README Template 74.x (please do not delete the README Template Version line!) ESO Programme ID: SINFONI Science Verification Principal Investigator Name: Dieter Nuernberger, ESO Santiago + Paranal, Chile Principal Investigator E-mail Address: dnuernbe@eso.org Principal Investigator Telephone Number: +56 2 463 3080 Principal Investigator Postal Address: European Southern Observatory / Casilla 19001 / Santiago 19 / Chile Co Investigator Name: Ralf Siebenmorgen, ESO Garching, Germany Co Investigator E-mail Address: rsiebenm@eso.org Co Investigator Name: Michael Sterzik, ESO Santiago + Paranal, Chile Co Investigator E-mail Address: msterzik@eso.org Instrument: SINFONI OPC Priority Class: - OPC Approved Total Execution Time: --- Estimated Total Execution Time (including overheads): --- README File Submission Date: 30 August 2004 Revised Version: 24 November 2004 Programme Description ===================== General Overview ---------------- This is a pure IFU spectroscopy programme consisting of 7 OBs for observations in the K, J and H band. OB ID OB Name Exposure Time Execution Time Priority 177857 OrionBN_IFU_KJH_250 00:18:00.000 00:59:19.000 1 181503 OrionBN_IRn_IFU_KJH_250 00:18:00.000 01:00:51.000 1 181502 OrionBN_P1_IFU_KJH_100 00:24:00.000 01:02:53.000 1 181501 OrionBN_P2_IFU_KJH_100 00:24:00.000 01:02:53.000 1 181500 OrionBN_P3_IFU_KJH_100 00:24:00.000 01:02:53.000 1 181499 OrionBN_P4_IFU_KJH_100 00:24:00.000 01:02:53.000 2 181498 OrionBN_P5_IFU_KJH_100 00:24:00.000 01:02:53.000 2 2 OBs use SPIFFI's 250 mas camera (FOV = 8.0" x 8.0") and are centered on Orion BN and Orion BN IRn, respectively. 5 OBs use SPIFFI's 100 mas camera (FOV = 3.2" x 3.2") and are centered on 5 diffuse emission knots in the neighbourhood of Orion BN (see Finding Chart for Orion BN). All OBs can be executed independently from each other and, eventuelly, repeated 2-3 times. All OBs use the following AO reference source: Orion BN , RA = 05:35:14.12 , DEC = -05:22:22.9 , K=8 mag . In case of unexpected problems in using Orion BN for AO referencing, one might alternatively use TCC0016 , RA = 05:35:14.91 , DEC = -05:22:39.3 , V=14 mag . Both Orion BN and TCC0016 are within a distance of less than 30" from our science pointings (see Finding Chart for Orion BN). The sky position has been selected almost 3 arcmin towards the northwest of Orion BN and is expected to be free of any bright source. However, please check the sky position carefully. If necessary, DITs (15s/30s) and NDITs (3/2) should be adjusted properly. Approved Waiver Request Summary ------------------------------- There is no waiver request. Critical Observing Condition Constraints ---------------------------------------- There are no critical observing condition constraints apart from those specified in the OBs. Time Critical Aspects --------------------- There are no time critical aspects. Special Calibration Information ------------------------------- There are no special calibration information. ToO Information --------------- This is not a ToO programme. Pre-Imaging Requirements ------------------------ No pre-imaging is required for this programme. Source of preimaging: Not applicable OB Information ============== List of Science OBs ------------------- (for ISAAC imaging, please indicate the magnitude of the brightest star in the field for each OB) Total Number of Submitted Science OBs: 7 Total Number of Submitted Finding Charts: 1 OB ID OB Name Associated Finding Charts Priority 177857 OrionBN_IFU_KJH_250 SINFONI_SV_FC-OrionBN.jpg 1 181503 OrionBN_IRn_IFU_KJH_250 SINFONI_SV_FC-OrionBN.jpg 1 181502 OrionBN_P1_IFU_KJH_100 SINFONI_SV_FC-OrionBN.jpg 1 181501 OrionBN_P2_IFU_KJH_100 SINFONI_SV_FC-OrionBN.jpg 1 181500 OrionBN_P3_IFU_KJH_100 SINFONI_SV_FC-OrionBN.jpg 1 181499 OrionBN_P4_IFU_KJH_100 SINFONI_SV_FC-OrionBN.jpg 2 181498 OrionBN_P5_IFU_KJH_100 SINFONI_SV_FC-OrionBN.jpg 2 Please note that there is a bright source (Orion BN, the AO reference source; K=8 mag) within a distance of less than 30 arcsec from our science pointings (see Finding Chart for Orion BN). List of Calibration OBs with Associated Science OBs --------------------------------------------------- Total Number of Submitted Calibration OBs: 0 OB Compliance Checks ==================== (Y = Yes, N = No, NA = Not Applicable) Do all your OBs comply with the instrument specific requirements listed on the instrument specific Phase 2 Web pages ? [Y] Do all your Finding Charts comply with the both the general and instrument-specific finding chart requirements? [Y] If you submitted OBs for standard stars, did you specify the magnitude and spectral type of all standard stars ? [NA] Have you included OBs for any calibrations that you need but which are not a part of the Calibration Plan? [NA] [FORS only] Do all your FORS OBs use only the allowed detector read-out modes listed on the FORS1/FORS2 Phase 2 Web pages? [NA] [FORS only] Do all your FORS MOS/LSS OBs contain the mandatory "through-slit image" template? [NA] [UVES only] Do all your UVES OBs use only the allowed templates listed on the UVES Phase 2 Web pages ? [NA] [ISAAC only] Did you indicate the magnitude of the brightest star in the field for ISAAC imaging observations? [NA] [ISAAC only] If you submitted OBs for standard stars, did you use the provided StandardStar templates? [NA] [FLAMES only] Did you specify the hour angle range for which your Target Setup files are valid ? [NA] [VIMOS only] Did you specify suitable guide stars for all your OBs using Guidecam? [Y/N/NA] [VIMOS only] Did you check that the chosen guide stars are suitable for all the offset positions and that they do not produce unacceptable vignetting of the field of view? [NA] If you answered "NO" to any of these questions, please revise your OBs *before* submission.