0 Assigned ID: 4504 ----- Attempting Submission 1 (Wed May 24 18:49:24 GMT 2023) ----- POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures. The following changes were made: 1) The coordinates of the targets are centered in the middle between the two nuclei, for galaxies with separations >10" 2) Exact central wavelength of the emission lines for the ramp filters. 3) We assigned two orbits to the galaxies that originally had 2 orbits in Phase I. In other words, we found that there is no need for swapping the orbits between the targets. 1932872059 ----- Attempting Submission 1 (Thu Sep 14 07:54:34 GMT 2023) ----- ----- Attempting Submission 2 (Fri Dec 08 11:36:16 GMT 2023) ----- ----- Attempting Submission 3 (Wed Dec 13 04:12:17 GMT 2023) ----- ----- Attempting Submission 4 (Fri Feb 23 15:21:57 GMT 2024) ----- The Visit Planner was not run, since visits are already scheduled The following changes were made: 1) The coordinates of the targets are centered in the middle between the two nuclei, for galaxies with separations >10" 2) Exact central wavelength of the emission lines for the ramp filters. 3) We assigned two orbits to the galaxies that originally had 2 orbits in Phase I. In other words, we found that there is no need for swapping the orbits between the targets. Probing SMBH/Galaxy Co-Evolution with Dual and Binary AGN A fundamental role is attributed to major mergers and supermassive black holes in the evolution of galaxies. But theoretical models trying to explain the role of galaxy mergers in the fueling and evolution of active galactic nuclei (AGN) have to make broad assumptions about the physical processes involved, and the prescriptions used are poorly constrained. Dual AGN, which are kpc-scale separation AGN pairs in galaxy mergers, offer the unique opportunity to investigate complex processes that are rarely detected simultaneously: vigorous star formation, two AGN, outflowing winds of ionized gas and tidal distortions. To provide the much needed guidance on these relevant processes, we propose [O III] and Halpha imaging of the complete sample of confirmed dual AGN at z < 0.05 and the only confirmed binary AGN, 4C+37.11, using ACS narrow-band filters. HST imaging is the only way to achieve the angular resolution and sensitivity required to study the detailed morphologies of faint tidal tails, narrow-line regions (NLRs), gas clouds between the two nuclei and compact star-forming regions. With a minimal investment of 15 orbits for such astrophysically important objects, we will be able to answer the following key questions: (i) how does merger dynamics contribute to the onset of star formation and AGN? (ii) how do the NLRs from the two AGN combine during the merger process? and (iii) what are the relative timescales and energetics of AGN- and star formation-driven outflows during different phases of the merger sequence? HST has observed only one dual AGN with narrow-band filters. This program will deliver a legacy of morphological data of dual AGN for studies of galaxy evolution. We aim to obtain HST narrow band [O III] and Halpha images for all the galaxies in our program using ACS narrow and medium filters. The ACS ramp filters provide the spectral coverage we require for our observations. The high sensitivity of ACS ensures that we will get very high signal to noise ratio (SNR) images (> 100) of the central regions of each system and reach even their outskirts and low surface brightness regions at SNR> 5 in a ~3' x 3' FOV. We need both [O III] and Halpha in order to separate gas ionized by the AGN from star forming material. For [O III] we will use FR505 and for Halpha FR656 or FR716N depending on the redshift of the galaxy. Precise continuum subtraction is also vital. For this, medium band filters are ideal, as they are close in wavelength, and can be chosen to be free of strong lines, but still produce plenty of SNR. For [O III] we will use F550M, and for Halpha we will use FR647M. A one-orbit visit will devote 1200 s of exposure to [O III] and 300 s to Halpha, giving the same or somewhat higher SNR expected in the latter. The remaining 300 s of exposure time will be apportioned between the continuum filters F550M and FR647M, with a 4 to 1 ratio (240 s for the blue filters and 60 s for the red filters). For each target, there will be 21 min of overheads (7 min for guide-star acquisition and 14 min for filter change and readout). The total time spent on science exposures and overheads is ~51 min. We checked the V-magnitude of our targets and we are now using two orbits for ESO 509-66, 4C+37.11 and IRAS 01197+0044. For the rest of the galaxies one orbit is sufficient. Our team combines an extensive experience in the reduction and analysis of HST data of nearby AGN and galaxy mergers, particularly with ACS and WFC3. We have developed all the necessary tools to analyze HST images in a timely fashion. Dr. Francisco Muller-Sanchez is an expert in galaxy evolution and dynamics, particularly AGN and their outflows. He has led several past HST observing campaigns with 9 papers published in the past decade on data analysis carried out with HST observations. In particular, he reduced and analyzed the HST images of the galaxy NGC 6240, which appear in the publication: Muller-Sanchez et al. (2018, Nature, 556, 345). In addition, he is currently leading the analysis and modeling of the kinematics of the gas in nearby AGN and confirmed dual AGN. Dr. Julia Comerford has extensive experience in multiwavelength studies of dual AGN. The program will benefit from her experience with the wide range of available ancillary data to ensure that the interpretation of the kinematics within the central 200 pc is consistent with what is known for each galaxy on larger scales and at a broad range of wavelengths (e.g. X-ray, optical, mid-IR, etc.). Dr. Ezequiel Treister is an expert in multiwavelength selectors of AGN. He will assist in the data reduction and interpretation of the physical properties of the NLR (e.g., emission-line ratios and excitation mechanisms), and merger induced inflows. Dr. George Privon has extensive experience working with optical and near-IR images from HST (e.g., Privon et al. 2018, ApJ, 846, 74). He also has experience in the computational simulations of galaxy mergers that will be required to interpret these data. Co-I M. Ruby is a second-year graduate student at the University of Memphis. In 2018 he graduated from Union University in Jackson, TN with a BS in Physics with Honors. He is working under Dr. Muller-Sanchez supervision at the University of Memphis and plans to earn a PhD studying galaxy mergers and their effects on AGN activity. He also has interests in creating data reduction and other support software. 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J2000 J2000 GALAXY INTERACTING GALAXY MULTIPLE NUCLEI NLR TIDAL TAIL WIND This object was generated by the targetselector and retrieved from the NED database. J2000 J2000 ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR716N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR716N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR656N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR716N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR716N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR656N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR656N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR656N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR656N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR656N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR716N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M ACS/WFC RampFilter No No FR505N ACS/WFC RampFilter No No FR656N ACS/WFC RampFilter No No FR647M ACS/WFC Imaging No No F550M POS-TARG DITHER 3.034 LINE false false 2 85.29 ACS-WFC-DITHER-LINE 1 false /private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit13141036491658116810.xml The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. (Tic-Visit :proposal-id 17512 :visit-id "01" :proposal-version -1 :trans-version "20240604" :date "14-Jun-2024 09:47:56.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 852752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17512 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17512 :visit-id "01" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2643 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3023 :pcs-gap 0 ) true 1 0 /private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit277533210046146043.xml The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. (Tic-Visit :proposal-id 17512 :visit-id "02" :proposal-version -1 :trans-version "20240604" :date "14-Jun-2024 09:48:32.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 568608 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17512 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17512 :visit-id "02" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2752 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3005 :pcs-gap 0 ) (Tic-Orbit :proposal-id 17512 :visit-id "02" :orbit-number 2 :pcs-time 380 :si-vis-utilization 2564 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3005 :pcs-gap 0 ) true 2 1 /private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit17841878409198442612.xml The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. (Tic-Visit :proposal-id 17512 :visit-id "03" :proposal-version -1 :trans-version "20240604" :date "14-Jun-2024 09:47:56.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 426464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17512 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17512 :visit-id "03" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2648 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3028 :pcs-gap 0 ) true 1 0 /private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit2781872794615634620.xml The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. (Tic-Visit :proposal-id 17512 :visit-id "04" :proposal-version -1 :trans-version "20240604" :date "14-Jun-2024 09:47:57.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 852752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17512 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17512 :visit-id "04" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2649 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3032 :pcs-gap 0 ) true 1 0 /private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit3883896826751337361.xml The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. 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(Tic-Visit :proposal-id 17512 :visit-id "10" :proposal-version -1 :trans-version "20240604" :date "14-Jun-2024 09:48:01.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 426464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17512 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17512 :visit-id "10" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2626 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3010 :pcs-gap 0 ) true 1 0 /private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit10395441312410288239.xml The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. (Tic-Visit :proposal-id 17512 :visit-id "11" :proposal-version -1 :trans-version "20240604" :date "14-Jun-2024 09:48:02.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 426464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17512 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17512 :visit-id "11" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2657 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3039 :pcs-gap 0 ) true 1 0 /private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit11838987263968716311.xml The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. 1711377767000 99.5 (Tic-Visit :proposal-id 17512 :visit-id "12" :proposal-version -1 :trans-version "20240604" :date "14-Jun-2024 09:48:52.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 426464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17512 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17512 :visit-id "12" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2752 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3015 :pcs-gap 0 ) true 1 1