! Proposal 6432, submission 1 ! PI: Prof. D. Reimers ! Received Tue Feb 13 12:00:22 EST 1996 ! From: hhagen@eso.org ! +====================+ ! | PED OUTPUT PRODUCT | ! +====================+ ! ! /diskc/visitor/hhagen/6432.prop ! Generated by PREPROCESSOR, version 6.0e ! Date: Tue Feb 6 19:28:04 MET 1996 Proposal_Information Title: Ly-alpha forest clouds at intermediate redshifts z=0.8 to 1.4 in the new double QSO HS 1216+5032 Proposal_Category: GO Scientific_Category: QSO Absorption Lines Cycle: 6 Investigators PI_Name: Prof. D. Reimers PI_Institution: Hamburger Sternwarte CoI_Name: Dr. H.-J. Hagen CoI_Institution: Hamburger Sternwarte Contact: Y CoI_Name: Dr. J. Bergeron CoI_Institution: European Southern Observatory, Munich Contact: CoI_Name: Dr. A. Smette CoI_Institution: University of Groningen Contact: Abstract: We propose to observe spectroscopically both components of the new double QSO HS 1216+5032 (z=1.43, d=9.1") with the FOS in high resolution in the range 2200 to 3270Angstrom with the aim to measure transverse dimensions of Ly-alpha forest clouds in the in this respect unexplored redshift range z=0.8 to 1.4 for which this QSO pair is an excellent target with a linear separation of 80 h_50^ -1 kpc. This double QSO recently discovered by the Hamburg survey is particularly well suited for a Ly-alpha forest study since it samples Ly-alpha clouds on a scale slightly smaller than the expected characteristic cloud sizes. Identification and spectroscopy of possible parent galaxies at z~1 from the ground combined with FOS data will yield 2-dimensional information on Ly-alpha clouds for the first time. Questions Observing_Description: We propose to take high-resolution spectra of both components with the FOS G270H. With an estimated flux >= 10^-15 erg/cm^2/s/Angstrom at 2400Angstrom for component A a S/N>=20 is reached in 22 min for Lambda>2400Angstrom (1 orbit). , Component B is about a factor of 6 to 7 fainter than A which requires about 140 min. exposure time or 4 orbits. Altogether 5 orbits are necessary to cover both objects with a S/N>=20 for Lambda>2400Angstrom. Real_Time_Justification: None. Medium resolution spectroscopy with DeltaLambda~2Angstrom covering the optical from 3300 to 6700Angstrom will be conducted with the Calar Alto 3.5m telescope (accepted for March 96). Deep imaging and spectroscopy of the QSO environment will be applied for at the CFHT 4m telescope for spring 96 (J. Bergeron). Calibration_Justification: Additional_Comments: Fixed_Targets Target_Number: 1 Target_Name: HS-1216+5032A Alternate_Names: Description: GALAXY,QSO, Position: RA=12H 18M 41.12S +/- 0.05S,DEC=50D 15' 36.4" +/- 0.5", PLATE-ID=00LK Equinox: J2000 RV_or_Z: Z = 1.45 RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: B = 17.0 F(3000)=10+/-3e-16 Comments: Target_Number: 2 Target_Name: HS-1216+5032B Alternate_Names: Description: GALAXY,QSO, Position: RA=12H 18M 40.62S +/- 0.05S,DEC=50D 15' 44.2" +/- 0.5", PLATE-ID=00LK Equinox: J2000 RV_or_Z: Z = 1.45 RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: B = 19.0 F(3000)=2+/-1e-16 Comments: Solar_System_Targets Generic_Targets Scan_Data Visits Visit_Number: 10 Visit_Requirements: On_Hold_Comments: Visit_Comments: Exposure_Number: 11 Target_Name: HS-1216+5032A Config: FOS/RD Opmode: ACQ/BINARY Aperture: 4.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 12S Special_Requirements: ONBOARD ACQ FOR 12-19 Comments: Exposure_Number: 12 Target_Name: HS-1216+5032A Config: FOS/RD Opmode: ACCUM Aperture: 4.3 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 33M Special_Requirements: Comments: Exposure_Number: 19 Target_Name: HS-1216+5032B Config: FOS/RD Opmode: ACCUM Aperture: 4.3 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 183M Special_Requirements: Comments: Data_Distribution ! Defaults indicated; change if desired Medium: 8MM Blocking_Factor: 10 Ship_To: PI_Address Ship_Via: UPS Recipient_Email: ! Let us know what you think of this template and software! ! Please send a list of your likes and dislikes to your Program Coordinator