! Proposal 6719, submission 1 ! PI: Dr. Edward Olszewski ! Received Tue Feb 6 13:21:42 EST 1996 ! From: edo@as.arizona.edu ! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template ! $Id: 6719,v 5.1 1996/08/27 19:15:14 pepsa Exp $ ! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template ! $Id: 6719,v 5.1 1996/08/27 19:15:14 pepsa Exp $ ! ! Refer to the HST Phase II Proposal Instructions to fill this out ! ! Anything after a "!" is ignored, and may be deleted ! ! All keywords with multiple entries are comma delimited except the ! Visit_Requirements and Special_Requirements keywords which can be ! delimited with carriage returns or semi-colons, but not commas ! ! For help call your Program Coordinator: Sleiman ! Phone: 410-338-4753 , E-mail: sleiman@stsci.edu ! ! This partially completed template was generated from a Phase I proposal. ! Name of Phase I Proposal: archive-0852.olszewski.prop ! Date generated: Fri Dec 22 18:20:59 EST 1995 ! Proposal_Information ! Section 4 Title: The Gaseous Environment of the Ursa Minor Dwarf Spheroidal Galaxy Proposal_Category: GO Scientific_Category: STELLAR POPULATIONS Cycle: 6 Investigators PI_name: Dr. Edward Olszewski PI_Institution: Steward Observatory CoI_Name: Dr. Jill Bechtold CoI_Institution: Steward Observatory, University of Arizona Contact: ! Y or N (designate at most one contact) Abstract: ! Free format text (please update) We propose to probe the interstellar gas content of the Ursa Minor dwarf spheroidal galaxy. We have discovered a V=18.66 QSO at approximately 1 core radius from the center of UMi. We will use the FOS to look for EUV absorption lines from gas in UMi. This technique complements previous unsuccessful searches for gas in dSph. These galaxies should have large reservoirs of gas: some of them ( e.g. Carina and Leo I), made a significant second generation of stars a few Gyr ago, and since their gravitational potential is dominated by dark matter, they should be able to retain an observable amount of gas, built up through infall or stellar mass loss. We intend to use the G270H grating, which allows us to observe the Mg II doublet, Mg I, Fe II lines, and weak Fe I, Al I, Mn II, and Ti II lines. Because of the patchy nature of the Milky Way high velocity halo gas, we will also observe a brighter, nearby QSO (2^degrees away) to ensure that we can ascribe any detections to UMi. Finally we will take a low resolution, G160L, spectrum to see if the UMi QSO is clear of optically thick Lyman limits for future spectroscopy of more highly ionized species. Questions ! Free format text (please update) Observing_Description: def\nhi =1.0truecm Exposure times were estimated using the STSDAS SYNPHOT software in IRAF, normalizing a power law spectrum of slope +1 to the measured B magnitude. We used the published QSO Key Project spectra (Bahcall et al. 1993) obtained from the archives to calculate the S/N needed to attain a given equivalent-width limit: one needs S/N~30 per DIODE to get an equivalent-width limit of ~0.2Angstrom\ (3- Sigma). We will use the 1^'' aperture since the resolution is little affected for point sources, and the overhead for acquisition is less. We note that scattered light will be negligible, since the central surface brightness of UMi is 25.1 mag arcsec^-2, and there are no objects as bright as the QSO within 25 arcsec. \oneskip 1.underlineUMI-COS253 = QSO 1508+673: nhi10920 sec (182 min) actual exposure with FOS/RD, G270H and 1.0^'' aperture. This will cover the 2225 - 3280 Angstrom\ spectrum at about 100 km/sec resolution, to look for absorption lines from the ISM of UMi, at v(helio) = -250 km/sec. Lines of Mg II, Mg I, Fe II, and Mn II are expected. An equivalent width limit of about 0.2 Angstrom will be achieved. (It will take 5 orbits to achieve this exposure time: see below.) 2.underline B2 1503+691: nhi2700 sec (45 min) exposure with FOS/RD, G270H and 1.0^'' aperture. This brighter (V = 17) QSO will be used to look for absorption from Galactic gas, particularly high velocity gas in the Galactic halo, in the direction of UMi. Signal-to-noise will be comparable to UMI-COS253 spectrum. (2 orbits: see below.) 3.underlineUMI-COS253 = QSO 1508+673: nhi2760 sec (46 min)exposure with FOS/BL, G160L and 4.3^'' circular aperture. This low dispersion spectrum, covering 1150 - 2400 Angstrom will be used to look for optically thick Lyman limits from intervening metal-line systems for wavelengths short of 1550 Angstrom. This low resolution spectrum will also be used to estimate exposure times of follow-up high dispersion spectroscopy. We estimate using SYNPHOT that we will achieve 27 counts at 1250 Angstrom\ and 190 counts at 2200 Angstrom adequate for finding the strong Lyman limits features. (2 orbits: see below.) \oneskip We calculated orbits as follows: indentFirst object, UMi QSO, red side: Guidestar acq 8m; aperture acq 41m; 2m exposure; 6 m readout; end of orbit 1. Orbit 2--5: reacq 6m; 45m exposure; 6m readout. 182 m=10,920 sec total exposure. This will give 1000 counts/diode at Mg II. Start change to blue side, using all 39 m of occulted time indentChange sides of FOS: need 6m of unocculted time to finish the side change of FOS; guidestar reacq 6m; 41 min of aperture acquisition; end orbit 1. Then Orbit 2: 6 m reacq; 45m exposure; 6m readout. Begin change back to red side while moving telescope, using all 39m of occulted time. ControlQSO: 6 m to finish change to red side; 8 m to acquire guidestar; 41 m of aperture acq; end of orbit 1. Orbit 2: 6m of reacq; 46m exposure; 6m readout. This will give 1000 counts/diode at Mg II. Real_Time_Justification: None. We will supplement these observations with high dispersion optical spectroscopy at Ca II H&K obtained at the Multiple Mirror Telescope. Calibration_Justification: ! Move appropriate text from Real_Time_Justification Additional_Comments: Fixed_Targets ! Section 5.1 Target_Number: 1 Target_Name: QSO1508+673 Alternate_Names:UMI COS253 Description:GALAXY,QSO Position: RA=15H 08M 40.41S +/- 0.1S, DEC=+67D 17' 47.52" +/- 0.5", PLATE-ID=00A9 ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox:J2000 RV_or_Z:Z=1.7 RA_PM: 0.0 ! Units are seconds of time per year Dec_PM: 0.0 ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: V= 18.6 +/- 0.5 B-V = 0.2 +/- 0.1 ! Include at least V and B-V Comments:a red FOS spectrum will be taken immediately followed by a blue spectrum Target_Number: 2 Target_Name: B2-1503+691 Alternate_Names: Description:GALAXY,QSO Position: RA=15H 04m 12.69S +/- 0.1S, DEC=+68D 56' 13.2" +/- 0.5", PLATE-ID=01L5 ! Most common specification format is ! RA=0H 0M 0.00S +/- 0S, ! DEC=0D 0' 0.0" +/- 0", ! PLATE-ID=0000 Equinox:J2000 RV_or_Z:Z=0.3 RA_PM: 0.0 ! Units are seconds of time per year Dec_PM: 0.0 ! Units are seconds of arc per year Epoch: Annual_Parallax: Flux: V= 17.0 +/- 0.5 B-V= 0.2 +/- 0.1 ! Include at least V and B-V Comments:the control qso for target 1 Visits ! Section 6 Visit_Number:1 Visit_Requirements: ! Section 7.1 Exposure_Number:10 ! Section 6.5 Target_Name:QSO1508+673 Config:FOS/RD Opmode:ACQ/PEAK Aperture:4.3 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-Y=1.23, SEARCH-SIZE-Y=3, SEARCH-SIZE-X=1 Number_of_Iterations:1 Time_Per_Exposure:3.63S Special_Requirements:ONBOARD ACQ FOR 20 ! Section 7.2 Comments:stage 1 of 4-stage peakup Exposure_Number:20 ! Section 6.5 Target_Name:QSO1508+673 Config:FOS/RD Opmode:ACQ/PEAK Aperture:1.0 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-X=0.61,SCAN-STEP-Y=0.61, SEARCH-SIZE-X=2,SEARCH-SIZE-Y=6 Number_of_Iterations:1 Time_Per_Exposure:3.63S Special_Requirements:ONBOARD ACQ FOR 30 ! Section 7.2 Comments:stage 2 of 4-stage peakup Exposure_Number:30 ! Section 6.5 Target_Name:QSO1508+673 Config:FOS/RD Opmode:ACQ/PEAK Aperture:0.5 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-X=0.29,SCAN-STEP-Y=0.29, SEARCH-SIZE-Y=3, SEARCH-SIZE-X=3 Number_of_Iterations:1 Time_Per_Exposure:3.63S Special_Requirements:ONBOARD ACQ FOR 40 ! Section 7.2 Comments:stage 3 of 4-stage peakup Exposure_Number:40 ! Section 6.5 Target_Name:QSO1508+673 Config:FOS/RD Opmode:ACQ/PEAK Aperture:0.3 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-X=0.11,SCAN-STEP-Y=0.11, SEARCH-SIZE-Y=4, SEARCH-SIZE-X=4 Number_of_Iterations:1 Time_Per_Exposure:36S Special_Requirements:ONBOARD ACQ for 50 ! Section 7.2 Comments:final peakup Exposure_Number:50 ! Section 6.5 Target_Name:QSO1508+673 Config:FOS/RD Opmode:ACCUM Aperture:1.0 Sp_Element:G270H Wavelength: Optional_Parameters: Number_of_Iterations:1 Time_Per_Exposure:10920s Special_Requirements: Comments:exposure on the object in the 1" aperture Exposure_Number:55 ! Section 6.5 Target_Name:WAVE Config:FOS/RD Opmode:ACCUM Aperture:1.0 Sp_Element:G270H Wavelength: Optional_Parameters: Number_of_Iterations:1 Time_Per_Exposure:DEF Special_Requirements: Comments:calibration for 50; don't move anything between 50 and 55; the end of 55, and 55, must be in same orbit; when done switch to blue FOS ! Section 7.2 Exposure_Number:60 ! Section 6.5 Target_Name:QSO1508+673 Config:FOS/BL Opmode:ACQ/PEAK Aperture:0.25-PAIR-A Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-X=0.11,SCAN-STEP-Y=0.11, SEARCH-SIZE-Y=4, SEARCH-SIZE-X=4 Number_of_Iterations:1 Time_Per_Exposure:60S Special_Requirements:ONBOARD ACQ for 70 ! Section 7.2 Comments:final peakup for 70 Exposure_Number:70 ! Section 6.5 Target_Name:QSO1508+673 Config:FOS/BL Opmode:ACCUM Aperture:1.0-PAIR-A Sp_Element:G160L Wavelength: Optional_Parameters: Number_of_Iterations:1 Time_Per_Exposure:2700S Special_Requirements: Comments:done with blue side after this exposure; this is a low-resolution reconnaissance exposure Visit_Number:2 Visit_Requirements: ! Section 7.1 On_Hold_Comments: Visit_Comments: visit 2 does not have to be done at same time as visit 1; it's a different qso Exposure_Number:80 ! Section 6.5 Target_Name:B2-1503+691 Config:FOS/RD Opmode:ACQ/PEAK Aperture:4.3 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-Y=1.23, SEARCH-SIZE-Y=3, SEARCH-SIZE-X=1 Number_of_Iterations:1 Time_Per_Exposure:1.S Special_Requirements:ONBOARD ACQ FOR 90 ! Section 7.2 Comments:stage 1 of 4-stage peakup Exposure_Number:90 ! Section 6.5 Target_Name:B2-1503+691 Config:FOS/RD Opmode:ACQ/PEAK Aperture:1.0 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-X=0.61,SCAN-STEP-Y=0.61, SEARCH-SIZE-X=2,SEARCH-SIZE-Y=6 Number_of_Iterations:1 Time_Per_Exposure:1.S Special_Requirements:ONBOARD ACQ FOR 100 ! Section 7.2 Comments:stage 2 of 4-stage peakup Exposure_Number:100 ! Section 6.5 Target_Name:B2-1503+691 Config:FOS/RD Opmode:ACQ/PEAK Aperture:0.5 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-X=0.29,SCAN-STEP-Y=0.29, SEARCH-SIZE-Y=3, SEARCH-SIZE-X=3 Number_of_Iterations:1 Time_Per_Exposure:1.S Special_Requirements:ONBOARD ACQ FOR 110 ! Section 7.2 Comments:stage 3 of 4-stage peakup Exposure_Number:110 ! Section 6.5 Target_Name:B2-1503+691 Config:FOS/RD Opmode:ACQ/PEAK Aperture:0.3 Sp_Element:MIRROR Wavelength: Optional_Parameters:SCAN-STEP-X=0.11,SCAN-STEP-Y=0.11, SEARCH-SIZE-Y=4, SEARCH-SIZE-X=4 Number_of_Iterations:1 Time_Per_Exposure:10S Special_Requirements:ONBOARD ACQ for 120 ! Section 7.2 Comments:final stage of 4-stage peakup Exposure_Number:120 ! Section 6.5 Target_Name:B2-1503+691 Config:FOS/RD Opmode:ACCUM Aperture:1.0 Sp_Element:G270H Wavelength: Optional_Parameters: Number_of_Iterations:1 Time_Per_Exposure:2500S Special_Requirements: Comments:the object finally Exposure_Number:125 ! Section 6.5 Target_Name:WAVE Config:FOS/RD Opmode:ACCUM Aperture:1.0 Sp_Element:G270H Wavelength: Optional_Parameters: Number_of_Iterations:1 Time_Per_Exposure:DEF Special_Requirements: Comments:calibration for 120; don't move anything between 120 and 125 Data_Distribution ! 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