CU-JADE: A Method for Traversing Extinction Jumps along the Line of Sight

TL;DR

CU-JADE is a new method that detects abrupt changes in extinction data to improve distance measurements to molecular clouds, helping map the 3D structure of the interstellar medium more accurately.

Contribution

The paper introduces CU-JADE, a novel CUSUM-based technique that enhances distance estimation to molecular clouds by detecting extinction jumps, combining multiwavelength data for comprehensive 3D mapping.

Findings

Successfully identified multilayered molecular gas in Cepheus.

Determined accurate distances beyond Cygnus Rift.

Constructed a 3D extinction map up to 4 kpc.

Abstract

Although interstellar dust extinction serves as a powerful distance estimator, the solar system's location within the Galactic plane complicates distance determinations, especially for molecular clouds (MCs) at varying distances along the line of sight (LoS). The presence of complex extinction patterns along the LoS introduces degeneracies, resulting in less accurate distance measurements to overlapping MCs in crowded regions of the Galactic plane. In this study, we develop the CUSUM-based Jump-point Analysis for Distance Estimation (CU-JADE), a novel method designed to help mitigate these observational challenges. The key strengths of CU-JADE include: (1) sensitivity to detect abrupt jumps in Distance-$A_{\lambda}$ ($D$-$A$) datasets, (2) minimal systematic errors as demonstrated on both mock and observed data, and (3) the ability to combine CUSUM analysis with multiwavelength data to improve the completeness of distance measurements for nearby gas structures, even for extinction values as low as $\Delta A_{V} \gtrsim 0.15$ mag. By combining CO survey data with a large sample of stars characterized by high-precision parallaxes and extinctions, we uncovered the multilayered molecular gas distribution in the high-latitude Cepheus region. We also determined accurate distances to MCs beyond the Cygnus Rift by analyzing the intricate structure of gas and extinction within the Galactic plane. Additionally, we constructed a full-sky 3D extinction map extending to 4 kpc, which provides critical insights into dense interstellar medium components dominated by molecular hydrogen. These results advance our understanding of the spatial distribution and physical properties of MCs across the Milky Way.