The HST-pNFL program: Mapping the Fluorescent Emission of Galactic Outflows

0 Assigned ID: 404 ----- Attempting Submission 1 (Fri Apr 07 05:26:43 GMT 2017) ----- The number of orbits used exceeds the number allocated For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. Sensitive exposures should have an ETC run number provided. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. Sensitive exposures should have an ETC run number provided. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. Sensitive exposures should have an ETC run number provided. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. Sensitive exposures should have an ETC run number provided. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. Sensitive exposures should have an ETC run number provided. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. Sensitive exposures should have an ETC run number provided. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. Sensitive exposures should have an ETC run number provided. Changed all COS exposures to G130M (1291). Used ETC is check that the S/N in these exposures will be sufficient for science goals. Changed to include segments A and B Changed to ACQ to Mirror A Changed FP = ALL to FP = 3 Added FP=4 exposures Adjusted exposure times to fill orbits Turned on FLASH = YES Changed to use dither pattern for WFC F280N exposures Visit 18 replaces failed Visit 15 visit 59 replaces failed visit 09 1398697746 ----- Attempting Submission 1 (Thu Jul 20 22:15:25 GMT 2017) ----- HST Phase II Proposal 15340 (HST_pNFL_Phase_II.apt) successfully submitted. Receipt: # 15340-1 ----- Attempting Submission 2 (Fri Jul 28 20:37:36 GMT 2017) ----- ----- Attempting Submission 3 (Mon Nov 20 22:06:28 GMT 2017) ----- ----- Attempting Submission 4 (Thu Feb 01 21:23:30 GMT 2018) ----- ----- Attempting Submission 5 (Fri Feb 02 21:04:13 GMT 2018) ----- ----- Attempting Submission 7 (Fri Mar 16 20:42:15 GMT 2018) ----- ----- Attempting Submission 9 (Mon Mar 19 19:28:18 GMT 2018) ----- ----- Attempting Submission 10 (Tue Apr 17 20:15:20 GMT 2018) ----- ----- Attempting Submission 11 (Thu May 24 16:53:21 GMT 2018) ----- ----- Attempting Submission 12 (Fri Nov 16 18:06:39 GMT 2018) ----- Our science contact told us those warnings are fine. They are just present to make sure we are aware of the limitations. There's nothing that can be done on our end and we will treat them with care at the data analysis stage. The HST-pNFL program: Mapping the Fluorescent Emission of Galactic Outflows Galactic outflows associated with star formation are believed to play a crucial role in the evolution of galaxies and the IGM. Most of our knowledge about outflows has come from "down-the-barrel" UV absorption spectroscopy of star-forming galaxies. However, absorption-line data alone provide only indirect information about the radial structure of the gas flows, which introduces large systematic uncertainties in some of the most important quantities, such as the outflow rate, the mass loading factor, and the momentum, metal, and energy fluxes. Recent spectroscopic observations of star-forming galaxies with large (projected physical) apertures have revealed non-resonant (fluorescent) emission in the UV, e.g., FeII* and SiII*, that can be naturally produced by spatially extended emission from the same outflowing material traced in absorption. Encouraged by the most recent observations of FeII* emission by the SDSS-IV/eBOSS survey (Zhu et al. 2015), we propose a pilot program to use narrow-band filter UVIS F280N images to map the extended FeII* 2626 and 2613 fluorescent emission in a carefully-chosen sample of 4 starburst galaxies at z=0.065, and COS G130M to obtain down-the- barrel spectra for SiII absorption and SiII* emission. This HST pilot program can provide unique information about the spatial structure of galactic outflows and can potentially lead to a revolution in our understanding of outflow physics and its impact on galaxies and the IGM. We have carefully selected 4 starburst systems to map the fluorescent emission halo. We will use WFC3 UVIS F280N narrow band to observe Fe II* 2613, 2626, and F343N and F395N for the continuum. In addition, we will use COS/FUV G130M to obtain FUV spectra of Si II* 1194. The combination of these observations will provide us with the direct constraints of outflow geometry for the first time. Galaxies and the IGM 6 false false true false false false false SUPPORTED GALAXY STARBURST YES This object was generated by the targetselector and retrieved from the GALEX database. J2000 J2000 GALAXY STARBURST YES This object was generated by the targetselector and retrieved from the GALEX database. J2000 J2000 GALAXY STARBURST YES This object was generated by the targetselector and retrieved from the GALEX database. J2000 J2000 GALAXY INTERACTING GALAXY STARBURST YES This object was generated by the targetselector and retrieved from the GALEX database. J2000 J2000 GALAXY INTERACTING GALAXY STARBURST YES This object was generated by the targetselector and retrieved from the GALEX database. J2000 J2000 WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F280N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F280N COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 POS-TARG DITHER 0.173 LINE 0.112 false false 81.785 4 23.884 WFC3-UVIS-DITHER-BOX 1

false

1523995880554 The scheduling data was generated by CASM 25.2. 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CASM was run in Phase II mode. /private/var/folders/dv/kllm6qvx1m3bq_0v7lp6wwtc000702/T/OPVisit1503538935313004296.xml 1541915119000 316.7583735973974 (Tic-Visit :proposal-id 15340 :visit-id "09" :proposal-version -1 :trans-version "20180927" :date "16-Nov-2018 12:15:12.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2933 :al-overhead-at-end 123 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3298 :pcs-gap 0 ) true 1 0 Target: [extended source] Source diameter (arcsec): 20.0 Spectrum: Non-stellar Objects Starburst SB2 Kinney Recalibrated [911.0, 25592.0] Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.02 applied before normalization Normalization: Renormalized to abmag = 25.0 in filter Galex/NUV Redshift: z=0.065 Emission Lines: None 1542388513361 /private/var/folders/dv/kllm6qvx1m3bq_0v7lp6wwtc000702/T/OPVisit1503538935313004296.xml HOPR repeat of visit 09 (Tic-Visit :proposal-id 15340 :visit-id "09" :proposal-version -1 :trans-version "20180927" :date "16-Nov-2018 12:15:12.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2933 :al-overhead-at-end 123 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3298 :pcs-gap 0 ) false 1 0 Target: [extended source] Source diameter (arcsec): 20.0 Spectrum: Non-stellar Objects Starburst SB2 Kinney Recalibrated [911.0, 25592.0] Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.02 applied before normalization Normalization: Renormalized to abmag = 25.0 in filter Galex/NUV Redshift: z=0.065 Emission Lines: None 1523995888235 The scheduling data was generated by CASM 25.2. 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CASM was run in Phase II mode. 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CASM was run in Phase II mode. (Tic-Visit :proposal-id 15340 :visit-id "12" :proposal-version -1 :trans-version "20171009" :date "17-Apr-2018 16:11:29.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2813 :al-overhead-at-end 123 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3202 :pcs-gap 0 ) true 1 0 Target: [extended source] Source diameter (arcsec): 20.0 Spectrum: Non-stellar Objects Starburst SB2 Kinney Recalibrated [911.0, 25592.0] Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.02 applied before normalization Normalization: Renormalized to abmag = 25.0 in filter Galex/NUV Redshift: z=0.065 Emission Lines: None 1523995890714 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1536013922000 21.2340631110649 (Tic-Visit :proposal-id 15340 :visit-id "13" :proposal-version -1 :trans-version "20171009" :date "17-Apr-2018 16:11:30.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 408848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 124 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15340 :visit-id "13" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3224 :al-overhead-at-end 0 :internal-dur-at-end 398 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 2 0 1527180782755 The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. 1536726006000 89.0 (Tic-Visit :proposal-id 15340 :visit-id "14" :proposal-version -1 :trans-version "20180409" :date "24-May-2018 12:52:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 521888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2871 :al-overhead-at-end 0 :internal-dur-at-end 426 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3225 :pcs-gap 0 ) true 1 0 1523995897964 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1521471846000 193.97515428683437 (Tic-Visit :proposal-id 15340 :visit-id "15" :proposal-version -1 :trans-version "20171009" :date "17-Apr-2018 16:11:37.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 495888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "15" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2949 :al-overhead-at-end 0 :internal-dur-at-end 369 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3298 :pcs-gap 0 ) true 1 0 1523995899014 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15340 :visit-id "16" :proposal-version -1 :trans-version "20171009" :date "17-Apr-2018 16:11:38.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 930672 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "16" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2869 :al-overhead-at-end 0 :internal-dur-at-end 76 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3202 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15340 :visit-id "16" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2974 :al-overhead-at-end 0 :internal-dur-at-end 417 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3202 :pcs-gap 0 ) true 2 0 1523995899913 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15340 :visit-id "17" :proposal-version -1 :trans-version "20171009" :date "17-Apr-2018 16:11:39.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 504528 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "17" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2869 :al-overhead-at-end 0 :internal-dur-at-end 76 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3202 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15340 :visit-id "17" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2974 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3202 :pcs-gap 0 ) true 2 0 1527180498934 This is a HOPR replacement of Visit 15 1531687322000 90.01603219449947 (Tic-Visit :proposal-id 15340 :visit-id "18" :proposal-version -1 :trans-version "20180409" :date "24-May-2018 12:48:17.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 521888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15340 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15340 :visit-id "18" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2911 :al-overhead-at-end 0 :internal-dur-at-end 426 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3298 :pcs-gap 0 ) true 1 0