1. Name of program and authors
        Name: Kinetic Sunyaev-Zel'dovich Effect of Galaxy Clusters
        Authors: Naoki Yoshida, Naoshi Sugiyama, Tetsuo Hasegawa

     2. One short paragraph with science goal(s)

        Peculiar velocities of galaxy clusters can be determined
        from measurements of the thermal and kinetic Sunyaev-Zeldovich effects.
        Using a large sample of clusters distributed over a wide range of
        redshift, one can infer the time evolution of the cosmic velocity
        field of which the growth factor is a sensitive measure of
        cosmological parameters. In particular a systematic survey
        seves as an excellent method of determining the so-called
        equation of state of the dark energy.


     3. Number of sources (e.g., 1 deep field of 4'x4', 50 YSO's,
                                300 T Tauri stars with disks, ...; do NOT
                                list individual sources or your "pet object",
                                except in special cases like LMC, Cen A, HDFS)

	1' fields for 30 clusters

     4. Coordinates:

        4.1. Rough RA and DEC (e.g., 30 sources in Taurus, 30 in Oph, 20 in Cha,
                               30 in Lupus)

		(uniformly distributed over the sky)

        4.2. Moving target: no

        4.3. Time critical: no


     5. Spatial scales:

        5.1. Angular resolution (arcsec): 1

        5.2. Range of spatial scales/FOV (arcsec): 60

		(single field for Band 3, small mosaic for Band 6)

        5.3. Single dish total power data: yes

        5.4. ACA: yes

        5.5. Subarrays: no


     6. Frequencies:

        6.1. Receiver band: Band 3, 6

		(220 GHz is essential to remove foreground/background)

        6.2. Lines and Frequencies (GHz): 90 and 220 GHz
             (approximate; do NOT go into detail of
             correlator set-up but indicate whether multi-line or single line;
             apply redshift correction yourself; for multi-line observations
             in a single band requiring different frequency settings,
             indicate e.g. "3 frequency settings in Band 7" without specifying
             each frequency (or give dummies: 340., 350., 360. GHz).
             For projects
             of high-z sources with a range of redshifts, specify e.g.
             "6 frequency settings in Band 3". Apply redshift correction
             yourself)

        6.3. Spectral resolution (km/s): not required

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


     7. Continuum flux density:

        7.1. Typical value (Jy): 0.1 mJy/beam
             (take average value of set of objects)
             (optional: provide range of fluxes for set of objects)

        7.2. Required continuum rms (Jy or K): 0.01 mJy/beam

        7.3. Dynamic range within image: 10
             (from 7.1 and 7.2, but also indicate whether e.g. weak objects
              next to bright objects)


     8. Line intensity:

        8.1. Typical value (K or Jy):
             (take average value of set of objects)
             (optional: provide range of values for set of objects)

        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):

         30 x 0.7 hours for Band 3
	30 x 10 hours for Band 6 mosaic

     11. Total integration time for program (hr):

         321 hours

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

***********************************************************************

Review Pierre Cox: It seems to me that these programmes could be
merged in one programme since part of the information in 1.4.2 will be
available in 1.4.1.  What is the rationale behind the number of
clusters? Time estimates are correct.

Review Chris Carilli: similar to 1.4.1.