Dr Jesse van de Sande

Dr Jesse van de Sande

Lecturer
Science
School of Physics

I am a Lecturer in Astrophysics at the School of Physics, at the University of New South Wales. My passion lies in sharing knowledge and mentoring and I enjoy lecturing and public speaking.

My research interests focus on understanding how our Milky Way and more massive galaxies form, evolve, and die. I have expertise in utilising integral field and near-infrared spectroscopic data to determine galaxies' stellar kinematic properties. I am currently involved in several large galaxy surveys:

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E-mail
j.van_de_sande@unsw.edu.au
Location
Rm 127 Level 1 Old Main Building School of Physics

ADACS Merit Allocation Program  - Software development
ASTRO3D - distinguished visitor grant
The Hunstead Fund for Astrophysics - visitor grant
ASTRO3D - conference grant
The Hunstead Fund for Astrophysics - conference grant
AAL - Keck Observing travel funding
Leids Kerkhoven-Bosscha (LKBF) - travel grants
Leids Universiteits Fonds (LUF) - 1st price best travel story
Leids Universiteits Fonds (LUF) - international travel grant

2020-2022 ARC - Discovery Early Career Researcher Award (DECRA)

1) GECKOS (https://www.geckos.org.au/) is an IFS survey of 35 nearby edge-on Milky Way-like galaxies, going out to larger radius, deeper, and with higher spatial resolution than existing IFS nearby galaxy surveys. I am the Principal Investigator of the GECKOS ESO VLT/MUSE large program, and also lead the GECKOS team. The main goal of the survey is to determine the interplay between internal and external processes that shape disk galaxies with similar mass as our Galaxy.

2) The SAMI Galaxy Survey successfully created a large 3D integral-field spectroscopic dataset of 3000 galaxies across a large range of mass and environment. Since 2016 I have been leading the stellar kinematic workgroup producing high-quality stellar kinematic data products. My most recent work answered one of the fundamental questions from the SAMI science case: how do mass and environment impact the kinematic properties of galaxies?

3) Hector is the next major dark-time instrument for the AAT and is a multi-object integral-field-unit spectrograph aimed at obtaining a low-redshift galaxy survey of up to 15,000 galaxies. Within the Hector Galaxy Survey I have been leading the stellar kinematic working group. Due to its spectral resolution, Hector will revolutionise our ability to measure higher-order kinematic signatures that offer a complementary yet unique insight into the orbital structure of galaxies.

 

 

My Research Supervision

I am (co)supervising three PhD students:

Michelle Ding - UNSW
Susie Tuntipong - University of Sydney
Tomas Rutherford - currently at ESO, Garching, Germany