README CONTENTS The Readme file shall consist of the following fields. 1. Date & Time of delivery 23rd April 2010 17:00 GMT 2. ICC individual to be contacted where problems arise with the delivery (1) Sarah Leeks (RAL) (2) Michael Pohlen (Cardiff) Note: always copy spire@stfc.ac.uk 3. Cycle for which the data being delivered is applicable. Cycle 013 4. Delivery information - names of all files contained in the tar file SPIRE_MC_ASTR_pv78_C013_53_CUS_CAL.xml SPIRE_MC_ASTR_pv78_C013_53_CUS.def SPIRE_AOR_C013_53_CAL.aor SPIRE_AOR_C013_53_ENG.aor SPIRE_CUS_THCP.py SPIRE_Duration.txt SPIRE_Readme_C013_53.txt 5. Cus Script & Calibration files ICC internal configuration control issues (a) Name of ICC mission configuration from which files were exported (for reference purposes only) pvPhase_mconfig_78 (b) Name of the CVS Tag related to this delivery (if relevant) N/A (c) Name of the ICC Database containing this delivery (for reference purposes only) mps_phs_1 (d) HCSS Cus version used when working with these files 1387 6. AOR File issues (a) HSpot, PHS & MPS versions used : Note if you don't use MPS then no need to mention it HSpot 4.4.4 PHS 609 over 1436 (HCSS 2.3.0), MPS 1387, HCSS 2.0.1 (b) Number of AOR files delivered in the .aor file CAL:23 ENG:41 (c) Overall Time Estimation calculated by HSpot - In Hours, Minutes & Seconds CAL: 10h10m46s ENG: 12h05m38s 7. Spacecraft Database issues (a) ICC MIB version applicable to these cus & calibration files SPIRE 4.0.02 PR (b) HPSDB version (if known) that contains this MIB HPSDB_MOC_HERSCH_CCS_issueMOC5_200910261200 (c) OBSM software version on the instrument applicable to this MIB the one currently loaded on the S/C 8. Go-ahead of the ICC CCB (if applicable) N/A 9. SxRs applicable to the updates of the scripts delivered in this release - If there is an ASTR Mission Configuration delivery, then flag the high level SxR which contains the list of SxRs since the last ASTR delivery that affect a released AOT + list other SxRs that are calibration MC specific other sxrs: [SPIRE-2501], [SPIRE-2519] 10. Additional notes (a) Update Information : If this corresponds to an update since the last delivery, explain what the updates consist of e.g. 2 more AORs added. (b) Instructions for the Mission Planners A list with all the solar system objects that are going to be observed. This will include specification of the constraints (if any) that has to be modified in the MPS properties file. Hygiea, Vesta, Hebe, Neptune *INSTRUCTIONS and note on new format* ------------------------------------ All the usual instructions about the min time for using the spectrometer etc are valid as per the scheduling guidelines. We give a heading for each OD (or OD pair) and below it are all observations to be scheduled on that specfied OD (pair) in sections A) B) etc, then we give the corresponding justifications. All of the observations for a sub instrument should be scheduled together in the blocks given below - i.e. where aor titles are given like this (no lines between the aor labels) then they must all be scheduled together and in the order given For example: SPhoto-SmallRep4-Hygiea SPhoto-Point-Rep4-Hygiea SPhoto-Point-Rep4-Hygiea-0001 However when there are empty lines between the AOR labels then these observations can be scheduled independently of each other and they can have observations from other sections ( A) B) etc) interspersed between them. SpirePhotoLargeScanGen-short-fine-scanY-ngc6543 SpirePhotoLargeScanGen-short-fine-scanY-Pi1Gru-1 SpirePhotoLargeScanGen-short-fine-scanY-BetaUMi Observations blocks can be scheduled anywhere in the OD except where specified otherwise below. In addition, please schedule the following observations according to the following instructions. *NEW REDY/STBY AORs for CLONING for Cycle 13 and onwards* -------------------------------------------------------- SpireEngREDYtoPHOT_STBYGen-0000 SpireEngREDYtoPHOT_STBYGen-0000 SpireEngPHOT_STBYtoREDYGen-0000 SpireEngSPEC_STBYtoREDYGen-0000 (these use the new BSM tuning parameters so correct the hick-up with OD341 onwards) [please take the Calibration_cycle13_2 out of the labels before cloning] *Observations for OD 358* ------------------------ Scheduling instructions: Because of the variablity of some of the sources it is important to perform these observations at the time of the other ones. These observations should not be placed directly after the cooler recycle, they should be done at least 8 hours after it. NOTE no PhotoPointJiggle observations should be done before the observations listed here, Hygiea measurements must be the first ones using PhotoPointJiggle on the OD. Observations: SPhoto-SmallRep4-Hygiea SPhoto-Point-Rep4-Hygiea SPhoto-Point-Rep4-Hygiea-0001 SPhoto-SmallRep4-0851+202 SPhoto-Point-Rep4-0851+202 SPhoto-Point-Rep4-0851+202-0001 SPhoto-Point-Rep4-GammaDra SPhoto-SmallRep4-GammaDra SPhoto-Large-Rep4-8x8-GammaDra SPhoto-Point-Rep4-GammaDra-0001 Justifications: 7-pt jiggle observations - repeat of final tests (due to new BSM tuning parameters not being used on OD 341), they should use the new BSM settings as found from the BSM tuning tests (REDY/STBY aors are included to make sure of this). We observe several targets to examine the range suitable for this mode (a faint, intermediate and bright source). The observations are separated into pairs to examine the APE effect. Small maps are also performed as references to compare to. Some observations are also covered by rcal plan AOT section. *Observations for PHOT OD 358/359* --------------------------------- Observations: A) SpirePhotoLargeScanGen-short-fine-scanY-ngc6543 SpirePhotoLargeScanGen-short-fine-scanY-Pi1Gru-1 SpirePhotoLargeScanGen-short-fine-scanY-BetaUMi SpirePhotoLargeScanGen-short-fine-scanY-0537-441 SpirePhotoLargeScanGen-short-fine-scanY-8C0716+714 B) SpirePhoto_Cal_StdLoadCurveGen-DarkSky-PSW-E6 SpirePhotoPcalFlashGen C) SPhoto-Point-Rep4-Hebe SPhoto-SmallRep4-Hebe SPhoto-Large-Rep4-8x8-Hebe SPhoto-Point-Rep4-DarkSky SPhoto-SmallRep4-DarkSky SPhoto-Large-Rep4-8x8-DarkSky SPhoto-Large-Rep4-8x8-Neptune SPhoto-Point-Rep4-Neptune SPhoto-SmallRep4-Neptune Justifications: A) The observations in OD 342 show possible signs for improvment in the SIAM but we need more statistics which we get with these observations. B)Covered by Rcal Plan sections 4.2.1 Detector load curves C) Covered by RCal Plan section 4.2.4 AOTs *OBSERVATIONS for OD 361* ------------------------ Scheduling instructions: when SPIRE is in REDY, most efficient to do in DTCP Observations: SpireEngBsmTuneChopSettingsGen-0000 Justifications: final Tuning observations to optimise parameters (not covered by Rcal plan) *OBSERVATIONS for OD 363* ------------------------ Scheduling instructions: when SPIRE is in REDY AND when SPIRE Cooler has run out , most efficient to do in DTCP Observations: SpirePhoto_Cal_JfetVssTestCGen-0000 SpireSpectro_Cal_JfetVssTestCGen-0000 Justifications: Covered by Rcal Plan sections 4.3.2 Detectors, JFETs and Electronics *Observations for PHOT OD 368/369* ---------------------------------- Observations: A) SpirePhoto_Cal_StdLoadCurveGen-DarkSky-PSW-E6-0001 SpirePhotoPcalFlashGen-0001 B) SPhoto-Point-Rep4-Vesta SPhoto-SmallRep4-Vesta SPhoto-Large-Rep4-8x8-Vesta SPhoto-Point-Rep4-BetaUMi SPhoto-SmallRep4-BetaUMi SPhoto-Large-Rep4-8x8-BetaUMi SPhoto-Point-Rep4-DarkSky-0001 SPhoto-SmallRep4-DarkSky-0001 SPhoto-Large-Rep4-8x8-DarkSky-0001 SPhoto-Large-Rep4-8x8-Neptune-0001 SPhoto-Point-Rep4-Neptune-0001 SPhoto-SmallRep4-Neptune-0001 Justifications: A) Covered by Rcal Plan sections 4.2.1 Detector load curves B) Covered by RCal Plan section 4.2.4 AOTs *OBSERVATIONS for SPEC OD of the cycle* --------------------------------------- Scheduling Instructions: gyro propagation is low prority to have for this observation ONLY in the case that there time for the 1 hour stable attitude that would not otherwise get used for science observations should the 1 hour stable pointing be put in. Observations: A) SpireSpectro_CalGCO_FovMapFpgScan-short-fine-scan+Z-ngc6543 SpireSpectroPcalFlashGen-ngc6543 SpireSpectro_CalGCO_FovMapFpgScan-short-fine-scan+Z-Pi1Gru-1 SpireSpectroPcalFlashGen-Pi1Gru-1 SpireSpectro_CalGCO_FovMapFpgScan-short-fine-scan+Z-BetaUMi SpireSpectroPcalFlashGen-BetaUMi SpireSpectro_CalGCO_FovMapFpgScan-short-fine-scan+Z-0537-441 SpireSpectroPcalFlashGen-0537-441 SpireSpectro_CalGCO_FovMapFpgScan-short-fine-scan+Z-8C0716+714 SpireSpectroPcalFlashGen-8C0716+714 B) SpireSpectro_Cal_StdLoadCurveGen-DarkSky SpireSpectroPcalFlashGen C) SpireSpectroPointGen-CR-Rep5-NGC7027 SpireSpectroPointGen-CR-Rep10-Vesta SpireSpectroPointGen-CR-Rep16-DarkSky SpireSpectroPointGen-CR-Rep6-Neptune D) SpireSpectroPointGen-CR-Full-Rep4-DarkSky Justifications: A) The observations in OD 342 show possible signs for improvment in the SIAM but we need more statistics which we get with these observations. B) Covered by Rcal Plan section 4.2.1 Detector load curves C) Covered by RCal Plan section 4.2.4 AOTs D) Covered by RCal Plan section 4.2.4.6 AOTs (duration still TBD but not very often as it is a long observation) 11. CusCmdscript output file (see note below) (a) Name of CusCmdScript SPIRE_CUS_THCP.py MC_ASTR_pv78_C013_53 (b) Expected durations when this is run see SPIRE_Duration.txt