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UID:a96548175379fb20cfd5ef36f567678d
CATEGORIES:Guest Speaker Night
CREATED:20151103T111653
SUMMARY:Special Guest Speaker - Sue Knight
LOCATION:Green Point Observatory
DESCRIPTION:The Search for Cool Companions Around White Dwarf Stars\nSue KnightSue Knig
 ht has been a member of SASI since 1998. She was actively involved as the s
 ociety’s web administrator and Committee member. Sue also arranged the mont
 hly Guest Speaker talks, participated as a volunteer at the annual Open Nig
 hts and has written several articles for the society’s journal.\nAs an Info
 rmation Technology specialist for many years, Sue decided to change career 
 direction, after attending several astronomy conferences worldwide. She com
 pleted studies toward a Bachelor of Science degree at Macquarie University 
 in 2011 and is finalizing the next stage of her studies at Leicester Univer
 sity in the UK. Her research was focused on the search of companions to whi
 te dwarf stars in the infrared regime using Spitzer Telescope data.\nSue is
  an enthusiastic traveller and photographer as well as an avid reader of sc
 ience fiction novels.\nWe're looking forward to hear about Sue's research:\
 nThe Search for Substellar Common Proper Motion Companions to White DwarfsA
  large sample of white dwarfs within our solar neighbourhood has been exami
 ned to search for resolved common proper motion companions. The luminosity 
 of these white dwarfs make them ideal candidates for detecting low mass obj
 ects such as brown dwarfs and gas giant planets. Ultra cool brown dwarfs ar
 e particularly interesting due to their scarcity and they provide a crucial
  link between the colder gas giant planets and hotter T spectral type brown
  dwarfs. Furthermore, searching for brown dwarfs can also place constraints
  on the frequency of planetary systems around white dwarf progenitors. They
  also offer a unique opportunity to test properties predicted for them by a
 tmospheric models. I discuss my research and findings on the search for the
 se widely separated companions using data from the Spitzer Telescope data a
 s well the difficulty in distinguishing between brown dwarfs and extrasolar
  planets to date.
X-ALT-DESC;FMTTYPE=text/html:<p><span style="color: inherit; font-family: 'Helvetica Neue', Helvetica, A
 rial, sans-serif; font-size: 35px; line-height: 1.1;">The Search for Cool C
 ompanions Around White Dwarf Stars</span></p><h3>Sue Knight</h3><p><img src
 ="https://sasi.net.au/images/articles/Sue_Knight.jpg" alt="Sue Knight" widt
 h="466" height="262" style="margin-right: 10px; float: left;" />Sue Knight 
 has been a member of SASI since 1998. She was actively involved as the soci
 ety&rsquo;s web administrator and Committee member. Sue also arranged the m
 onthly Guest Speaker talks, participated as a volunteer at the annual Open 
 Nights and has written several articles for the society&rsquo;s journal.</p
 ><p>As an Information Technology specialist for many years, Sue decided to 
 change career direction, after attending several astronomy conferences worl
 dwide. She completed studies toward a Bachelor of Science degree at Macquar
 ie University in 2011 and is finalizing the next stage of her studies at Le
 icester University in the UK. Her research was focused on the search of com
 panions to white dwarf stars in the infrared regime using Spitzer Telescope
  data.</p><p>Sue is an enthusiastic traveller and photographer as well as a
 n avid reader of science fiction novels.</p><p>We're looking forward to hea
 r about Sue's research:</p><h4 style="text-align: left;"><span style="color
 : inherit; line-height: 1.1;"></span></h4><h4 style="text-align: left;">The
  Search for Substellar Common Proper Motion Companions to White Dwarfs</h4>
 <div style="text-align: left;">A large sample of white dwarfs within our so
 lar neighbourhood has been examined to search for resolved common proper mo
 tion companions. The luminosity of these white dwarfs make them ideal candi
 dates for detecting low mass objects such as brown dwarfs and gas giant pla
 nets.</div><div style="text-align: left;"> </div><div style="text-align: le
 ft;">Ultra cool brown dwarfs are particularly interesting due to their scar
 city and they provide a crucial link between the colder gas giant planets a
 nd hotter T spectral type brown dwarfs.</div><div style="text-align: left;"
 > </div><div style="text-align: left;">Furthermore, searching for brown dwa
 rfs can also place constraints on the frequency of planetary systems around
  white dwarf progenitors. They also offer a unique opportunity to test prop
 erties predicted for them by atmospheric models.</div><div style="text-alig
 n: left;"> </div><div style="text-align: left;">I discuss my research and f
 indings on the search for these widely separated companions using data from
  the Spitzer Telescope data as well the difficulty in distinguishing betwee
 n brown dwarfs and extrasolar planets to date.</div>
DTSTAMP:20260717T023404
DTSTART;TZID=Australia/Sydney:20151210T193000
DTEND;TZID=Australia/Sydney:20151210T213000
SEQUENCE:0
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