Trainee at the European Space Astronomy Center What is it all about? Gustaf Winroth guswi241@student.liu.se Link¨ oping University, Sweden European Space Astronomy Center, Madrid, Spain GW-2007 – p.1/7 The Center • Closest bus stop - 2 km ⇒ Get a ride • Cafeteria, where you eat lunch • Activity Clubs: football, tennis, etc. • Guards requiring ID and ESAC badge the first days GW-2007 – p.2/7 The People • Other Trainees • The Supervisors • The Staff at ESAC GW-2007 – p.3/7 The Concept of the Project The Phases: • Read the documentation and learn the software • Further confine the project with your supervisors • Process the data • Present the results GW-2007 – p.4/7 My Project (1) EPIC-pn can operate in different modes. Energy spectra can be retrieved from each mode. These should coincide, which is not always true. Take a line-rich source such as Cassiopeia A GW-2007 – p.5/7 My Project (2) Differences between the two modes before the correction: Energy Spectra − Cas A Red − FF, Black − Burst w/ no corr. 0.1 1 counts (arb. units) 10 100 ~/caldata/epchain/0412180101/CAS_A_burst.pha ~/caldata/0412180101/Cas_A_FF.pha 1 2 5 channel energy (keV) gwinroth 17−Oct−2006 13:09 GW-2007 – p.6/7 My Project (2) The two spectra after correction: CasA − 0412180101 Red − Full Frame, Green − Burst w/ new corr. 10 1 normalized counts/sec/keV 100 try16/0412180101/CAS_A_burst_newcal16.pha 0412180101/Cas_A_FF.pha 0.1 Simple task ⇒ 6 months of work 1 2 channel energy (keV) 5 gwinroth 13−Nov−2006 13:10 GW-2007 – p.7/7
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