Day 1 – Wednesday, 26 March
0815 - 0850 Registration Huxley
Building Forecourt
Session I: Welcome, Introduction
and GMT Overview Chair:
Penny Sackett
0900 - 0910 Prof
Aidan Byrne, Dean, College of Science, ANU Opening
of meeting
0910 - 0920 Harvey
Butcher, RSAA Director, ANU Welcoming
remarks
0920 - 0930 Wendy
Freedman, Chair, GMT Board Welcoming
remarks
0930 - 0940 Warrick
Couch, Swinburne University Goals
and scope of meeting
0940 - 1005 Matt
Johns, GMTO Overview
of GMT Project
1005 - 1030 Peter
McGregor, RSAA, ANU Overview
of GMT instruments/AO
1030 - 1100 Morning
tea & further registration
Session II: Brown
Dwarfs, Protostellar Disks and Exoplanets Chair:
Wendy Freedman
1100 - 1145 Penny
Sackett, RSAA, ANU Giant Steps: Planetary
Science in the GMT Era (Overview)
1145 - 1210 Chris
Tinney, UNSW What
Exoplanet and Brown Dwarf Science is the GMT good
for?
1210 - 1235 Roger
Angel, Univ of Az AO
methods and exoplanet searches
1235 - 1300 Andy
Szentgyorgyi, CfA The
GMT-CfA Large Earth Finder (G-CLEF): A high stability
optical
echelle spectrograph for exoplanet and cosmology
research
1300 - 1410 Lunch
Session III: Stellar Astrophysics
and Galactic Structure Chair:
Gary Da Costa
1410 - 1455 Ken
Freeman, RSAA, ANU Galactic Science with the
GMT (Overview)
1455 - 1520 Chris
Sneden, Univ of Tx The
First Stars and the GMT
1520 - 1550 Afternoon
Tea
1550 - 1615 Y.-W.
Lee, Yonsei Univ Globular
Clusters with multiple populations as remaining
cores
of primordial Galaxy building blocks
1615 - 1645 David
Lambert, Univ of Tx Stellar
astrophysics and galactic structure with GMTNIRS
1645 - 1710 Peter
Cottrell, Univ of Cant Element abundance
variations in globular clusters
1710 - 1730 Lucas
Macri, NOAO, Tx A&M Cepheids and
the distance scale with GMT
1900 - 2200 Conference
Dinner Teatro Vivaldi (ANU Arts Centre
Building, University Avenue)
Day 2 – Thursday, 27 March
Session III: Continued Chair:
Steve Shectman
0845 - 0910 Joss
Bland-Hawthorn, USyd Near
field cosmology
0910 - 0935 M.-G.
Lee, Seoul Nat Univ Stellar
Populations and Galaxy Formation in the GMT era
0935 - 1020 Mike
Meyer, Univ of Az From
GouldŐs Belt to the Local Group: Star and Planet
formation
with the GMT (Overview)
1020 - 1050 Morning
tea
Day 2 – Thursday, 27 March Continued
Session IV: Galaxies,
Cosmology and the Distant Universe Chair:
Darren DePoy
1050 - 1135 Matthew
Colless, AAO Cosmology and the Distant
Universe (Overview),
1135 - 1200 Michael
Dopita, RSAA, ANU Starbursts
and AGN: Probing Feedback in Galaxy Formation
with
GMT
1210 - 1230 Travel
to Mt Stromlo Observatory
1230 - 1330 Barbeque
lunch at Mt Stromlo Observatory
1400 - 1700 Visit
to Tidbinbilla Nature Reserve
1930 - 2030 Bob
Kirshner, CfA Public
lecture, Finkel Lecture Theatre
Day 3 – Friday, 28 March
Session IV: Continued Chair:
Warrick Couch
0845 - 0925 T.
Padmanabhan, IUCAA Progress
in Cosmology: Rumours and Reality (Overview)
0925 - 0950 Dawn
Erb, CfA Observing
Distant Galaxies with the GMT
0950 - 1015 J.
Lee, Seoul Nat Univ Cosmic
voids as a new cosmological probe
1015 - 1040 Nick
Suntzeff, Tx A&M Exploding
stars in the early universe [not given]
1040 - 1110 Morning
tea
Session IV: Continued Chair:
Bob Kirshner
1110 - 1135 Karl
Glazebrook, Swinburne Studies
of massive high-redshift galaxies with GMT
1135 - 1200 Ram
Sagar, ARIES, India Relevance
of GMT for GRB studies
1200 - 1225 Michael
Murphy, Swinburne Varying
fundamental constants? Next generation, high-
precision
echelle spectroscopy
1225 - 1335 Lunch
Session IV: Continued Chair:
Bob Kirshner
1335 - 1400 Stuart
Wyithe, UMelb The
photon budget for reionization
1400 - 1425 Andy
Bunker, AAO Galaxies
within the reionization epoch: exploring the high
redshift
universe with GMT
1425 - 1455 Afternoon
tea
Session V: Synergy
with Other Facilities Chair:
Harvey Butcher
1455 - 1520 Jochen
Liske, ESO Status
of E-ELT project and its science case
1520 - 1545 Paul
Ho, CfA Submillimeter
studies of star and planet formation
1545 - 1610 Xiaohui
Fan, Univ of Az Joint
Scientific Opportunities with the GMT and ALMA
1610 - 1635 Elaine
Sadler, USyd SKA
and GMT
1635 - 1655 Pat
McCarthy, OCIW Meeting
summary and a look to the future