1. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave1 Spectrometer Wavelength Calibration XHSPOT Proposal: PVSpecWave H. Feuchtgruber

2. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave2 47” x 47” - Blue array: 400 pixels - Red array: 400 pixels - 2 different blue filters - 3 grating orders - Grating range: 32000-1064000 positions - Spectral resolution elements: ~3650 (x sampling x time) Description of the Calibration Problem 1 st order 3 rd order 2 nd order 2x

3. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave3 PCD Requirements PCD sec. 4.2.1: Required accuracy: “Peak position to within 10-20% of a spectral resolution element”

4. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave4 XHSPOT Proposal: PVSpecWave (1) CUS AOR NameObservation Name Duration [Sec] PacsCal_WaveCalChopGen PVSpecWave_421C_nStdRS_chopnodorderB_WHya_000115603 PacsCal_WaveCalChopGen PVSpecWave_421C_nStdRS_chopnodorderA_Neptune_000115613 PacsCal_WaveCalChopGen PVSpecWave_421C_nStdRS_chopnodorderA_WHya_000115603 PacsCal_WaveCalChopGen PVSpecWave_421C_nStdRS_chopnodorderB_Neptune_000115613 PacsCal_WaveCalNoChopGen PVSpecWave_421D_nStdLS_nochoporderRed_NGC6302_0001533 PacsCal_WaveCalNoChopGen PVSpecWave_421D_nStdLS_nochoporderRed_NGC6302_0002832 PacsCal_WaveCalNoChopGen PVSpecWave_421D_nStdLS_nochoporderRed_NGC6302_0003531 PacsCal_WaveCalNoChopGen PVSpecWave_421D_nStdLS_nochoporderRed_NGC6302_00041132 PacsCal_WaveCalNoChopGen PVSpecWave_421B_nStdRS_nochoporderA_Jupiter_00017834 PacsCal_WaveCalNoChopGen PVSpecWave_421B_nStdRS_nochoporderB_Jupiter_00017834 PacsCal_WaveCalNoChopGen PVSpecWave_421D_nStdLS_nochoporderA_NGC6302_0001529 PacsCal_WaveCalNoChopGen PVSpecWave_421D_nStdLS_nochoporderA_NGC6302_0002530 PacsCal_WaveCalNoChopGen PVSpecWave_421D_nStdLS_nochoporderB_NGC6302_0001529 PacsCal_WaveCalNoChopGen PVSpecWave_421A_nStdRS_nochoporderA_Jupiter_0001704 PacsCal_WaveCalNoChopGen PVSpecWave_421A_nStdRS_nochoporderA_Jupiter_0002704 PacsCal_WaveCalNoChopGen PVSpecWave_421A_nStdRS_nochoporderB_Jupiter_00011015 PacsCal_WaveCalNoChopGen PVSpecWave_421A_nStdRS_nochoporderB_Jupiter_0002427 PacsCal_WaveCalNoChopGen PVSpecWave_421A_nStdRS_nochoporderB_Jupiter_00031015

5. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave5 XHSPOT Proposal: PVSpecWave (2) CUS AOR NameObservation Name Duration [Sec] PacsEng_PacsSpecSlewCalGen PVSpecWave_421B_nStdRS_SlewCalA_Dummy_000192 PacsEng_PacsSpecSlewCalGen PVSpecWave_421B_nStdRS_SlewCalA_Dummy_000292 PacsEng_PacsSpecSlewCalGen PVSpecWave_421B_nStdRS_SlewCalA_Dummy_000392 PacsEng_PacsSpecSlewCalGen PVSpecWave_421B_nStdRS_SlewCalB_Dummy_000192 PacsEng_PacsSpecSlewCalGen PVSpecWave_421B_nStdRS_SlewCalB_Dummy_000292 PacsEng_PacsSpecSlewCalGen PVSpecWave_421B_nStdRS_SlewCalB_Dummy_000392 PacsCal_WaveCalNodRasterGen PVSpecWave_425A_nStdRS_choprasterorderB_IC2501_000114733 PacsCal_WaveCalNodRasterGen PVSpecWave_425A_nStdRS_choprasterorderA_IC2501_000114734 PacsCal_WaveCalNodRasterGen PVSpecWave_425A_nStdRS_choprasterorderA_IC2501_000214733 PacsEng_Spec_CRE_setup_uGen PVSpecWave_421B_nStdCRE_setup_Dummy_00019 PacsEng_Spec_CRE_setup_uGen PVSpecWave_421B_nStdCRE_setup_Dummy_00029 PacsEng_Spec_CRE_setup_uGen PVSpecWave_421B_nStdCRE_setup_Dummy_00039 PacsEng_Spec_CRE_setup_uGen PVSpecWave_421B_nStdCRE_setup_Dummy_00049 PacsEng_Spec_CRE_setup_uGen PVSpecWave_421B_nStdCRE_setup_Dummy_00059 …. more to be filled in according to actual target visibilities !

6. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave6 Wavelength Calibration Targets (1) Suitable target list containing strong molecular lines: - PICC-ME-TN-013, ”Use of late type stars for PACS wavelength calibration”, (D. Lutz) -“Photometric and Spectroscopic Calibration of Herschel Instruments with Planets and Satellites”, (Th. Encrenaz, R. Moreno, A. Coustenis) Uranus(H 2 O), Neptune(H 2 O, CO), Saturn(H 2 O, NH 3, PH 3 ) Jupiter (H 2 O, NH 3, PH 3 ; fills entire 5x5 field of view !) Justtanont et al., A&A, 360, 1117-1125 (2000), “ISO-LWS observations of rotational CO lines from C-rich objects”

7. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave7 Wavelength Calibration Targets (2) Suitable target list containing strong atomic fine-structure lines: -19 selected Planetary Nebulae: IC418, IC2501, NGC5315, He2-131, NGC6210, NGC6543, NGC 6572, SwSt1, BD +30 3639, NGC6826, IC4997, NGC7027, NGC7662, NGC40, NGC3242, NGC3918, NGC5882, NGC6302, NGC6905 - Atomic fine-structure lines within the PACS wavelength range: [OIII]=51.8145µm;[NIII]=57.317µm;[OI]=63.184µm; [OIII]=88.356µm; [NII]=121.898µm;[OI]=145.525µm; [CII]=157.741µm;[NII]=205.178µm; - References: 1) ISO 95-015, Planetary nebulae to be used as ISO-SWS Astronomical Calibration Sources, H.W.W. Spoon, K.A. van der Hucht, D. Lutz 2) An Infrared Spectral Line List of Astrophysical Interest (2.4-200µm) and its use in the SWS and LWS ISO Central Program 3) www.mpe.mpg.de/ir/ISO/linelists/FSlines.html 4) Liu et al., MNRAS, 323, 343, (2001), “ISO LWS observations of planetary nebula fine-structure lines” [provides also observed line fluxes]

8. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave8 PVSpecWave: The spatial situation 43.9” Diameter of Jupiter Mid-Jun-09 as seen from L2 White crosses indicate location of all PACS spectrometer spatial pixels

9. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave9 PVSpecWave: Spatial Information about Targets Fluxes of moons and faint ring are being neglected Roll-angle will be important for assigning rotational velocity shifts separately for each spatial pixel (max. Δ λ ~11km/s) Check that no other bright targets come close to Jupiter at actual observation date/time. Require Herschel velocity towards target and doppler shifts

10. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave10 Status of Analysis and Uplink Preparation Analysis code (or CAP) is unchanged from FM ILT - Operating system: MS WinXP - Use HIPE to generate L0 products - Use IDL code to derive new calibration parameters - Output = ASCII files of polynomial coefficients for inclusion into pipeline Updated input model spectra for all giant planets are available now covering the entire PACS wavelength range and convolved to the PACS spectral resolution, inclusion of HD lines in progress For the overall calibration strategy and formalism see presentation at the Herschel Calibration Workshop#2 Uplink (1 st version) is defined in X-HSPOT proposal PVSpecWave No relevant SOVT data available for analysis Semi-Automatic calibration procedure

11. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave11 Calculated fluxes for 1 spatial pixel

12. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave12 Calibration Targets for Molecular Lines Start PV Start Routine Ops Target visibilities (HSPOT)

13. PACS CoP & PV Review 21/22 Jan 2009 PVSpecWave13 Target visibilities (HSPOT) Calibration on bright PNs Start PV Start Routine Ops selected out of Ref. (1) Monitoring for roll angle/time dependencies etc.