! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template ! $Id: 6766,v 7.1 1996/03/18 14:12:00 pepsa Exp $ ! Hubble Space Telescope Cycle 6 (1996) Phase II Proposal Template ! $Id: 6766,v 7.1 1996/03/18 14:12:00 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: Landis ! Phone: 410-338-4560 , E-mail: landis@stsci.edu ! ! This partially completed template was generated from a Phase I proposal. ! Name of Phase I Proposal: archive-0970.goodrich.prop ! Date generated: Fri Dec 22 16:06:58 EST 1995 ! Proposal_Information ! Section 4 Title: Narrow-Line Seyfert 1s and the Iron Enigma in Active Galaxies Proposal_Category: GO Scientific_Category: AGN Cycle: 6 Investigators PI_name: Robert Goodrich PI_Institution: Space Telescope Science Institute CoI_Name: Anuradha Koratkar CoI_Institution: Space Telescope Science Institute Contact: ! Y or N (designate at most one contact) CoI_Name: Beverly Wills CoI_Institution: University of Texas Contact: ! Y or N (designate at most one contact) CoI_Name: Dirk Grupe CoI_Institution: Universitaets-Sternwarte, Goettingen Contact: ! Y or N (designate at most one contact) CoI_Name: Klaus Beuermann CoI_Institution: Universitaets-Sternwarte, Goettingen Contact: ! Y or N (designate at most one contact) Abstract: ! Free format text (please update) Seyfert 1 galaxies and QSOs show a number of intriguing correelations between their X-ray spectra, kinematics in the form of broad-line widths, and Fe II spectrum. Recent ROSAT spectra have shown that these relationships are very pronounced in the the so-called narrow-line Seyfert 1s, Seyfert 1s with particularly narrow permitted lines. NLS1s as a class show very strong Fe II, and very steep soft X-ray spectra. By studying the entire X-ray--UV--optical continuum, combined with UV and optical emission line strengths (in particular the Fe II lines), we will be able to shed light on the nature of these relationships, and on the physical conditions in the BLR. Questions ! Free format text (please update) Observing_Description: Our goal is to cover a wide wavelength range in both the optical and UV, concentrating on the UV. The FOS is ideal for this, providing coverage from 1150--6800 Angstrom with the gratings G130H, G190H, G270H, G400H, and G570H. Our target redshifts are z = 0.025--0.031 for three objects, and z = 0.236 for RX J0134-42. We have used IUE fluxes and measured optical--UV continuum slopes to estimate continuum flux levels at all wavelengths, except for RX J0134-42, for which no UV data exist. In this case we extrapolate the optical continuum using Alpha = 1.7, where F_Nu \propto nu^- Alpha. Using the inverse sensitivity values given in Tables 1 -6 and 1-7 of the FOS Instrument Handbook allows us to calculate count rates per diode at 50 Angstrom intervals in each grating. At the count rates we derive the FOS detector backgrounds are not important. The signal-to-noise, S/N, was then calculated for a typical exposure time. Table 1 gives examples at a more or less typical wavelength in each grating. Note that we tabulate S/N values per diode in the continuum; the S/N in the emission lines will be higher, and continuum regions over which we can average many diodes together will have much higher S/N. For a sample calculation let us consider Mrk 493 at 2000 Angstrom observed with the G190H/RD configuration. The continuum flux is 22.9 * 10^-15 erg cm^-2 s^-1 AA^-1 at 2000 Angstrom, and the G190H/RD inverse sensitivity is 9.85 * 10^-15 erg cm^-2 s^-1 AA^-1 diode count^-1. Dividing the flux by the inverse sensitivity we find 2.32 ct s^-1 diode^-1. In a 40 minute exposure we will get 5600 ct diode^-1, or a continuum S/N = 75 diode^-1. Our orbit-packing strategy will be to use a standard guide star acquisition (8^ m) followed by a standard binary acquisition with FOS/BL (9^ m). Removing the 6^ m overhead this allows ~ 30^ m for the first exposure, which will be the G130H grating. The second orbit will also be with the G130H grating, allowing another 40^ m accounting for guide star reacquisition and FOS overhead. During occultation we will switch to the red side, and the third orbit will be 25^ m in G190H and 9^ m in G570H, accouting again for guide star reacquisition and Two FOS overheads. The fourth orbit will contain a 20^ m G270H exposure and a 14^ m G400H exposure. The estimated S/N using the above observing strategy and flux level estimates are shown for representative wavelengths in the following table. Note that the fluxes are in units of 10^-15 erg cm^-2 s^-1 AA^-1, and we have assumed a power law for the continuum shape. begincentering begintable*h begintabular*6.5in l@ \fill c@ \fill c@ \fill c@ \fill c@ \fill c@ \fill c@ \fill Object&G130H&G190H&G270H&G400H&G570H&Flux at fiducial, &70^ m&25^ m&20^ m&14^ m&9^ m& wavelength, slope, WPVS 007&16&26&47&41&27&6.5 at Lambda1500, Alpha = 0.85, RX J0134- 42&37&47&62&39&19&16.7 at Lambda1900, Alpha = -0.89, Mrk 493&32&56&117&122&95&22.9 at Lambda2000, Alpha = 1.7, Akn 564&22&40&84&88&69&13.2 at Lambda1450, Alpha = 1.7, endtabular* endtable* endcentering Real_Time_Justification: None. ROSAT has already observed these targets, providing us with soft X-ray spectra which we can compare to the HST optical/UV data. Calibration_Justification: Additional_Comments: Fixed_Targets Target_Number: 1 Target_Name: WPVS007 Alternate_Names: Description: GALAXY, SEYFERT Position: RA=00H 39M 15.8S +/- 2", DEC=-51D 17' 03" +/- 2", PLATE-ID=03BW Equinox: J2000 RV_or_Z: Z=0.028 RA_PM: Dec_PM: Epoch: Annual_Parallax: Flux: F-CONT(1300)=9.0 +/- 0.9 E-15 F-CONT(1500)=5.9 +/- 0.6 E-15 F-CONT(1700)=7.0 +/- 0.7 E-15 F-CONT(1900)=6.8 +/- 0.7 E-15 F-CONT(3800)=2.5 +/- 0.3 E-15 F-CONT(5000)=1.5 +/- 0.15 E-15 F-CONT(6000)=1.2 +/- 0.12 E-15 F-CONT(7000)=0.94 +/- 0.09 E-15 Comments: Target_Number: 2 Target_Name: RXJ0134-42 Alternate_Names: Description: GALAXY, SEYFERT Position: RA=01H 34M 16.8S +/- 1", DEC=-42D 58' 27" +/- 1", PLATE-ID=01W0 Equinox: J2000 RV_or_Z: Z=0.236 RA_PM: Dec_PM: Epoch: Annual_Parallax: Flux: F-CONT(1890)=17 +/- 1.7 E-15 F-CONT(4700)=2.0 +/- 0.2 E-15 F-CONT(5500)=1.3 +/- 0.2 E-15 F-CONT(6900)=0.7 +/- 0.1 E-15 Comments: Target_Number: 3 Target_Name: MRK493 Alternate_Names: Description: GALAXY, SEYFERT Position: RA=15H 59M 09.63S +/- 0.5", DEC=+35D 01' 47.5" +/- 0.5", PLATE-ID=01RN Equinox: J2000 RV_or_Z: Z=0.03190 RA_PM: Dec_PM: Epoch: Annual_Parallax: Flux: F-CONT(1300)=7.0 +/- 0.7 E-15 F-CONT(1500)=7.5 +/- 0.8 E-15 F-CONT(1700)=7.3 +/- 0.7 E-15 F-CONT(1900)=6.0 +/- 0.6 E-15 B=14.6 +/- 0.2 E(B-V)=0.01 Comments: Z=0.03190 Target_Number: 4 Target_Name: AKN564 Alternate_Names: Description: GALAXY, SEYFERT Position: RA=22H 42M 39.34S +/- 0.5", DEC=+29D 43' 31.3" +/- 0.5", PLATE-ID=02UE Equinox: J2000 RV_or_Z: Z=0.02398 RA_PM: Dec_PM: Epoch: Annual_Parallax: Flux: F-CONT(1300)=8.1 +/- 1.6 E-15 F-CONT(1500)=8.8 +/- 0.9 E-15 F-CONT(1700)=8.2 +/- 0.8 E-15 F-CONT(1900)=8.2 +/- 0.8 E-15 U=14.00 +/- 0.13 B=14.58 +/- 0.23 V=14.16 R=13.39 E(B-V)=0.06 Comments: Z=0.02398 Solar_System_Targets Generic_Targets Scan_Data ! This is a template for a single visit containing a single exposure ! Repeat exposure and visit blocks as needed Visits Visit_Number: 1 Visit_Requirements: Exposure_Number: 1 Target_Name: WPVS007 Config: FOS/BL 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 2-6 Comments: Simulated using (power=1.1, starmag=15.5) and (power=0.85, starmag=15.75), giving ACQ/BIN times of 11.2 and 12.0 sec. Exposure_Number: 2 Target_Name: WPVS007 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 64M Special_Requirements: Comments: Exposure_Number: 3 Target_Name: WPVS007 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G160L Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 4M Special_Requirements: Comments: To tie together red and blue observations accurately. Exposure_Number: 4 Target_Name: WPVS007 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 25M Special_Requirements: Comments: Exposure_Number: 5 Target_Name: WPVS007 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G570H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 9M Special_Requirements: Comments: Exposure_Number: 6 Target_Name: WPVS007 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 20M Special_Requirements: Comments: Exposure_Number: 7 Target_Name: WPVS007 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G400H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 14M Special_Requirements: Comments: Visit_Number: 2 Visit_Requirements: Exposure_Number: 1 Target_Name: RXJ0134-42 Config: FOS/BL Opmode: ACQ/BINARY Aperture: 4.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 5S Special_Requirements: ONBOARD ACQ FOR 2-6 Comments: Simulated using (power=0.89, starmag=14.5) and (power=1.7, starmag=16.5), for the UV and optical wavelengths, respectively. The ACQ/BIN times were 4s and 40s, so we have used 22s. Exposure_Number: 2 Target_Name: RXJ0134-42 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 64M Special_Requirements: Comments: Exposure_Number: 3 Target_Name: RXJ0134-42 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G160L Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 4M Special_Requirements: Comments: To tie together the red and blue spectra. Exposure_Number: 4 Target_Name: RXJ0134-42 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 25M Special_Requirements: Comments: Exposure_Number: 5 Target_Name: RXJ0134-42 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G570H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 9M Special_Requirements: Comments: Exposure_Number: 6 Target_Name: RXJ0134-42 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 20M Special_Requirements: Comments: Exposure_Number: 7 Target_Name: RXJ0134-42 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G400H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 14M Special_Requirements: Comments: Visit_Number: 3 Visit_Requirements: Exposure_Number: 1 Target_Name: MRK493 Config: FOS/BL Opmode: ACQ/BINARY Aperture: 4.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 7S Special_Requirements: ONBOARD ACQ FOR 2-6 Comments: Simulated using (power=1.2, starmag=15.25). Exposure_Number: 2 Target_Name: MRK493 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 64M Special_Requirements: Comments: Exposure_Number: 3 Target_Name: MRK493 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G160L Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 4M Special_Requirements: Comments: To tie together the red and blue spectra. Exposure_Number: 4 Target_Name: MRK493 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 25M Special_Requirements: Comments: Exposure_Number: 5 Target_Name: MRK493 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G570H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 9M Special_Requirements: Comments: Exposure_Number: 6 Target_Name: MRK493 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 20M Special_Requirements: Comments: Exposure_Number: 7 Target_Name: MRK493 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G400H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 14M Special_Requirements: Comments: Visit_Number: 4 Visit_Requirements: Exposure_Number: 1 Target_Name: AKN564 Config: FOS/BL Opmode: ACQ/BINARY Aperture: 4.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 6S Special_Requirements: ONBOARD ACQ FOR 2-6 Comments: Simulated using (power=1.8, starmag=14.3). Exposure_Number: 2 Target_Name: AKN564 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 64M Special_Requirements: Comments: Exposure_Number: 3 Target_Name: AKN564 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G160L Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 4M Special_Requirements: Comments: To tie together the red and blue spectra. Exposure_Number: 4 Target_Name: AKN564 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 25M Special_Requirements: Comments: Exposure_Number: 5 Target_Name: AKN564 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G570H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 9M Special_Requirements: Comments: Exposure_Number: 6 Target_Name: AKN564 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 20M Special_Requirements: Comments: Exposure_Number: 7 Target_Name: AKN564 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G400H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 14M Special_Requirements: Comments: Data_Distribution ! Defaults indicated; change if desired Medium: 8MM ! 8MM or 6250BPI or 1600BPI Blocking_Factor: 10 ! 10 or 1 ! Only astronomers with very old 9- ! track tape drives should consider ! a blocking factor of 1 Ship_To: PI_Address ! STSCI or PI_Address or ! PI Address from Phase I is: ! ! 3700 San Martin Drive ! Baltimore ! 21218 ! ! Ship_Via: UPS ! UPS (2-day) or OVERNIGHT ! Overnight shipping done at PI expense Recipient_Email: ! Needed if Ship_To: is not PI_Address ! ! Let us know what you think of this template and software! ! Please send a list of your likes and dislikes to your Program Coordinator