Science Keywords: Select from 2 to 5 items. Science Keywords is a required field. Please specify your scheduling constraints or 'No Constraints' on all Observation forms. Please specify your scheduling constraints or 'No Constraints' on all Observation forms. Please specify your scheduling constraints or 'No Constraints' on all Observation forms. Please specify your scheduling constraints or 'No Constraints' on all Observation forms. 0 Assigned ID: 2553 ----- Attempting Submission 1 (Wed Sep 15 12:14:47 GMT 2021) ----- Joint Chandra/HST The chip gap should not a concern for this science program, but it may be possible to choose a better dither pattern that fills the gap for ancillary/archival science. 1584622222 ----- Attempting Submission 1 (Thu Sep 23 18:29:10 GMT 2021) ----- Mapping the Activity of the LINER I NGC 5005 from ~30 pc out to kpc scales High resolution multi-wavelength maps of the nuclear regions of active galaxies reveal an increasingly complex view, with AGN, LINER and star-formation co-existing in the same, often highly obscured, nucleus. The ongoing deep high resolution spectral-spatial mapping of Compton-thick (CT) AGNs with Chandra explores one aspect of this multi-faceted activity. However, there are no comparable X-ray studies of LINERs. We propose deep Chandra ACIS-S observations of the nearby (~17 Mpc) LINER NGC 5005 (250 ks), for which the archival snapshot suggests an extended ionized region, akin to an AGN ionization cone. To get a fuller detailed picture of the AGN-host interaction, we propose 11 orbits with HSTWFC3 for diagnostic optical emission line imaging. We aim to measure [O III], H-alpha, H-beta, the [S II] 6717,6731 and red & blue continua of NGC 5005. Ratios between continuum-subtracted line maps will be used to make "BPT maps" to diagnose the local ionization state. The overall goals are similar to Programs #15350 (PI: Maksym) and #15609 (PI: Fabbiano), as are the basic strategies. This program requires some changes with respect to specific filters, and it is a WFC3-only program. Our goal is to reach >3-sigma detection for all lines within <3 arcsec of the nucleus. This will require 4 orbits of [O III] (F502N), 4 orbits of H-beta (F487N), 2 orbits of [S II] (F673N) and <1 orbit of H-alpha (F658N). Even the faintest H-alpha regions will be detected at ~16-sigma in one orbit, so we pack the continuua into the H-alpha orbit. Given the number of exposures, it is possible to use a box dither to improve PSF sampling for [O III], H-beta and [S II]. H-alpha and continuum observations are short and use a CR-split. All exposures use pre-flash amounts that vary with exposure. n/a Supermassive Black Holes and Active Galaxies 6 false false false false false false false false SUPPORTED GALAXY EMISSION LINE NEBULA LINER NLR NUCLEUS This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F487N WFC3/UVIS Imaging No No F673N WFC3/UVIS Imaging No No F658N POS-TARG DITHER 0.173 WFC3-UVIS-DITHER-BOX 0.112 false false 81.785 4 23.884 WFC3-UVIS-DITHER-BOX 1 false /System/Volumes/Data/data/CXC/PROPOSALS/OP-cache/hst_jointcxc_NGC5005_phase2_v1-v01.xml The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. 4 orbits of exposure for NGC 5005 using F502N. The box dither pattern should improve resolution (should it become relevant), and 8 exposures should be okay for cosmic ray rejection even if the individual exposures are a little long. (Tic-Visit :proposal-id 16837 :visit-id "01" :proposal-version -1 :trans-version "20210514" :date "23-Sep-2021 13:33:18.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2309952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16837 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16837 :visit-id "01" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2816 :al-overhead-at-end 126 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16837 :visit-id "01" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2808 :al-overhead-at-end 126 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16837 :visit-id "01" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2808 :al-overhead-at-end 126 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16837 :visit-id "01" :orbit-number 4 :pcs-time 392 :si-vis-utilization 2808 :al-overhead-at-end 126 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) true 4 0 /System/Volumes/Data/data/CXC/PROPOSALS/OP-cache/hst_jointcxc_NGC5005_phase2_v1-v02.xml The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. 4 orbits of exposure for NGC 5005 using F487N. The box dither pattern should improve resolution (should it become relevant), and 8 exposures should be okay for cosmic ray rejection even if the individual exposures are a little long. (Tic-Visit :proposal-id 16837 :visit-id "02" :proposal-version -1 :trans-version "20210514" :date "23-Sep-2021 13:33:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2309952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16837 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16837 :visit-id "02" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2816 :al-overhead-at-end 126 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16837 :visit-id "02" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2808 :al-overhead-at-end 126 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16837 :visit-id "02" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2808 :al-overhead-at-end 126 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16837 :visit-id "02" :orbit-number 4 :pcs-time 392 :si-vis-utilization 2808 :al-overhead-at-end 126 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) true 4 0 /System/Volumes/Data/data/CXC/PROPOSALS/OP-cache/hst_jointcxc_NGC5005_phase2_v1-v03.xml The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. 2 orbits of exposure for NGC 5005 using F673N. The box dither pattern should improve resolution (should it become relevant), and 4 exposures should be okay for cosmic ray rejection even if the individual exposures are a little long. (Tic-Visit :proposal-id 16837 :visit-id "03" :proposal-version -1 :trans-version "20210514" :date "23-Sep-2021 13:33:20.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1154976 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16837 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16837 :visit-id "03" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2817 :al-overhead-at-end 126 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16837 :visit-id "03" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2808 :al-overhead-at-end 126 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) true 2 0 /System/Volumes/Data/data/CXC/PROPOSALS/OP-cache/hst_jointcxc_NGC5005_phase2_v1-v04.xml The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. 1 orbit of exposure for NGC 5005 using F673N, plus brief continuum observations with F547M and F814W. This was tricky to pack because of readout constraints for 6 exposures. One subexposure needed to be fixed. This setup should be checked for a different orbit length. (Tic-Visit :proposal-id 16837 :visit-id "04" :proposal-version -1 :trans-version "20210514" :date "23-Sep-2021 13:33:22.0" :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 1732496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16837 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16837 :visit-id "04" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2817 :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 3200 :pcs-gap 0 ) true 1 0