Science Keywords: Select from 2 to 5 items. Science Keywords is a required field. 0 Assigned ID: 2557 ----- Attempting Submission 1 (Wed Sep 15 12:17:22 GMT 2021) ----- Joint Chandra/HST POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. 0 ----- Attempting Submission 1 (Fri Oct 08 16:18:09 GMT 2021) ----- HST Phase II Proposal 16841 successfully submitted. Receipt: # 16841-1 ----- Attempting Submission 2 (Mon Oct 11 15:45:46 GMT 2021) ----- HST Phase II Proposal 16841 successfully submitted. Receipt: # 16841-2 ----- Attempting Submission 3 (Mon Oct 11 21:24:44 GMT 2021) ----- HST Phase II Proposal 16841 successfully submitted. Receipt: # 16841-3 ----- Attempting Submission 4 (Wed Oct 13 14:23:22 GMT 2021) ----- We have checked the FOV in Aladin to ensure good coverage. We propose deep Chandra ACIS observations and joint HST narrow band imaging of the nearby Compton-thick AGN ESO137-G034. The recent Chandra discovery of extended kpc-scale hard X-ray continuum (3-6 keV) and Fe Ka emission in Compton-thick AGN provides physical constraints on the obscuring torus and demonstrates the impact of the supermassive black hole (SMBH) on the host galaxy via feedback. Comparing deep Chandra data with multi-wavelength high resolution data (e.g. HST, ALMA, VLT/SINFONI), we will conduct an unprecedented comprehensive analysis of the extended X-ray emission, and the multi-phase interstellar media (i.e. cold and warm molecular gas, ionized gas, and dust) at sub-arcsec resolution to ultimately understand how the central SMBH interacts with and impacts the host galaxy. We are conducting new WFC3/UVIS narrow band imaging of [SII]6717,6730 and Hbeta, and corresponding continuum observations. Together with archival narrow band images of [OIII]5007 and Halpha, we will perform spacially resolved BPT mapping and diagnose excitation mechanisms in the different regions of NLR in ESO137-G034. Based on the archival WFPC2 data of ESO137-G034 and our experience with silimar Seyfert galaxies, we designed the program to be conducted with one orbit per line. At z = 0.0090, [S II] lines shift to the F673N filter and we use the F763M filter to get the continuum, which is far enough from the Halpha complex. We initially planned to use the narrow filter F645N for [SII] continuum following our successful Cycle 25 program. For Hbeta, we need to use the quad filter FQ492N. We will use F547M for the contiuum, which is slightly contaminated by the [OIII]5007 line at very low throughput but can be modeled. We initially planned to use the archival [OIII] continuum as the continuum for Hbeta. Given that there is enough time, we would like to get a new continuum for Hbeta using the same instrument for easier data reduction and better quality. These medium band filters are broader and better for getting good continuum S/N than narrow band filters. The modification of continuum filters from Phase I are made due to more detailed checking of effective wavelength coverage, S/N, and actual available time. We use a 4-point dither pattern for the lines and a 2-point dither pattern for the continuum to better sample the PSF and for cosmic removal. We have checked the FOV in Aladin to ensure good coverage. n/a Supermassive Black Holes and Active Galaxies 6 false false false false false false false false SUPPORTED GALAXY NLR SEYFERT J2000 J2000 WFC3/UVIS Imaging No No F673N WFC3/UVIS Imaging No No F645N WFC3/UVIS Imaging No No FQ492N POS-TARG DITHER 0.173 LINE 0.112 false false 81.785 4 23.884 WFC3-UVIS-DITHER-BOX 1 false /Users/jingzhema/Desktop/OP-cache/HST_Cycle29_PhaseII-v01.xml 1633709727490 The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 16841 :visit-id "01" :proposal-version -1 :trans-version "20210514" :date "08-Oct-2021 12:15:27.0" :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 3464992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16841 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16841 :visit-id "01" :orbit-number 1 :pcs-time 383 :si-vis-utilization 3005 :al-overhead-at-end 127 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3389 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16841 :visit-id "01" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2997 :al-overhead-at-end 127 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3389 :pcs-gap 0 ) true 2 0