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Members
Ruiyu Pan
Niels Bohr Institute, Copenhagen, Denmark
​IR signatures from AGN at high redshift​​
Archana Purushothaman
University of Bologna, Italy
Upper limit of dust masses as function
of progenitor mass​​
Aman Kumar
Indian Institute of Astrophysics, India
Dust formation in low and intermediate
mass SN progenitors
​​​
Sujit Das
Indian Institute of Astrophysics, India
Evolution of late stage massive stars
and their environments
​​​
Abantika Ghosh
Calcutta University, India & University of Albany, USA
Dust formation efficiency of supernovae based on their light curves
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