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ZENODO
Dataset . 2017
License: CC BY SA
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2017
License: CC BY SA
Data sources: ZENODO
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2017
License: CC BY SA
Data sources: Datacite
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Evolution Of Cosmic Star Formation In The Scuba-2 Cosmology Legacy Survey

Authors: Bourne, Nathan;

Evolution Of Cosmic Star Formation In The Scuba-2 Cosmology Legacy Survey

Abstract

This dataset consists of tabulated data from the figures included in the referenced publication. The following datasets are included: Stacked SFR obscuration (IRX=IR/UV) of UVJ-selected star-forming galaxies: Weighted mean IRX as a function of Muv & stellar mass (Figure 12): MUV_irx1.dat Weighted mean IRX as a function of beta, over all masses and redshifts: beta_irx.dat Weighted mean IRX as a function of beta, binned by stellar mass (Figure 13): beta_irx_mstar.dat Weighted mean IRX as a function of beta, binned by redshift (Figure 14): beta_irx_z.dat Cosmic SFR density as a function of redshift for massive galaxies log(Ms/Msol)>10 (Figure 15): All mass-selected galaxies: sfrd_massive.dat UV-luminous galaxies Muv<M*; log(Ms/Msol)>10: sfrd_hiLUV.dat IR-luminous galaxies detected at 450µm: sfrd_IRdet.dat Cosmic SFR density as a function of redshift corrected to all stellar masses (Figure 16): All mass-selected galaxies: sfrd_uvlfcorr.dat UV-luminous galaxies Muv<M*; log(Ms/Msol)>10: sfrd_hiLUV_uvlfcorr.dat Full details of the binning and stacking methodology are explained in the paper.

{"references": ["Bourne, Nathan et al. (2017) Monthly Notices of the Royal Astronomical Society, 467, 1360"]}

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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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