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GMRT Observing Application
DEADLINE: Wednesday, October 15, 2003
INSTRUCTIONS: Each numbered item must have an entry or N/A or NA
SEND TO: GMRT Time Allocation Committee, NCRA--TIFR,
Post Bag 3, Ganeshkhind, Pune 411 007, INDIA
Email: gtac@ncra.tifr.res.in
Proposal Code:
Received:
(1) Date of preparing this application:
(2) Title of Proposal:
(3) AUTHORS + INSTITUTION Will come to
GMRT?
Email (needed for PI & Co­PIs)
+ Please write the PI's name in CAPITAL LETTERS.
(4) Related previous GMRT proposal number(s):
(5) Contact author Address:
Telephone:
Fax:
(6) If this proposal is intended to support a Ph.D. project, please mention the name of the Ph.D. student, the anticipated year
of completion of the Ph.D. and also include a brief outline of the Ph.D. project in the Scientific Justification:
(7) Scientific Category:
# astrometry, geodesy & techniques, # solar, # propagation, # planetary, # stellar, # pulsar # ISM, # galactic
center, # galactic structure & dynamis (HI), # normal galaxies, # active galaxies, # cosmology
(8) Wavebands 21 cm 50 cm 90 cm 128 cm 200 cm Total
(9) Time requested (hrs) xxx xxx xxx xxx xxx xxx
(10) Type of Observation:
(check all that apply)
# imaging, # point source, # continuum, # solar, # spectroscopy, # pulsar,
# phased array, # Other
(11) ABSTRACT (Please type within this space only.)

(12) Will PI/ Co­PI be present for observations? # Yes # No Data reduction at? # Home # Other
xxxxxx
(13) Help required: # None # Consultation # Friend (extensive help)
(14) Spectroscopy Only: line 1 line 2 line 3 line 4
Transition (HI, OH, etc) --------- --------- --------- ---------
Rest Frequency (MHz) --------- --------- --------- ---------
Velocity (km/s) --------- --------- --------- ---------
Observing frequency (MHz) --------- --------- --------- ---------
Correlator mode --------- --------- --------- ---------
IF bandwidth(s) (MHz) --------- --------- --------- ---------
Hanning smoothing (y/n) --------- --------- --------- ---------
Number of channels per IF --------- --------- --------- ---------
Frequency Resolution (kHz/channel) --------- --------- --------- ---------
Rms noise (mJy/bm, nat. weight., 1 hr) --------- --------- --------- ---------
Rms noise (K, nat. weight., 1 hr) --------- --------- --------- ---------
(15) Number of sources xxx (If more than 10 please attach a list together with LST range(s). If more than 30
sources give only selection criteria and LST range(s).)
(16) NAME Epoch: 1950# 2000# Config­ Band Band­ Total Flux Largest Requ­ Time ъ LST
RA Dec ration + (#cm) width line cont. angular ired requ­ range
hh mm ± xx.x# (MHz) (Jy # ) (Jy) size rms ested
(mJy/
beam) (hrs) (hrs)
+ Please indicate your preference as per the following possibilities:
F All antennas available.
Nxx Only xx antennas required (eg. VLBI, pulsar test/ monitoring)
C00 Central square antennas only
C01 Central Square antennas + 1 st antenna in each arm } Phased Array
A00 Arm antennas only
A01 Arm antennas only with upto 4 antennas from the Central Square
# Flux at the peak of the line.
ъ including the overheads.
Notes to the table (if any):
(17) Dates preferably avoided:
(18) Special requirements of hardware, software, or operating procedures, etc:
. 1 side band (16 MHz) # or, 2 sidebands (32 MHz) #
. Is integration time less than 8s required for extended periods? #
. Specify expected disk space requirement for the project (if more than 10 GBytes):
. Phased array required #
. If pulsar, specify pulsar hardware required:
(19) Please attach a self­contained Scientific Justification not exceeding 1000 words. (Preprints or reprints will
be ignored, unless reporting previous GMRT observations). When your proposal is scheduled, the contents of the
cover sheets become public information (Any supporting pages are for refereeing purpose only).
(20) IMPORTANT: If your proposal(s) for GMRT observations have been scheduled in the past, please attach a
brief status report (not exceeding 150 words) on each such proposal, and attach any preprint/ reprint based on these
GMRT observations.
A sheet giving guidelines to PIs and Co­PIs coming to observe with the GMRT is enclosed.