Skills, Tools and Experience
Software and Programming
Python
- For most of my data analysis I use Python and a multitude of packages,
including Astropy, Pandas, Keras with Tensorflow, Numpy, Scipy, and Scikit-Learn
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For interactive, exploration analysis I use Jupyter notebooks and for
automation of tasks I use scripts.
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To demonstrate th access of Virtual Observatory services and archives with
Python, I have created a set of
Jupyter notebooks with my
colleague Ada Nebot.
Astronomical Data Reduction Software
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very experienced: Miriad
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experienced: IRAF and CASA
Virtual Observatory-aware Software
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very experienced: Aladin, Topcat, DS9
Languages
German (native), English (C2), French (B1), Spanish (A1)
Telescope Proposals and Observing Experience
SKA precursors and pathfinders
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Lead of the HI specific angular momentum project in
the MALS survey on MeerKAT
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Member of the
MIGHTEE-HI
science team
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Member of the WALLABY science team
ALMA ACA array, Chajnantor (CHL)
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PI of a project to map CO in HI-rich galaxies (observed, analysis ongoing )
Australian Telescope Compact Array (ATCA),
Narrabri, (AUS)
- Co-Investigator of multiple projects mapping the HI
content of local galaxies:
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A large observing program to map the atomic hydrogen in HI-rich galaxies. (PI: V. Kilborn)
The data are the foundation of my PhD thesis and are published in
Lutz et al. (2018). Data cubes
can be found in
VizieR.
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A project with the ATCA to map the atomic
hydrogen in gas poor galaxies. (PI: V. Kilborn). Results are published in
Murugeshan et al. (2019).
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The Lord of the Rings:
a large project with the ATCA to map the atomic
hydrogen in gas poor galaxies. (PI: C. Murugeshan)
- Observing with the ATCA for more than 300h
- Supporting continuum and spectral line
observations at wavelengths of 16cm, 4cm, 15mm,
7mm and 4mm as the Duty Astronomer
IRAM 30m single dish, Pico Veleda, (ESP)
- 30h to observe the mm continuum emission of NGC4214 with
the NIKA2 camera, observations are queued (PI: K. Lutz)
- 60h of observations of the CO(1-0) and CO(2-1)
mission line spectra in local galaxies for the
xGASS /
xCOLDGASS project (see
Saintonge et al. (2017))
VLA, New Mexico (USA)
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PI of a project to map the HI and L-band continuum in the NGC1052 group,
observations are ongoing
WiFeS IFU, 2.3m ANU telescope, Siding
Spring Observatory, (AUS)
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PI of a project mapping the gas-phase metallicity of local galaxies (18 nights
granted), results are published in
Lutz et al. (2020)
Dark Energy Camera (DECam), CTIO
Victor-Blanco 4m Telescope, Cerro Tololo, (CHL)
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PI of a project for deep imaging of local galaxies
and their environment (2 Nights granted)
EFOSC2 spectrograph, ESO New
Technology Telescope (NTT), La Silla, (CHL)
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5 nights of observations of optical longslit
spectra of local galaxies for the
xGASS /
xCOLDGASS projects (Lutz et al. submitted)