Published June 21, 2021 | Version v1
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Data from "Multi-wavelength continuum sizes of protoplanetary discs: scaling relations and implications for grain growth and radial drift"

  • 1. University of Cambridge

Description

Table 1, Table 2, and Table 3 from Tazzari et al., 2021, "Multi-wavelength continuum sizes of protoplanetary discs: scaling relations and implications for grain growth and radial drift", Monthly Notices of the Royal Astronomical Society, arXiv:2010.02249

Both tables are available in IPAC format, which is in human- and machine-readable:

from astropy.io import ascii
tb = ascii.read('Table1.txt', format='ipac')

Table comments (stored at the beginning of the ASCII file as lines starting with "/") can be read as:

tb.meta['comments']

Files

Table1.txt

Files (21.6 kB)

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md5:8349efd6cf0009f87da9e2c54974be41
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md5:8abe4c948c551f1192b8dcf0f03f6c07
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md5:643bb56ef4e7f16134970e60b11cf1fe
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Additional details

Related works

Is compiled by
Preprint: arXiv:2010.02249 (arXiv)

Funding

European Commission
ECOGAL - Star Formation and the Galactic Ecology 291227
European Commission
DUSTBUSTERS - Dust and gas in planet forming discs 823823
UK Research and Innovation
Consolidated Grant Astronomy Observation and Theory 2019-2022 ST/S000623/1