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Disambiguation of "Sawicki, Marcin"

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Stars, Dust, and the Growth of UV-Selected Sub-L* Galaxies at Redshift z~2

. (2011)cite arxiv:1108.5186Comment: Resubmitted to MNRAS after addressing referee's comments.

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Martin Sawicki

Peter Sawicki

Sergiusz Sawicki

Piotr Sawicki

Diethard Sawicki

 

Other publications of authors with the same name

Confirmation of a Steep Luminosity Function for Lyman-alpha Emitters at z = 5.7: A Major Component of Reionization, , , , , and . (2014)cite arxiv:1412.0655Comment: 9 pages, 4 figures.The Obscured Fraction of Quasars at Cosmic Noon, , , , , , , , and . (2022)cite arxiv:2209.07797Comment: 25 Pages, 19 Figure, ApJ accepted.Ruby Annotation, , , , and . World Wide Web Consortium, Recommendation REC-ruby-20010531, (May 2001)Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem, and . (Jan 23, 2018)Ionizing radiation from AGNs at z>3.3 with the Subaru Hyper Suprime-Cam Survey and the CFHT Large Area U-band Deep Survey (CLAUDS), , , , , , , , , and 1 other author(s). (2021)cite arxiv:2109.10138Comment: 19 pages, 12 figures. Accepted for publication in Monthly Notices of the Royal Astronomical Society.The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe, , , , , , , , , and 167 other author(s). (2016)cite arxiv:1606.00043Comment: 210 pages, 91 figures. Exposure draft. Appendices to the Detailed Science Case can be found at http://mse.cfht.hawaii.edu/docs/.Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1704.06004Comment: 28 pages, 11 figures, submitted to a special issue of PASJ.Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging, , and . (2014)cite arxiv:1407.2319Comment: Accepted for publication in MNRAS.$Łambda$CDM not dead yet: massive high-z Balmer break galaxies are less common than previously reported, , , , , , , , , and 8 other author(s). (2023)cite arxiv:2310.03063Comment: Submitted to MNRAS, 10 pages (+4 in Appendix), 5 figures (+4), 1 table (+1).Detections of Faint Lyman-alpha Emitters at z = 5.7: Galaxy Building Blocks and Engines of Reionization, , , , and . (2011)cite arxiv:1104.2900 Comment: 15 pages, 12 figures. Submitted to ApJ.