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20152026
most citedMolecules with ALMA at Planet-forming Scales (MAPS) I: Program Overview and Highlights

288 citations · 2.9k across the 84 of their papers we have counts for

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Showing 2025Show all

9 papers · 1 filter

astro-ph.EP2025

CORINOS IV: Quantifying Baseline-Fitting Uncertainties in SO Ice Measurements with JWST/MIRI

Rachel E. Gross, Yao-Lun Yang, L. Ilsedore Cleeves +15

Sulfur dioxide (SO) ice has been tentatively detected in protostellar envelopes, but its reliability as a solid-state sulfur reservoir remains unclear. We present new measureme…

astro-ph.EP2025★ 2 cited

The Flying Saucer edge-on disc's Near Infrared silhouette revealed by the JWST JEDIce program

Emmanuel Dartois, Jennifer A. Noble, Jennifer B. Bergner +17

Edge-on discs offer a unique opportunity to probe radial and vertical dust and gas distributions in the protoplanetary phase. This study aims to investigate the distribution of mic…

astro-ph.EP2025

Oxygen Isotope Constraints on the Importance of Photochemical Processing in Protoplanetary Disks

Fred J. Ciesla, Eric Van Clepper, Jennifer Bergner +1

Observations have revealed evidence of photochemical processing in protoplanetary disks. This processing occurs in the photon dominated layer, the optically thin regions of the dis…

astro-ph.SR2025★ 1 cited

Variation of the disk thickness across ice bands: A method to determine ice abundances in highly inclined protoplanetary disks

Laurine Martinien, Gaspard Duchêne, François Ménard +6

The James Webb Space Telescope provides unprecedented information to study ices in protoplanetary disks. However, the saturation of ice bands in highly inclined disks hinders the m…

astro-ph.GA2025

PEACHES IV: Tracing the Formation & Evolution of CH in Perseus Low-Mass Protostars

Jack G. Anderson, Jennifer B. Bergner, Yao-Lun Yang +2

The radical hydrocarbon molecule CH is widely detected in various stages of star and planet formation, and has emerged as a useful tracer of high-C/O gas within the photochemic…

astro-ph.EP2025★ 1 cited

On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres

Adina D. Feinstein, Richard A. Booth, Jennifer B. Bergner +34

Measuring a single elemental ratio (e.g., carbon-to-oxygen) provides insufficient information for understanding the formation mechanisms and evolution that affect our observations…