Material for VLA Expansion HI Working Group

J. Hibbard, chair

Members: C. Carilli, J. Gallimore, J. van Gorkom, F. Owen, E. Richards, M. Rupen, M. Thornley, M. Verheijen, M. Yun

1. For Michael (5/6/99)
2. MPR, GET THIS: Final vugraphs from Michele
3. Simulated Images. texp=2700 hrs, Tsys=28 K, effic=0.55, BW=500 MHz
   
   • Min Yun's Radio Continuum Simulation
   • Eric Richards' Radio Continuum Simulation:
     4'x4' region (1/60th FOV),
     HDF-sized region (1/130th FOV)
   • Jack Gallimore's simulated HI field (using synthetic disks)
   • HI Simulations from JEH (taking actual HI moment maps and simulating higher redshift observations):
     • tar file of iraf scripts for producing the following figures
     • Various objects w/artificial noise added (Ho=75, qo=0.1)
       A-array (FWHM @ 1.4 GHz = 1.6") vs B-array (FWHM @ 1.4 GHz = 4.8")
       Note: these are S/N maps, NOT integrated flux
       1. NGC 4038/9 comparison, A-array, B-array
       2. Arp 299 comparison, A-array, B-array
       3. NGC 7252 comparison, A-array, B-array
       4. Arp 295 system comparison, A-array, B-array
       5. M81 group comparison, A-array, B-array
       6. NGC 891 comparison, A-array, B-array
       7. NGC 1058 comparison, A-array, B-array
       8. NGC 3726 comparison, A-array, B-array
       9. NGC 3893 comparison, A-array, B-array
       10. NGC 3938 comparison, A-array, B-array
       11. NGC 4088 comparison, A-array, B-array
       12. NGC 4183 comparison, A-array, B-array
       13. NGC 4565 comparison, A-array, B-array
       14. NGC 7814 comparison, A-array, B-array
     • Cosmology trade study with NGC 4038/9 ("The Antennae") (A-array):
       1. comparison,
       2. Ho=75, qo=0.1
       3. Ho=75, qo=0.5
       4. Ho=50, qo=0.5
     • MPR, GET THIS: Exposure time trade study with NGC 4038/9 (B-array)
     • NGC 4038/9 No noise, no threshold Ho=75, qo=0.1, A-array
4. Calculations:
   1. EVLA/GMRT L-band comparison (data)
   2. MPR, GET THIS: EVLA/GMRT L-band comparison (table)
   3. tarfile of programs + plots
   4. Freq(z)
   5. rms(z) dW=20 km/s
   6. rms(z) dW=50 km/s
   7. arcsec/10kpc (z)
   8. dVol(z) {Omega cosmologies}
   9. dVol(z) {Ho cosmologies}
   10. Volume(z) {Ho cosmologies}
   11. MHI(z) {Tsys}
   12. MHI(z) {cosmologies}
   13. MHI(z) {cosmolgoies}{tidal,dwarf,spiral}
   14. MHI(z) constant vs variable linewidth
   15. MHI(z) dW=150km/s vs dW=f(MHI)
   16. dNgal(z)/dz dW=const {cosmologies}{tidal,dwarf,spiral}
   17. SUMgal(z)
   18. dNgal(z)/dz dW=f(MHI) {cosmologies}{tidal,dwarf,spiral}
   19. SUMgal2(z)
   20. NHI all
   21. NHI A,B
   22. NHI B
   23. NHI C,D
   24. NHI D
   25. NHI E
   26. log[SFR(z)] as function of cosmology S/N=8
5. Other Plots:
   1. Zwaan etal HI Mass Function 1997, ApJ, 490, 173
   2. Schneider etal HI Mass Function astro-ph/9810349
   3. NVSS Mosaicing 1998, AJ, 115, 1693
   4. 1.4 GHz Source counts from Ciliegi etal 1998
   5. 1.4 GHz dN/dS from Eric
   6. 1.4 GHz luminosity function, Serjeant etal 1998 MNRAS (astro-ph/9808259)
   7. SFR luminosity function, Cram 1998 ApJL, 506, L6
   8. SFR luminosity function, Richards 1998
   9. Lband below 1250 MHz from Marc

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