Images selected by ASAC in 2007 for

  1. astronomical relevance
  2. high S/N dynamic range (>1000)
  3. high spatial dynamic range (>100)

All model images were modified to have 1024 x 1024 pixels and 0.01" pixels.

Protoplanetary Disk

The original image was calculated in a numerical simulation by S. Wolf.
The model image ( SWOLF.MODEL) is 256 x 256 in size. It represents a protoplanetary disk as simulated by Wolf and D'Angelo 2005. It simulates a M_planet = 1 M_jup around a star of M_star = 0.5 Msun at a Distance = 50pc. A FITS model image optimized for CASA use is available.

Protostellar Cluster

cluster.gif Model protostellar cluster, provided by K. Tatematsu. The model image (not yet found; will be at cluster.fits) has been used in previous ALMA simulations.

M51 in H alpha

m51.gif This is a continuum subtracted H alpha image of the nearby galaxy M51 (NGC 5194 -- provided by D. Thilker at NRAO). This H alpha image should be a reasonable representation of the atomic FIR lines and other tracers of massive star formation, and it may be reasonable model for other molecular transitions as well. Shown in logarithmic stretch. Image dynamic range is over 10000.
The model image ( M51HA.MODEL) is 512 x 512 pixels in size. Large negative pixels resulting from subtraction of saturated stars have been blanked with 0's.


m31HII.jpg This HII region in M31 displays complex extended structure.
A small model FITS image ( M31_128.FITS)is available. It was 1024 x 1024 pixels in size and had a pixel scale of 0.01 arcsecond for the 3 km array simulation.

HCO+ J=4-3 line emission in a protostellar envelope

HCO 4-3 60.jpg This is a model of the HCO+ 4-3 line emission in a protostellar envelope provided by M. Hogerheijde. The model is viewed at inclination 60 degrees.
The model image ( HCO+_4-3_60.FITS) is 560 x 560 pixels in size. Obvious image boundary structures are also included, but we will treat it like any other structure in the image.

---+ A Few more interesting ones

3c288.png3c288 radio galaxy 3c288.fits - imaging the bright jet and the large lobes can be nontrivial
30dor.png30Dor Spitzer IRAC 8um image from SAGE 30dor.fits
g41.pngVGPS cm continuum image with interesting range of structures g41.1-0.3.b.fits
Einstein.jpgEinstein's face fits file Einstein.fits
Topic attachments
I Attachment Action Size Date Who Comment
30dor.fitsfits 30dor.fits manage 253 K 2015-03-24 - 12:43 JimBraatz 32 bit version
30dor.pngpng 30dor.png manage 43 K 2009-06-02 - 22:53 RemyIndebetouw  
3c288.fitsfits 3c288.fits manage 284 K 2009-06-02 - 22:52 RemyIndebetouw  
3c288.pngpng 3c288.png manage 85 K 2009-06-02 - 22:51 RemyIndebetouw  
Einstein.fitsfits Einstein.fits manage 354 K 2015-03-17 - 12:23 JimBraatz 32 bit version
Einstein.jpgjpg Einstein.jpg manage 11 K 2011-05-18 - 09:27 AmyKimball  
HCO_4-3_60.jpgjpg HCO_4-3_60.jpg manage 57 K 2009-06-01 - 12:12 RemyIndebetouw  
cluster.gifgif cluster.gif manage 11 K 2009-06-01 - 12:19 RemyIndebetouw  
g41.1-0.3.b.fitsfits g41.1-0.3.b.fits manage 604 K 2009-06-02 - 22:56 RemyIndebetouw  
g41.pngpng g41.png manage 83 K 2009-06-02 - 22:54 RemyIndebetouw  
m31HII.jpgjpg m31HII.jpg manage 30 K 2009-06-01 - 12:19 RemyIndebetouw  
m51.gifgif m51.gif manage 114 K 2009-06-01 - 12:20 RemyIndebetouw  
Topic revision: r7 - 2015-03-24, JimBraatz
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