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Q/W-band Observations toward Starless Cores in Orion (QWOSCO). I. Overview, Isotopologues, Isomers, and Complex Organics

  • Authors: Shih-Ying Hsu, Xunchuan Liu, Sheng-Yuan Liu, Tie Liu, Naomi Hirano, Mika Juvela, Kee-Tae Kim, Chin-Fei Lee, Shanghuo Li, Sheng-Jun Lin, Sheng-Li Qin, Dipen Sahu, Ken'ichi Tatematsu, Fengwei Xu, L. Viktor Tóth

Shih-Ying Hsu et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 2.

The detection statistics and distribution of the molecular column densities. In the boxplots, the box spans the IQR, from the first quartile (Q1, 25%) to the third quartile (Q3, 75%). The line within each box indicates the median (Q2, 50%), which is also labeled at the right end of each row. The whiskers extend from the quartiles to 1.5 times the IQR (i.e., values within Q1 -1.5 × IQR and Q3 +1.5 × IQR), while data points outside this range are treated as outliers and shown in circles.

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