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Junior career | Senior career | Orpo equivalent | SS equivalent |
---|---|---|---|
Kriminalassistentanwärter | Wachtmeister | Unterscharführer | |
apl. Kriminalassistent | Oberwachtmeister | Scharführer | |
Kriminalassistent | Revieroberwachtmeister | Oberscharführer | |
Kriminaloberassistent | Hauptwachtmeister | Hauptscharführer | |
Kriminalsekretär | Meister | Sturmscharführer | |
Kriminalobersekretär | Hilfskriminalkommissar Kriminalkommissar auf Probe apl. Kriminalkommissar |
Leutnant | Untersturmführer |
Kriminalinspektor | Kriminalkommissar with less than three years in that rank | Oberleutnant | Obersturmführer |
Kriminalkommissar Kriminalrat with less than three years in that rank |
Hauptmann | Hauptsturmführer | |
Kriminalrat Kriminaldirektor Regierungs- und Kriminalrat |
Major | Sturmbannführer | |
Oberregierungs- u. Kriminalrat | Oberstleutnant | Obersturmbannführer | |
Regierungs- u. Kriminaldirektor Reichskriminaldirektor |
Oberst | Standartenführer |
Last Update | |
Created | 29 January 15 |
Looped Audio | No |
Audio Files Included | WAV |
Bit Rate | 320 kbps |
Sample Rate | 16-Bit Stereo, 44.1 kHz |
Main Track Length | 0:01 |
Number of Sound Effect Clips | 1 |
P.R.O. Affiliated | Canada SOCAN |
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Fig. #8201;5 Each row shows a grey-scale image of the Spitzer 3.6 #8201; #956;m observations, superimposed with grey contours indicating the 1.4 #8201;GHz observations and black contours showing the 4.8 #8201;GHz (left panel) and 8.6 #8201;GHz (middle panel) observations. The IFRS are always the sources at the image centres. Contours start at 3 #963; and increase by factors of 2. The 1.4 #8201;GHz restoring beam and the 4.8 #8201;GHz/8.6 #8201;GHz restoring beams, which are the same size, are indicated with ellipses in the lower left corners of the images. The right panel shows the flux density measurements available for a source and 3 #963; upper limits where no detection was made (indicated with arrows). The solid line indicates the best available spectral index, and dashed lines indicate a power-law with an index 1 #963; larger and 1 #963; smaller than determined by the data. We note that all sources have a signal-to-noise ratio of more than 9 in the 1.4 #8201;GHz observations, so there is no doubt that they are real sources and not spurious. |
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