR galaxy luminosity function and dust-obscured star-formation rate density out to z~5, , , , , , , und . (2017)cite arxiv:1706.00426Comment: 17 pages, 12 figures, 5 tables, submitted to MNRAS.An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115, , , , , , , , , und 21 andere Autor(en). (2017)cite arxiv:1704.03868Comment: ApJ submitted. Comments welcome.