IC 1396 members HSC and UKIDSS photometry

To identify member populations of IC 1396, we employed the random forest (RF) classifier of machine learning technique. The RF classifier is an ensemble of individual decision trees suitable for large, high-dimensional datasets. The training set used in this work is derived from previous Gaia-based studies, in which the member stars are younger than ~10Myr.

However, its sensitivity is limited to ~20mag in the r2 band, making it challenging to identify candidates at the fainter end. In this analysis, in addition to magnitudes and colours, we incorporated several derived parameters from the magnitude and colour of the sources to identify candidate members of the star-forming complex. By employing this method, we were able to identify promising candidate member populations of the star-forming complex.

We discuss the associated limitations and caveats in the method and improvements for future studies. In this analysis, we identify 2425 high-probability low-mass stars distributed within the entire star-forming complex, of which 1331 are new detections. A comparison of these identified member populations shows a high retrieval rate with Gaia-based literature sources, as well as sources detected through methods based on optical spectroscopy, Spitzer, H{alpha}/X-ray emissions, optical photometry, and 2MASS photometry.

The mean age of the member populations is ~2-4Myr, consistent with findings from previous studies. Considering the identified member populations, we present preliminary results by exploring the presence of sub-clusters within IC 1396, assessing the possible mass limit of the member populations, and providing a brief discussion on the star formation history of the complex. The primary aim of this work is to develop a method of identifying candidate member populations from a deep, sensitive dataset such as Subaru-HSC by employing machine learning techniques.

Although we overcome some limitations in this study, the method requires further improvements to address the caveats associated with such a membership analysis.