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This project aims to develop software tools for accurate background subtraction and spectrophotometry of point sources in crowded fields. Key tasks include the collection of test data, testing of point spread functions (PSFs), and evaluation of observational strategies. Collaboration between teams from AIP, ESO, MIL, and CAM will facilitate data analysis and software distribution. Milestones include initial observations and data workshops, leading to the final software release targeted for Q4 2005. This research is integral to understanding stellar populations, high-redshift galaxies, and gravitational lensing.
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Task 2.4 Crowded Field 3D Spectroscopy : • goals: • “to implement software tools for accurate background subtraction and spectrophotometry of point sources in crowded fields. • tasks and subtasks • collection of test data • testing PSFs • experimental stage • link to Task 1.2: Resolved stellar populations • link to Task 1.6: High redshift galaxies • link to Task 1.2: Graviational lensing • collect software being produced during research projects • coordination between groups - distribution • participating teams • AIP, ESO, MIL, CAM
attaching people to the tasks • AIP: Martin Roth, Thomas Becker, Lise Christensen, postdoc n.n., • Lutz Wisotzki, Knud Jahnke • CAM: • DUR: • ESO: • LEI: • MAR: • MIL: • tentative timeline: • collection of test data: Q3 … Q4-2004 • first observations: August - September 2002, Calar Alto • other telescopes: ? • first results: Q4-2003 • Version(s) 1.0 Q4-2004
milestones • Data Analysis Workshop, December 2004 (?) • Conference, Q1 2005 (?) • Euro3D Software Distribution, Q4-2005 • coordination within the RTN sub-groups • T.B.D. • status and availability of instruments • T.B.D. • observing strategy • understanding PSF properties • developing techniques at 4m-class telescopes • application to 8m-class telescopes • Publications • %