# # # ######################################### # ## ## # ## FUSE Phase 2 Proposal Template ## # ## ## # ## for use in Cycle 4, 4/01/2003 ## # ## ## # ######################################### # # Refer to FUSE Cycle 4 Phase 2 Instructions for complete details. # # Proposal Identification # This Proposal is a STANDARD (SURVEY) program prog_id: title: t_alloc_total: # Ksec t_alloc_orb: # Orbits, for French programs only. # ###################### # ## ## # ## PI Information ## # ## ## # ###################### pi_title: pi_first_name: pi_last_name: pi_affiliation: pi_institution: pi_address: pi_country: pi_phone: pi_fax: pi_email: # ###################### # ## ## # ## LI Information ## # ## ## # ###################### # Optional, if Program PI designates a separate primary contact person. li_title: li_first_name: li_last_name: li_affiliation: li_institution: li_address: li_country: li_phone: li_fax: li_email: # ######################## # ## ## # ## Co-I Information ## # ## ## # ######################## # COI - 1, repeat if necessary for other Co-Is. coi_title: coi_first_name: coi_last_name: coi_institution: coi_country: coi_phone: coi_email: # ############################ # ## ## # ## Proposal Information ## # ## ## # ############################ # # NOTE: Although not required, keeping text block lines to 80 characters # or less will prevent line wraps and improve readability in the # formatted output. # ------------- # | Abstract | # ------------- abstract_text: # ENTER ABSTRACT TEXT HERE. # ---------------- # | Feasibility | # ---------------- feasibility_text: # ENTER FEASIBILITY AND SAFETY DISCUSSION HERE. # ------------------ # | Special Reqs. | # ------------------ spec_req_text: # ENTER DISCUSSION OF SPECIAL REQUIREMENTS KEYWORDS SPECIFIED HERE. # ------------------ # | Support Info. | # ------------------ support_info_text: # ENTER ANY OTHER RELEVANT SUPPORTING INFORMATION HERE. # For targets above the nominal bright limit (1e-10 ergs-1s-1cm-2A-1), # if you have a preferred observational technique, please discuss. # State the wavelength coverage required. See Phase 2 Instructions. # # Object-specific Information # # Note: Keywords are on uncommented lines, terminated with a colon. # ENTER INPUTS TO THE RIGHT OF THE COLON for each relevant keyword, # NOT on the following line. The blank lines below are for readability # only. Comments or example formats are listed above each item (to # prevent line wraps in the electronic submission). After the fact, # comment lines may be deleted if you wish. # # Also, you may add other comment lines at will, so long as each comment # line begins with a pound sign and is <=80 characters in length. However, # any such lines are for YOUR BENEFIT ONLY and are not part of your official # submission. (Only uncommented lines are visible to the Parser and carried # forward into the database.) # # Repeat the following keywords as necessary for each separate target. # Optional keywords may be left blank or dropped entirely. # # ############################ # ## ## # ## Object 1 Information ## # ## ## # ############################ # Object number. Use 1-99. object_number: 1 # Object name from Phase 1 when possible. NO SPACES in target name. object_name: # Numerical object class from listing in Appendix B. object_class: # Object-level special requirement(s): MOVE and/or TOO. object_spec_req: # RA and Dec in J2000. # Use format: 20:31:45.22 and +31:02:01.5 (INCLUDING the colons). ra_j2000: dec_j2000: # Two-letter source type designation: PC, PE, EC, or EE. source_type: # Reference wavelength in Angstroms; e.g., 1032.0. lambda_ref: # Reference flux in cgs units; e.g., 1.2E-12. NO SPACES. flux_lambda_ref: # FWHM of emission line in Angstroms; e.g., 0.5. # Required for PE and EE types. eline_fwhm: # "Flux" per sq. arcsec. Extended sources only (EE and EC). # Example: 3.0E-15 sb_lambda_ref: # Equiv. continuum fluxes at 950, 1050, and 1150 A; e.g., 1.2E-12. # NOTE: For BRIGHT objects (fluxes above the nominal limit of 1e-10) # these MUST be the INTRINSIC fluxes for the TARGET # NO offset or defocused fluxes. See Phase 2 Instructions. flux_950: flux_1050: flux_1150: # Flux accuracy: HIGH, MED, or LOW. See Phase 2 Instructions. flux_accuracy: # V magnitude in magnitudes; e.g., 12.5. # If V magnitude is not applicable to your target, enter 99. v_mag: # Magnitude range (variable sources only). Example: 9.9-13.2. v_range: # Resolution element (for S/N calc.) in Angstroms; e.g., 0.033. resolution_element: # Total expected cts/sec, preferably from Exposure Time Calculator, # Count Rate Tool or simulated spectrum. Provide count rate estimates # appropriate for INTRINSIC source fluxes. expected_ct_rate: # Channel assumption for S/N calculation. See Phase 2 Instructions. # Valid entries are: LIF1, LIF2, SIC1, SIC2, or TOTAL. sig_noise_chan: # Calculated S/N per specified resolution element; e.g., 15. sig_noise: # Spectral type (if appropriate). NO SPACES. # Do NOT enter the FUSE source type designation (e.g., "PE") here. spectral_type: # E(B-V) in magnitudes; e.g., 0.10. color_excess: # Source redshift: Z format or km/s, as appropriate. red_shift: # High proper motion flag. Enter Y if you applied a Proper Motion # correction to the coordinates above. Enter N or leave blank otherwise. high_prop_motion: # Target priority within this program: 1 or 2 for science targets. # Use 4 for offset stars. object_prio: # Phase zero point and period. See Phase 2 instructions. # Only needed for EPHEM observations. phase_zero: phase_period: # # ################################################## # ## ## # ## Object 1 Observation-specific Information ## # ## ## # ################################################## # # Repeat as needed to specify additional observations of a given target. # The `observation_num:' keyword must be first for each new observation. # # As with above, comments and format examples are given preceding each # line. These comments may be deleted if you wish. # Observation number: Use 1-99. # Start with 1 for each new object. # For MON observations, enter 1 TO N, where N is the # total number of observations on the object. observation_num: 1 # Object number of the target for this observation. obs_object_num: # Object number of the offset target, if any. off_object_num: # Instrument mode: HIST or TTAG. instrument_mode: # Aperture for science: LWRS, MDRS, or HIRS. aperture_req: # Observation time in SECONDS; e.g., 20000. NO COMMAS. # NOTE: "per observation" for MON observations. obs_time_req: # Observation-level special requirements: # HOLD, SNAP, SAFTSNP, MON, ROLL, EPHEM, SPATIAL, CONTIG, # CVZ, COORD, FESIMG, FPSPLIT. See Phase 2 Instructions for details. # If you need to specify more than one special requirement, # enter them all on one line with commas between them. obs_spec_req: # If ROLL spec. requirement was specified above, enter # position angle and tolerance in decimal degrees. # Allowed ROLL angles are: aperture_pa +/- pa_tolerance. # Sample inputs: aperture_pa: 25.0 and pa_tolerance: 5.0. aperture_pa: pa_tolerance: # If MON spec. req. was specified above, enter separation # and tolerance on separation. Example: 21.00 and 3.00. mon_t_sep: mon_delta_tsep: # If EPHEM spec. req. was specified above, enter # desired phase (between 0.0 and 1.0) and # phase tolerance. Example: 0.5 and 0.05. phase_desired: phase_delta: # If FESIMG spec. req. was specified above, enter # target position with respect to aperture: IN or OUT. targ_pos: # Duplicate above lines as necessary for additional # targets and/or observations. # End of form.