Erratum: Protoplanetary Disk Masses from Radiative Transfer Modeling: A Case Study in Taurus (Astronomical Journal (2019) 157 (144) DOI: 10.3847/1538-3881/ab0a56)

Nicholas P. Ballering; Josh A. Eisner

doi:10.3847/1538-3881/ab1c56

Erratum: Protoplanetary Disk Masses from Radiative Transfer Modeling: A Case Study in Taurus (Astronomical Journal (2019) 157 (144) DOI: 10.3847/1538-3881/ab0a56)

Nicholas P. Ballering, Josh A. Eisner

Astronomy

Research output: Contribution to journal › Comment/debate › peer-review

Abstract

There was a plotting error in Figure 5 of the original paper. The blue curves in the third column were plotted using too few points so the shapes of the curves were not clear. A corrected version of the figure is shown here. (Figure Presented).

Original language	English (US)
Article number	214
Journal	Astronomical Journal
Volume	157
Issue number	5
DOIs	https://doi.org/10.3847/1538-3881/ab1c56
State	Published - May 2019

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-3881/ab1c56

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title = "Erratum: Protoplanetary Disk Masses from Radiative Transfer Modeling: A Case Study in Taurus (Astronomical Journal (2019) 157 (144) DOI: 10.3847/1538-3881/ab0a56)",

abstract = "There was a plotting error in Figure 5 of the original paper. The blue curves in the third column were plotted using too few points so the shapes of the curves were not clear. A corrected version of the figure is shown here. (Figure Presented).",

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AU - Eisner, Josh A.

PY - 2019/5

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N2 - There was a plotting error in Figure 5 of the original paper. The blue curves in the third column were plotted using too few points so the shapes of the curves were not clear. A corrected version of the figure is shown here. (Figure Presented).

AB - There was a plotting error in Figure 5 of the original paper. The blue curves in the third column were plotted using too few points so the shapes of the curves were not clear. A corrected version of the figure is shown here. (Figure Presented).

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Erratum: Protoplanetary Disk Masses from Radiative Transfer Modeling: A Case Study in Taurus (Astronomical Journal (2019) 157 (144) DOI: 10.3847/1538-3881/ab0a56)

Abstract

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