Members will be sent instructions on how to join the m eeting in the week prior to the event.
In her prese ntation Dr Anshu Gupta will focus on how galaxies evolve in conjunction wit h their chemical evolution.
Her main focus is to understand how the l ocal environment shapes galaxies as we see them today, from clouds of gas t o galaxies like our Milky Way. She combines observations from the largest g round based telescopes with the state-of-the-art cosmological simulations t o estimate if galaxies living in dense galaxy clusters produce metals faste r than galaxies living in isolation.
is a postdoctoral fellow at the University of New So uth Wales, Sydney. She completed her dual bachelor undergraduate and Master of Science degrees in May 2013 at the Indian Institute of Science Educatio n and Research, Mohali, India. Her thesis is titled: 3He [II] - An alternat ive probe for Reionization.
She did her graduate studies/PhD (2018) a t Australian National University (ANU), Canberra with Prof Lisa Kewley and Dr Tiantian Yuan. Her thesis is titled: Chemical evolution of star-forming galaxies in the overdense environment.
"I am interested in understanding the origin and evolution of galaxies like ou r own Milky Way. My primary research focus is in figuring out how galaxies build different elements. I use optical and near-infrared spectroscopic obs ervations of galaxies, to understand the evolution of kinematic, chemical a nd other inter-stellar medium properties of galaxies over the past 12 billi on years.
In my work, I try to establishes a direct connection betwee n observations and, the state-of-the-art hydrodynamical simulations and the oretical models, which is essential to fully understand the physics of gala xy formation and evolution."
X-ALT-DESC;FMTTYPE=text/html:Members will be sent instructions on how to join the m eeting in the week prior to the event.
In her prese ntation Dr Anshu Gupta will focus on how galaxies evolve in conjunction wit h their chemical evolution.
Her main focus is to understand how the l ocal environment shapes galaxies as we see them today, from clouds of gas t o galaxies like our Milky Way. She combines observations from the largest g round based telescopes with the state-of-the-art cosmological simulations t o estimate if galaxies living in dense galaxy clusters produce metals faste r than galaxies living in isolation.
Dr Anshu Guptais a postdoctoral fellow at the University of New South Wales, Sydney. She completed her dual bachelor undergraduate and Master of Science degrees in May 2013 at the Indian Insti tute of Science Education and Research, Mohali, India. Her thesis is titled : 3He [II] - An alternative probe for Reionization.
She did her gradu ate studies/PhD (2018) at Australian National University (ANU), Canberra wi th Prof Lisa Kewley and Dr Tiantian Yuan. Her thesis is titled: Chemical ev olution of star-forming galaxies in the overdense environment.
"I am interested in understanding the origin and evolu tion of galaxies like our own Milky Way. My primary research focus is in fi guring out how galaxies build different elements. I use optical and near-in frared spectroscopic observations of galaxies, to understand the evolution of kinematic, chemical and other inter-stellar medium properties of galaxie s over the past 12 billion years.
In my work, I try to establishes a direct connection between observations and, the state-of-the-art hydrodynam ical simulations and theoretical models, which is essential to fully unders tand the physics of galaxy formation and evolution."
DTSTAMP:20260621T072307 DTSTART;TZID=Australia/Sydney:20200903T193000 DTEND;TZID=Australia/Sydney:20200903T213000 SEQUENCE:0 TRANSP:OPAQUE END:VEVENT END:VCALENDAR