! +====================+ ! | PED OUTPUT PRODUCT | ! +====================+ ! ! /spectre/data1/aroman/proposals/6001.prop ! Generated by PREPROCESSOR, version 6.0e ! Date: Sat Dec 30 17:47:41 EST 1995 Proposal_Information Title: NGC 5253 STARBURST AS A LABORATORY FOR ENRICHMENT PROCESSES Proposal_Category: GO Scientific_Category: Galaxies & Clusters Cycle: 5 Investigators PI_Name: Jean-Rene ROY PI_Institution: Universite Laval CoI_Name: Jeremy WALSH CoI_Institution: European Southern Observatory Contact: CoI_Name: Michael ROSA CoI_Institution: European Southern Observatory Contact: Abstract: The nearby starburst in NGC 5253 presents a unique snapshot of the short stage of element enrichment and an unprecedented opportunity to study the interaction between evolving massive stars and the interstellar medium. We propose to observe NGC 5253 with FOS to: (i) determine the carbon abundance near a region of enhanced nitrogen found from the ground to be associated with Wolf-Rayet stars, and (ii) to study the stellar population in the central starburst knots and to model their age and IMF in order to relate the stellar properties to the ISM enrichment. HST provides the long wavelength coverage to allow determination of element abundances, IMF and starburst age from stellar signatures, together with the high spatial resolution to measure change over arcsec scales. The proposed observations should result in a fundamental understanding of the link between starbursts and enrichment mechanisms of relatively low metallicity gas. Questions Observing_Description: It is proposed to observe three of the starburst knots in the dwarf elliptical blue compact galaxy NGC 5253 with the FOS and the 0.86'' round aperture; one of these knots is known to be enhanced in N from ground-based spectroscopy. The emission lines of H, C, N and O will be studied for abundance derivations, and the stellar continuum from 1150 to 8200 Angstrom\\\\ will be measured to assess the stellar population from O to G stars. Spectra at identical positions in the full UV range and in the optical to 8200 Angstrom\\\\ are needed. Full wavelength coverage between 1150 and 8200 Angstrom\\\\ will be achieved by two grating exposures with the blue tube (G130H and G190H) and four grating exposures with the amber tube (G270H, G400H, G570 and G 780H) of each of the three knots. Accurate positions of the knots will be derived from archive WFPC images of NGC 5253 to be released in september 1994. From our ground-based spectroscopic mapping of NGC 5253, we have been able to measure the V surface brightness of the stellar continuum in the three knots to be observed, here named UV1, UV2 and UV3 (corresponding to regions 1, 6 and 2 respectively in Walsh & Roy (1989). The V surface brightness is 18.4 mag arcsec^-2 for both UV1 and UV3 and 18.8 for UV2. The extinction for UV1 is A_V = 0.96 mag, and similar for UV2 and UV3. We aim for a fairly uniform S/N across all the grating domains, so that we can disentangle the various stellar contributions. With S/N >= 10 on the continuum, we will get good line fluxes since the minimum H Beta\\\\ equivalent width (in UV2) is 36 and the C III 1908 Angstrom\\\\ line has an equivalent width of ~5. Section lists the requested exposure times in seconds for V = 18.5, A_V = 0.9 for each grating for a mean of 200 counts/diode (S/N ~ 12). For the G130H spectrum, the exposure time has been estimated for 100 counts per bin. Since the resolution is higher for this grating, we can bin by a factor 3, so we reduce the exposure time to 3000 s. The largest fraction of exposure time is spent on this wavelength region and is justified by its astrophysical importance. For the six grating exposures, 3 orbits are required per starburst knot. We plan to obtain the color of acquisition stars around NGC 5253 from archive HST frames, and use acq/binary; we will check the images for extended sources which would confuse the acq/binary. The centering should be ~0.5 arcsec. Real_Time_Justification: Calibration_Justification: Additional_Comments: Should be scheduled in cooperation wit a related proposal, proposal number 6021 (Kobulnicky and Skillman), for best efficiency. This file is intended to be merged with 6021 to achieve a 12-orbit, 2-visit schedule file. Targets list in this file is same as 6021, for completeness, though not all targets are observed in this visit. Fixed_Targets Target_Number: 1 Target_Name: STAR-OFFSET Alternate_Names: Description: STAR Position: RA=13H 39M 51.7925S +/- 0.01S,DEC=-31D 39' 03.244" +/- 0.1" Equinox: J2000 RV_or_Z: RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: V = 14.5+/-0.5 B-V = 0.5+/-0.5 Comments: Target_Number: 2 Target_Name: NGC5253-UV1 Alternate_Names: Description: EXT-MEDIUM, HII REGION Position: RA-OFF=4.03S+/- 0.01S,DEC-OFF=35.93"+/- 0.1",FROM 1 Equinox: J2000 RV_or_Z: V = +400 RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: SURF(V) = 18.4+/-0.2 B-V = 0.0 A(V) = 0.9 Comments: Object in the galaxy is a stellar cluster Target_Number: 3 Target_Name: NGC5253-UV2 Alternate_Names: Description: EXT-MEDIUM, HII REGION Position: RA-OFF=4.08S+/- 0.01S,DEC-OFF=31.54"+/- 0.1",FROM 1 Equinox: J2000 RV_or_Z: V = +400 RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: SURF(V) = 18.8+/-0.2 B-V = 0.0 A(V) = 0.9 Comments: Object in the galaxy is a stellar cluster Target_Number: 4 Target_Name: NGC5253-UV3 Alternate_Names: Description: EXT-MEDIUM, HII REGION Position: RA-OFF=3.63S+/- 0.01S,DEC-OFF=33.70"+/- 0.1",FROM 1 Equinox: J2000 RV_or_Z: V = +400 RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: SURF(V) = 18.4+/-0.2 B-V = 0.0 A(V) = 0.9 Comments: Object in the galaxy is a stellar cluster Target_Number: 5 Target_Name: NGC5253-HII-1 Alternate_Names: Description: EXT-MEDIUM, HII REGION Position: RA-OFF=4.061S+/- 0.01S,DEC-OFF=37.31"+/- 0.1",FROM 1 Equinox: J2000 RV_or_Z: V = +400 RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: SURF(V) = 18.4+/-0.2 B-V = 0.0 A(V) = 0.9 Comments: Object in the galaxy is location in an HII region suspected to be N enriched Target_Number: 6 Target_Name: NGC5253-HII-2 Alternate_Names: Description: EXT-MEDIUM, HII REGION Position: RA-OFF=4.007S+/- 0.01S,DEC-OFF=39.13"+/- 0.1",FROM 1 Equinox: J2000 RV_or_Z: V = +400 RA_PM: 0.0 Dec_PM: 0.0 Epoch: Annual_Parallax: 0.0 Flux: SURF(V) = 18.4+/-0.2 B-V = 0.0 A(V) = 0.9 Comments: Object in the galaxy is location in an HII region far from the N enriched location Solar_System_Targets Generic_Targets Scan_Data Visits Visit_Number: 01 Visit_Requirements: On_Hold_Comments: Visit_Comments: To be coordinated with Kobulnicky and Skillman (6021) NGC 5253 observations which comprises an additional visit. Exposure_Number: 1 Target_Name: STAR-OFFSET Config: FOS/RD Opmode: ACQ/PEAK Aperture: 4.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: SEARCH-SIZE-X=1,SEARCH-SIZE-Y=3,SCAN-STEP-Y=1.23 Number_of_Iterations: 1 Time_Per_Exposure: 1S Special_Requirements: ONBOARD ACQ FOR 2 Comments: Pattern A on offset star Exposure_Number: 2 Target_Name: STAR-OFFSET Config: FOS/RD Opmode: ACQ/PEAK Aperture: 1.0 Sp_Element: MIRROR Wavelength: Optional_Parameters: SEARCH-SIZE-X=6,SEARCH-SIZE-Y=2,SCAN-STEP-X=0.61,SCAN-STEP-Y=0.61 Number_of_Iterations: 1 Time_Per_Exposure: 1S Special_Requirements: ONBOARD ACQ FOR 3 Comments: Pattern B1 on offset star Exposure_Number: 3 Target_Name: STAR-OFFSET Config: FOS/RD Opmode: ACQ/PEAK Aperture: 0.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: SEARCH-SIZE-X=5,SEARCH-SIZE-Y=5,SCAN-STEP-X=0.17,SCAN-STEP-Y=0.17 Number_of_Iterations: 1 Time_Per_Exposure: 1S Special_Requirements: ONBOARD ACQ FOR 4-34 Comments: Pattern D1 on offset star to achive 0."1 centering, errors will then be dominated by errors in offsets Exposure_Number: 4 Target_Name: NGC5253-UV1 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 99S Special_Requirements: Comments: Exposure_Number: 5 Target_Name: NGC5253-UV1 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G780H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 2000S Special_Requirements: Comments: Exposure_Number: 6 Target_Name: NGC5253-UV1 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G570H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 185S Special_Requirements: Comments: Exposure_Number: 7 Target_Name: NGC5253-UV1 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G400H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 90S Special_Requirements: Comments: Exposure_Number: 8 Target_Name: NGC5253-UV1 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 240S Special_Requirements: Comments: Exposure_Number: 9 Target_Name: NGC5253-UV1 Config: FOS/RD Opmode: ACQ Aperture: 4.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 20S Special_Requirements: Comments: Exposure_Number: 10 Target_Name: NGC5253-UV2 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 250S Special_Requirements: Comments: Exposure_Number: 11 Target_Name: NGC5253-UV2 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 90S Special_Requirements: Comments: Exposure_Number: 12 Target_Name: NGC5253-UV2 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G400H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 90S Special_Requirements: Comments: Exposure_Number: 13 Target_Name: NGC5253-UV2 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G570H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 185S Special_Requirements: Comments: Exposure_Number: 20 Target_Name: NGC5253-UV2 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G780H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 1870S Special_Requirements: Comments: Exposure_Number: 21 Target_Name: NGC5253-UV3 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G780H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 2390S Special_Requirements: Comments: Exposure_Number: 22 Target_Name: NGC5253-UV3 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G570H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 550S Special_Requirements: Comments: Exposure_Number: 23 Target_Name: NGC5253-UV3 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G400H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 300S Special_Requirements: Comments: Exposure_Number: 24 Target_Name: NGC5253-UV3 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G270H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 200S Special_Requirements: Comments: Exposure_Number: 25 Target_Name: NGC5253-UV3 Config: FOS/RD Opmode: ACCUM Aperture: 1.0 Sp_Element: G190H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 600S Special_Requirements: Comments: Exposure_Number: 31 Target_Name: NGC5253-UV3 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 1380S Special_Requirements: Comments: Exposure_Number: 32 Target_Name: NGC5253-UV2 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 1040S Special_Requirements: Comments: Exposure_Number: 33 Target_Name: NGC5253-UV1 Config: FOS/BL Opmode: ACCUM Aperture: 1.0 Sp_Element: G130H Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 1000S Special_Requirements: Comments: Exposure_Number: 34 Target_Name: NGC5253-UV1 Config: FOS/BL Opmode: ACQ Aperture: 4.3 Sp_Element: MIRROR Wavelength: Optional_Parameters: Number_of_Iterations: 1 Time_Per_Exposure: 20S Special_Requirements: SAME POS AS 33 Comments: Data_Distribution ! 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