Title  GRB environment 
Pi     
Time   300 hrs

11. Name of program and authors:  GRB environment

   2. One short paragraph with science goal(s):

Gamma ray bursts are thought to originate with the explosion of
massive stars in regions of prodigious star forming activity at
moderate to large distances.  This program seeks to survey the regions
of a number of gamma ray burst sources to characterize the infrared
emission associated with their hosts.  The resulting catalog will help
to assess whether the paradigm for GRBs is valid.

   3. Number of sources: 300 GRB positions

   4. Coordinates:  

      4.1. Rough RA and DEC All sky.

      4.2. Moving target: yes/no  (e.g. comet, planet, ...)  no

      4.3. Time critical: yes/no  (e.g. SN, GRB, ...)  no, the survey is post GRB


   5. Spatial scales:

      5.1. Angular resolution (arcsec): 1"

      5.2. Range of spatial scales/FOV (arcsec):           
           (optional: indicate whether single-field, small mosaic, 
            wide-field mosaic...)  single field

      5.3. Single dish total power data: no

      5.4. ACA: no

      5.5. Subarrays: no


   6. Frequencies:

      6.1. Receiver band: Band   7 and 9

      6.2. Lines and Frequencies (GHz):  280 GHz, 345 GHz 650 GHz
          
 
      6.3. Spectral resolution (km/s): continuum

      6.4. Bandwidth or spectral coverage (km/s or GHz): 8 GHz 


   7. Continuum flux density:

      7.1. Typical value (Jy):  .05 
          
           
      7.2. Required continuum rms (Jy or K): .03 mJy (1.1 mm); .25 mJy (.45 mm)

      7.3. Dynamic range within image:    >5              
          

   8. Line intensity:

      8.1. Typical value (K or Jy):
          

      8.2. Required rms per channel (K or Jy):

      8.3. Spectral dynamic range:              


   9. Polarization:  no  (optional)

      9.1. Required Stokes
   
      9.2. Total polarized flux density (Jy)

      9.3. Required polarization rms and/or dynamic range

      9.4. Polarization fidelity


   10. Integration time for each observing mode/receiver setting (hr): 20 mins

   11. Total integration time for program (hr): 300

   12. Comments on observing strategy (e.g. line surveys, Target of
       Opportunity, Sun, ...): (optional)

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Review Chris Carilli: OK