Presentation is loading. Please wait.

Presentation is loading. Please wait.

Robbie Auld1 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Simulated HI observations Robbie Auld Cardiff University collaborating.

Similar presentations


Presentation on theme: "Robbie Auld1 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Simulated HI observations Robbie Auld Cardiff University collaborating."— Presentation transcript:

1 Robbie Auld1 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Simulated HI observations Robbie Auld Cardiff University collaborating with Oxford SKADS team

2 Robbie Auld2 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Outline Description of the data pipeline Sky simulation (SEX)‏ Telescope Simulation Detection Technique Comparisons: HIPASS vs. SEX dN/dz – SEX vs. SAX Future THINGS: IC 2574

3 Robbie Auld3 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Data Pipeline Cleaned datacube Web query Sky model SKA simulator ParselTongue script (HRK) that uses AIPS routines. Includes: antenna Tsys, antenna layout, gain factors, integration time per visibility, total observation time Corrupted cube Source Finder S 3 simulation (RW & FL) Query generated via the web interface, source list and datacube generated locally with S 3 Tools. Duchamp source finder package (ATNF)‏

4 Robbie Auld4 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Resulting datacube Filled UV plane!

5 Robbie Auld5 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Source detector: Duchamp Locates sets of contiguous voxels (3D pixels) above some threshold. Threshold determination:  Manual (absolute value / S/N value)‏  Automatic (False Discovery Rate method)‏ Enhancement  Spectral smoothing (Hanning)‏  Spatial smoothing (Gaussian convolution)‏  A trous (wavelet procedure)‏ Voxels above threshold are flagged, merging algorithm rejects multiple detections

6 Robbie Auld6 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Duchamp output Postscript file of all detections VO compatible catalogue file

7 Robbie Auld7 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Comparisons with HIPASS

8 Robbie Auld8 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SEX shortcomings HIMF (0 < z < 0.1)‏ Wilman et al. 2008

9 Robbie Auld9 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SEX vs. SAX: dn/dz Abdalla & Rawlings (2005)‏ Diamonds – SAX Stars – SEX SEX differential number counts too low.

10 Robbie Auld10 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Future THINGS: IC 2574 Integrated intensityVelocity Field Explore effects of different array configurations with the galaxy in the local neighbourhood and then try moving it further away.


Download ppt "Robbie Auld1 Simulated HI Observations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Simulated HI observations Robbie Auld Cardiff University collaborating."

Similar presentations


Ads by Google