Proposal_Information Title: Ne VIII Emission in the QSO PG 1148+549 Proposal_Category: GTO/FOS Scientific_Category: Quasars Cycle: 5 Investigators PI_name: E. MARGARET BURBIDGE PI_Institution: UNIVERSITY OF CALIFORNIA, SAN DIEGO CoI_Name: RICHARD J. HARMS CoI_Institution: APPLIED RESEARCH CORPORATION CoI_Name: J. ROGER P. ANGEL CoI_Institution: UNIVERSITY OF ARIZONA CoI_Name: FRANK BARTKO CoI_Institution: UNAFFILIATED CoI_Name: EDWARD BEAVER CoI_Institution: UNIVERSITY OF CALIFORNIA, SAN DIEGO CoI_Name: RALPH C. BOHLIN CoI_Institution: SPACE TELESCOPE SCIENCE INSTITUTE CoI_Name: ARTHUR F. DAVIDSEN CoI_Institution: JOHNS HOPKINS UNIVERSITY CoI_Name: HOLLAND C. FORD CoI_Institution: SPACE TELESCOPE SCIENCE INSTITUTE CoI_Name: GEORGE F. HARTIG CoI_Institution: SPACE TELESCOPE SCIENCE INSTITUTE CoI_Name: BRUCE H. MARGON CoI_Institution: UNIVERSITY OF WASHINGTON Abstract: UV spectra of the bright QSO PG 1148+549 (V=15.8, z=0.978) will be obtained to study the far UV emission lines. Low resolution IUE spectra show an emission line at the expected location of Ne VIII 770,780 emission. Ne VIII emission must come from a region of very high ionization and small Lyman continuum optical depth. The presence of Ne VIII emission could indicate a new emission component in the broad emission line region of QSOs beyond the conventional optically thick emission line clouds. These observations will also be used to measure the Ly alpha forest absorption near z = 1. Questions Observing_Description: We will use FOS/BL and the G130H, G190H, and G270H gratings to obtain spectra with complete wavelength coverage from ~1200 to ~3300 Angstrom in one QSO. We will use the Binary Search acquisition and the 1.0" aperture. We will use only FOS/BL (instead of FOS/RD for the G190H and G270H settings) because a side switch is too time consuming. For the exposure times given below, we expect SNRs per diode of ~15 for G130H and G190H and 25 for G270H (based on fluxes measured with the IUE) and the count rates given in version 5.0 of the FOS Manual (Fig. 1.2.3). Real_Time_Justification: None. Calibration_Justification: We request that wavelength calibration lamps be taken with F190H and G130H grating settings to minimize the wavelength uncertainties caused by grating shifts. We request that the lamp exposures be obtained DURING OCCULTATION to maximize the science target exposure times. Fixed_Targets Target_Number: 1 Target_Name: PG1148+549 Description: GALAXY, Quasar, BLR Position: RA=11H 51M 20.44S +/- 0.3S, DEC=54D 37' 32.8" +/- 0.5", PLATE-ID=00LK Equinox: 2000 RV_or_Z: Z=0.97 Flux: V=15.82, B-V=0.3 F-CONT(800) = 1.0 +/- .4 E-14 F-CONT(1550) = 5.3 +/- .3 E-15 Visits Visit_Number: 1 Exposure_Number: 1 Target_Name: PG1148+549 Config: FOS/BL Opmode: ACQ/BINARY Aperture: 4.3 Sp_Element: MIRROR Number_of_Iterations: 1 Time_Per_Exposure: 15S Special_Requirements: ONBOARD ACQ FOR 2-7 Exposure_Number: 2 Target_Name: PG1148+549 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: 1200-1600 Number_of_Iterations: 1 Time_Per_Exposure: 1570S Special_Requirements: EXPAND Exposure_Number: 3 Target_Name: WAVE Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: 1200-1600 Number_of_Iterations: 1 Time_Per_Exposure: DEF Exposure_Number: 4 Target_Name: PG1148+549 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: 1200-1600 Number_of_Iterations: 1 Time_Per_Exposure: 970S Special_Requirements: EXPAND Exposure_Number: 5 Target_Name: PG1148+549 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: 2300-3250 Number_of_Iterations: 1 Time_Per_Exposure: 350S Special_Requirements: MAX DUR 150% Exposure_Number: 6 Target_Name: PG1148+549 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: 1580-2330 Number_of_Iterations: 1 Time_Per_Exposure: 750S Special_Requirements: MAX DUR 150% Exposure_Number: 7 Target_Name: WAVE Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: 1580-2330 Number_of_Iterations: 1 Time_Per_Exposure: DEF Data_Distribution Medium: 8MM Blocking_Factor: 10 Ship_To: ROSS COHEN CASS 0111 9500 GILMAN DRIVE LA JOLLA, CA 92093-0111 Ship_Via: UPS Recipient_Email: ross@cassfos03.ucsd.edu