No evolution of the AGN fraction was found, either along the merger sequence or compared to isolated galaxies (5.0%). A total of 61 (5.5%) AGNs in pairs were identified based on the emission-line diagnostics. This pair sample of 1156 IFU-covered galaxies were selected by the velocity offset, projected separation, and morphology from SDSS IV-MaNGA survey, and is further classified into four cases along the merger sequence based on morphological signatures. Lower right: Interaction show different impact on the resolved properties of AGNs and SFGs. Lower left: Similar distributions of paired AGNs and isolated AGNs in the SFR-Mass diagram. Upper panel: An example of AGN identification using IFU data. An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs Lei Zhu (Deputy Director of CASSACA more details, please read the attached announcement ( pdf). Jiasheng Huang (Chief Scientist of CASSACA or Dr. The deadline for applications is now extended to May,31st 2022. We are aiming to support 3 or 4 projects in this call.
The duration of each project should be two years at maximum, and can request up to 75,000 USD/year. These funds are for research projects based on a collaboration between astronomers from China and Chile, and the subject can be in areas such as astronomical research, observations, instrumental development, theory, etc. Based on the principles established in a 2013 Memorandum of Understanding (MoU) between the Chinese Academy of Sciences (CAS) and the National Commission of Scientific and Technological Research of the Republic of Chile (CONICYT), and the more specific guidelines described in a recent (2015) Agreement between the National Astronomical Observatories of China (NAOC), the Chinese Astronomical Society, the Chilean Astronomical Society (SOCHIAS) and CONICYT ( pdf), we are now inviting research proposals that involve China-Chile collaboration in astronomical research, to promote astronomical research collaborations between China and Chile, to advance astronomy in both countries.
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