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UID:b2a61fe7bf91033190a3aaa7e012040b
CATEGORIES:Guest Speaker Night
CREATED:20200901T225922
SUMMARY:Guest Speaker - Dr Anshu Gupta – UNSW
LOCATION:Zoom Meeting - members will be invited
DESCRIPTION:Note that this meeting will be held as a video conference over ZoomMembers 
 will be sent instructions on how to join the meeting in the week prior to t
 he event.\nJourney of Metals through the Cosmic WebIn her presentation Dr A
 nshu Gupta will focus on how galaxies evolve in conjunction with their chem
 ical evolution.\nHer main focus is to understand how the local environment 
 shapes galaxies as we see them today, from clouds of gas to galaxies like o
 ur Milky Way. She combines observations from the largest ground based teles
 copes with the state-of-the-art cosmological simulations to estimate if gal
 axies living in dense galaxy clusters produce metals faster than galaxies l
 iving in isolation.\nDr Anshu Guptais a postdoctoral fellow at the Universi
 ty of New South Wales, Sydney. She completed her dual bachelor undergraduat
 e and Master of Science degrees in May 2013 at the Indian Institute of Scie
 nce Education and Research, Mohali, India. Her thesis is titled: 3He [II] -
  An alternative probe for Reionization.\nShe did her graduate studies/PhD (
 2018) at Australian National University (ANU), Canberra with Prof Lisa Kewl
 ey and Dr Tiantian Yuan. Her thesis is titled: Chemical evolution of star-f
 orming galaxies in the overdense environment.\nResearch Interests"I am inte
 rested in understanding the origin and evolution of galaxies like our own M
 ilky Way. My primary research focus is in figuring out how galaxies build d
 ifferent elements. I use optical and near-infrared spectroscopic observatio
 ns of galaxies, to understand the evolution of kinematic, chemical and othe
 r inter-stellar medium properties of galaxies over the past 12 billion year
 s.\nIn my work, I try to establishes a direct connection between observatio
 ns and, the state-of-the-art hydrodynamical simulations and theoretical mod
 els, which is essential to fully understand the physics of galaxy formation
  and evolution."\n
X-ALT-DESC;FMTTYPE=text/html:<h2 style="color: #444444; background-color: #f7f7f7;"><span style="backgro
 und-color: #ffff00;">Note that this meeting will be held as a video confere
 nce over Zoom</span></h2><p style="border: none; line-height: 1.5em; color:
  #444444; font-size: 14px; background-color: #f7f7f7;"><span style="backgro
 und-color: #ffff00;">Members will be sent instructions on how to join the m
 eeting in the week prior to the event.</span></p><h2><span style="color: in
 herit;">Journey of Metals through the Cosmic Web</span></h2><p>In her prese
 ntation Dr Anshu Gupta will focus on how galaxies evolve in conjunction wit
 h their chemical evolution.</p><p>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.</p><h2><img src="https://www.sasi.net.
 au/images/Dr_Anshu_Gupta.jpg" alt="Dr Anshu Gupta image" style="margin-righ
 t: 10px; float: left;" />Dr Anshu Gupta</h2><p>is 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.</p><p>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.</p><h4>Resea
 rch Interests</h4><p>"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.</p><p>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."</p>
DTSTAMP:20260621T072516
DTSTART;TZID=Australia/Sydney:20200903T193000
DTEND;TZID=Australia/Sydney:20200903T213000
SEQUENCE:0
TRANSP:OPAQUE
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