230 citations · 423 across the 15 of their papers we have counts for
15 papers
Estimation of Dust Mass from Infrared Emission and Extinction of Supernova Remnants: G93.7-0.2, G109.1-1.0, G156.2+5.7, and G166.0+4.3
Zhe Zhang, Jun Li, Biwei Jiang +1
Supernova remnants (SNRs) are major sites for both the production and destruction of interstellar dust, and quantifying their dust budget is essential for understanding the life cy…
Distance Determination of Southern Galactic Plane Supernova Remnants with the Mopra CO Survey and DECaPS 3D Dust Map
Fupeng Liu, He Zhao, Biwei Jiang +2
Accurate distance measurements to supernova remnants (SNRs) are crucial for understanding their physical properties, evolutionary processes, and role in the Galactic interstellar m…
Extinction of Taurus, Orion, Perseus and California Molecular Clouds Based on the LAMOST, 2MASS, and Gaia Surveys II: The Extinction Law
Zhetai Cao, Biwei Jiang, Shu Wang +1
The extinction law from ultraviolet (UV) to infrared (IR) (0.2-24 m) is determined by relying on the blue-edge method and color excess ratios for some nearby molecular clouds, f…
Data-driven stellar intrinsic colors and dust reddenings for spectro-photometric data: From the blue-edge method to a machine-learning approach
He Zhao, Shu Wang, Biwei Jiang +4
Intrinsic colors (ICs) of stars are essential for the studies on both stellar physics and dust reddening. In this work, we developed an XGBoost model to predict the ICs with the at…
The Infrared Extinction Law in the Ophiuchus Molecular Cloud based on UKIDSS and Spitzer
Jun Li, Xi Chen
Investigating the extinction properties in dense molecular clouds is of significant importance for understanding the behavior of interstellar dust and its impact on observations. I…
Dust Mass Associated with the Supernova Remnant IC 443 when Emission Meets Extinction
Jun Li, Biwei Jiang, He Zhao
The dust mass of the well-known supernova remnant (SNR) IC 443 is estimated from both the infrared emission and the visual extinction. With photometry to the images taken by \emph{…