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Cited article:

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Excess C/H in Protoplanetary Disk Gas from Icy Pebble Drift Across the CO Snowline

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CO Depletion in Protoplanetary Disks: A Unified Picture Combining Physical Sequestration and Chemical Processing

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13C17O suggests gravitational instability in the HL Tau disc

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ALMA Observations of Young Eruptive Stars: Continuum Disk Sizes and Molecular Outflows

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Bright C2H emission in protoplanetary discs in Lupus: high volatile C/O > 1 ratios

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Line Ratios Reveal N2H+ Emission Originates above the Midplane in TW Hydrae

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A Three-phase Approach to Grain Surface Chemistry in Protoplanetary Disks: Gas, Ice Surfaces, and Ice Mantles of Dust Grains

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Dust Continuum Emission and the Upper Limit Fluxes of Submillimeter Water Lines of the Protoplanetary Disk around HD 163296 Observed by ALMA

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The First Detection of 13C17O in a Protoplanetary Disk: A Robust Tracer of Disk Gas Mass

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The Astrophysical Journal Letters 882 (2) L31 (2019)
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Planet-forming material in a protoplanetary disc: the interplay between chemical evolution and pebble drift

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Gas versus dust sizes of protoplanetary discs: effects of dust evolution

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Systematic Variations of CO Gas Abundance with Radius in Gas-rich Protoplanetary Disks

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Probing the Gas Content of Late-stage Protoplanetary Disks with N2H+

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Unlocking CO Depletion in Protoplanetary Disks. II. Primordial C/H Predictions inside the CO Snowline

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Ingredients for solar-like systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov–Gerasimenko

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