Tim Schrabback
Universität Innsbruck, University of Bonn, Stanford University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories · Stellar, planetary, and galactic studies
About
In my research I am using weak gravitational lensing as a tool for cosmological and astrophysical investigations. My current major project responsibilities include:
- Speaker and sub-project lead of the new FWF Special Research Area (SFB) Dark UNiverse Explorations
- Euclid: National representative of Austria on the Euclid Collaboration Board. I am also leading four projects at the University of Innsbruck funded by the Austrian Research Promotion Agency (FFG) via the Austrian Space Applications Programme, which are related to the accurate measurement of weak lensing signals in data from ESA's Euclid Mission.
- South Pole Telescope: Lead of the high-redshift weak lensing follow-up campaign
- German eROSITA Consortium: Lead of the high-redshift weak lensing follow-up campaign
Employment
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University of Innsbruck Professor for astrophysics (focus: extragalactic astrophysics)2022 - Present
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University of Bonn Senior research staff (Akademischer Oberrat auf Zeit)2017 - 2022
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University of Bonn Research staff (Akademischer Rat auf Zeit)2011 - 2017
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Stanford University KIPAC Fellow2010 - 2011
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Leiden University Postdoctoral researcher2007 - 2010
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University of Bonn Research assistant (wissenschaftlicher Mitarbeiter)2007 - 2007
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University of Bonn Research assistant (wissenschaftlicher Mitarbeiter)2004 - 2005
Education
- 2004 - 2008
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University of Bonn Diploma1998 - 2004
Projects & Funding
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Dark UNiverse Explorations FWF Austrian Science Fund2026 - 2030
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Weak lensing shear calibration and validation for Euclid's Data Release 2 Österreichische Forschungsförderungsgesellschaft2026 - 2028
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Accurate quantification and correction of member contamination in Euclid weak lensing shear profiles Österreichische Forschungsförderungsgesellschaft2024 - 2027
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Accurate weak lensing measurements with Euclid: Accounting for galaxy substructures and the cluster shear regime Österreichische Forschungsförderungsgesellschaft2023 - 2027
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Weak lensing shear calibration for the Data Release 1 of ESA's Euclid mission Österreichische Forschungsförderungsgesellschaft2022 - 2026
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HST+XMM-Newton gravitational lensing and X-ray analysis of merging SPT galaxy clusters at high redshifts Bundesministerium für Wirtschaft und Energie2021 - 2023
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Deep HST lensing analysis of the most massive known galaxy cluster at redshift z>1: SPT-CLJ2106-5844 Bundesministerium für Wirtschaft und Energie2020 - 2023
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Analysis of new WHT, VLT, and SOAR observations: Confirming new galaxy clusters from Planck & Calibrating the masses of high-redshift SPT clusters via weak gravitational lensing for cosmological investigations Deutsche Forschungsgemeinschaft2019 - 2022
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Constraining the masses of nine SPT-SZ galaxy clusters at redshifts z>1.2 via a weak gravitational lensing analysis of new multi-filter HST observations Bundesministerium für Wirtschaft und Energie2018 - 2021
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Analysis of the weak gravitational lensing effect in new mosaic Hubble Space Telescope observations of the relaxed high-redshift galaxy cluster SPT-Cl J2043-5035 Bundesministerium für Wirtschaft und Energie2016 - 2019
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Cosmological and astrophysical analysis of new Hubble Space Telescope Snapshot gravitational lensing observations for a representative sample of massive high-redshift galaxy clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey Bundesministerium für Wirtschaft und Energie2014 - 2019
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Calibrating SZ Mass Estimates with Weak Lensing: Executing observations with the Magellan Telescope in October 2014 German Research Foundation2014 - 2015
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X-ray and gravitational lensing analysis of two extremely massive galaxy clusters at high redshift Bundesministerium für Wirtschaft und Energie2013 - 2016
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Matter distribution and mass calibration of the most massive galaxy clusters at intermediate and high redshift Bundesministerium für Wirtschaft und Energie2012 - 2015
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PhD Scholarship Studienstiftung des Deutschen Volkes2005 - 2007
Publications (342)
- Euclid Quick Data Release (Q1): XXXVII. Searching for giant gravitational arcs in galaxy clusters with mask region-based convolutional neural networks Save
- Euclid Quick Data Release (Q1): XXXVIII. Euclid spectroscopy of quasars. 1. Identification and redshift determination of 3500 bright quasars Save
- Euclid: A UV-faint quasar in a highly luminous star-forming host galaxy at z ≍ 7.7 Save
- Euclid: Discovery of 31 new quasars at 6.6 < z < 7.8 Save
- Euclid: Field-level inference of primordial non-Gaussianity and cosmic initial conditions Save
- Euclid Quick Data Release (Q1): II. VIS processing and data products Save
- Euclid Quick Data Release (Q1): IX. First visual morphology catalogue Save
- Euclid Quick Data Release (Q1): VI. From spectrograms to spectra: The SIR spectroscopic processing function Save
- Euclid Quick Data Release (Q1): VII. Characteristics and limitations of the spectroscopic measurements Save
- Euclid Quick Data Release (Q1): XII. Quenching precedes bulge formation in dense environments but follows it in the field Save
- Euclid Quick Data Release (Q1): XIII. Exploring galaxy properties with a multi-modal foundation model Save
- Euclid Quick Data Release (Q1): XIV. A first view of the star-forming main sequence in the Euclid Deep Fields Save
- Euclid Quick Data Release (Q1): XIX. First study of red quasars selection Save
- Euclid Quick Data Release (Q1): XV. A probabilistic classification of quenched galaxies Save
- Euclid Quick Data Release (Q1): XVI. Optical and near-infrared identification and classification of point-like X-ray selected sources Save
- Euclid Quick Data Release (Q1): XVII. First Euclid statistical study of galaxy mergers and their connection to active galactic nuclei Save
- Euclid Quick Data Release (Q1): XVIII. First Euclid statistical study of the active galactic nuclei contribution fraction Save
- Euclid Quick Data Release (Q1): XX. The active galaxies of Euclid Save
- Euclid Quick Data Release (Q1): XXI. Active galactic nuclei identification using diffusion-based inpainting of Euclid VIS images Save
- Euclid Quick Data Release (Q1): XXIII. The average far-infrared properties of Euclid-selected star-forming galaxies Save