Marcin Sawicki
Identifiers
- name variant Marcin Sawicki 0.60 · backfill
Papers (51)
- Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff astro-ph.GA · 2026 · author #2
- The Role of Cluster Environments in Quiescent Galaxy Stellar Halo Assembly astro-ph.GA · 2026 · author #3
- LARgE Survey. I. Dead Monsters: the Massive End of the Passive Galaxy Stellar Mass Function at Cosmic Noon astro-ph.GA · 2019 · author #2
- Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity astro-ph.GA · 2018 · author #11
- Gemini Infrared Multi-Object Spectrograph: Instrument Overview astro-ph.IM · 2018 · author #7
- On the fast quenching of young low-mass galaxies up to z $\sim$ 0.6: new spotlight on the lead role of environment astro-ph.GA · 2018 · author #2
- Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common astro-ph.GA · 2018 · author #15
- Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem astro-ph.GA · 2018 · author #2
- Chemical Mapping of the Milky Way With The Canada-France Imaging Survey: A Non-parametric Metallicity-Distance Decomposition of the Galaxy astro-ph.GA · 2017 · author #38
- The Canada-France Imaging Survey: First results from the u-band component astro-ph.GA · 2017 · author #38
- SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-End Counts at 450 um astro-ph.GA · 2017 · author #34
- Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z \sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky astro-ph.GA · 2017 · author #7
- The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe astro-ph.IM · 2016 · author #170
- Missing Stellar Mass in SED Fitting: Spatially Unresolved Photometry can Underestimate Galaxy Masses astro-ph.GA · 2015 · author #2
- Confirmation of a Steep Luminosity Function for Lyman-alpha Emitters at z = 5.7: A Major Component of Reionization astro-ph.GA · 2014 · author #4
- Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging astro-ph.GA · 2014 · author #2
- SEDfit: Software for Spectral Energy Distribution Fitting of Photometric Data astro-ph.IM · 2012 · author #1
- Stars, Dust, and the Growth of UV-Selected Sub-L* Galaxies at Redshift z~2 astro-ph.CO · 2011 · author #1
- Keck Deep Fields. IV. Luminosity Dependent Clustering and Galaxy Downsizing in UV-Selected Galaxies at z=4, 3, and 2 astro-ph.CO · 2011 · author #2
- Detections of Faint Lyman-alpha Emitters at z = 5.7: Galaxy Building Blocks and Engines of Reionization astro-ph.CO · 2011 · author #4
- The build-up of mass in UV-selected sub-L* galaxies at z~2 astro-ph.CO · 2011 · author #1
- How Future Space-Based Weak Lensing Surveys Might Obtain Photometric Redshifts Independently astro-ph.CO · 2011 · author #2
- Using the 1.6um Bump to Study Rest-frame NIR Selected Galaxies at Redshift 2 astro-ph.CO · 2010 · author #2
- Stellar Populations of Lyman-alpha Emitters at z=4.86: A Comparison to $z\sim5$ LBGs astro-ph.CO · 2010 · author #8
- New Results from the Magellan IMACS Spectroscopic Lyman Alpha Survey: NICMOS Observations of Lyman Alpha emitters at z=5.7 astro-ph.CO · 2010 · author #5
- Lyman Break Galaxies at z~5: Rest-Frame UV Spectra. III astro-ph.CO · 2009 · author #9
- Serendipitous Discovery of an Overdensity of Lyman-Alpha Emitters at z~4.8 in the Cl1604 Supercluster Field astro-ph.CO · 2009 · author #3
- The Stellar Populations of Lyman Break Galaxies at z~5 astro-ph · 2008 · author #4
- Differential Evolution of Lyman Break Galaxies from $z$=5 to 3 astro-ph · 2008 · author #3
- The Stellar Populations of Lyman Break Galaxies at $z\sim5$ astro-ph · 2008 · author #4
- A Magellan IMACS Spectroscopic Search for Lyman-Alpha Emitting Galaxies at Redshift 5.7 astro-ph · 2008 · author #2
- Four quasars above redshift 6 discovered by the Canada-France High-z Quasar Survey astro-ph · 2007 · author #16
- The Long Faint Tail of the High-Redshift Galaxy Population astro-ph · 2006 · author #1
- Keck Deep Fields. III. Luminosity-dependent Evolution of the Ultraviolet Luminosity and Star Formation Rate Densities at z~4, 3, and 2 astro-ph · 2006 · author #1
- Sub-L* Galaxies at Redshifts z~4, 3, and 2: Their UV Luminosity Function and Luminosity Density astro-ph · 2005 · author #1
- Preliminary Results from a Spectrosopic LyA Survey at Redshift 5.7 with IMACS astro-ph · 2005 · author #2
- Imaging of SDSS z>6 quasar fields: gravitational lensing, companion galaxies and the host dark matter halos astro-ph · 2005 · author #7
- A search for the first massive galaxy clusters astro-ph · 2004 · author #4
- Submillimeter Observations of Low Metallicity Galaxy NGC 4214 astro-ph · 2004 · author #3
- Redshifts in the Hubble Deep Field South astro-ph · 2003 · author #1
- The Absorption and Emission Kinematics in the z=0.7450 Mg II Absorber Towards Q1331+17 astro-ph · 2003 · author #3
- The 1.6um Bump as a Photometric Redshift Indicator astro-ph · 2002 · author #1
- The Ultraviolet-Far Infrared Energy Budget of the Gravitationally Lensed Lyman Break Galaxy MS1512-cB58 astro-ph · 2001 · author #1
- Active Galactic Nuclei in the CNOC2 Field Galaxy Redshift Survey astro-ph · 2000 · author #6
- Spectroscopic Gravitational Lens Candidates in the CNOC2 Field Galaxy Redshift Survey astro-ph · 2000 · author #8
- The DDO IVC Distance Project astro-ph · 1998 · author #10
- The David Dunlap Observatory IVC Distance Project: First Results astro-ph · 1998 · author #3
- The Distance to the Draco Cloud astro-ph · 1998 · author #10
- A blind test of photometric redshift prediction astro-ph · 1998 · author #8
- Optical-IR Spectral Energy Distributions of z>2 Lyman Break Galaxies astro-ph · 1997 · author #1
- Optical-IR Spectral Energy Distributions of z>2 Galaxies astro-ph · 1997 · author #1
Mentions
- 1210.0285 #1 · backfill · confidence 0.70 Marcin Sawicki
- 1108.5186 #1 · backfill · confidence 0.70 Marcin Sawicki
- 1106.2146 #2 · backfill · confidence 0.70 Marcin Sawicki
- 1104.2900 #4 · backfill · confidence 0.70 Marcin Sawicki
- 1102.2005 #1 · backfill · confidence 0.70 Marcin Sawicki
- 1101.4635 #2 · backfill · confidence 0.70 Marcin Sawicki
- 1007.4951 #2 · backfill · confidence 0.70 Marcin Sawicki
- 1007.2057 #8 · backfill · confidence 0.70 Marcin Sawicki
- 1006.3076 #5 · backfill · confidence 0.70 Marcin Sawicki
- 0908.1646 #9 · backfill · confidence 0.70 Marcin Sawicki
- 0905.2233 #3 · backfill · confidence 0.70 Marcin Sawicki
- 0811.2041 #4 · backfill · confidence 0.70 Marcin Sawicki
- 0807.0137 #4 · backfill · confidence 0.70 Marcin Sawicki
- 0807.0123 #3 · backfill · confidence 0.70 Marcin Sawicki
- 0802.2393 #2 · backfill · confidence 0.70 Marcin Sawicki
- 0706.0914 #16 · backfill · confidence 0.70 Marcin Sawicki
Frequent Coauthors
- Kouji Ohta 7 shared papers
- Masayuki Akiyama 7 shared papers
- Ikuru Iwata 6 shared papers
- Alan Dressler 5 shared papers
- Crystal L. Martin 5 shared papers
- Kentaro Aoki 5 shared papers
- Luc Simard 5 shared papers
- Naoyuki Tamura 5 shared papers
- Robert Sorba 5 shared papers
- Anneya Golob 4 shared papers
- Chris J. Willott 4 shared papers
- David Crampton 4 shared papers
- David Thompson 4 shared papers
- Douglas Scott 4 shared papers
- Gabriela Mallen-Ornelas 4 shared papers
- Kim Venn 4 shared papers
- Kiyoto Yabe 4 shared papers
- Michael D. Gladders 4 shared papers
- Scott Chapman 4 shared papers
- Alan McConnachie 3 shared papers