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Science Keywords is a required field.0Assigned ID: 2563
----- Attempting Submission 1 (Wed Sep 15 12:18:37 GMT 2021) -----Joint Chandra/HSTPOS 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.0----- Attempting Submission 1 (Sun Sep 26 19:32:30 GMT 2021) -----We have checked these warningsTRACING X-RAY EMISSION REGIONS IN MCG-03-34-64MCG-03-34-64 is a nearby Seyfert galaxy with extremely heavy X-ray absorption that makes it one of the hardest sources in the X-ray sky. Consequently this is a superb candidate for study of the faint, extended, circumnuclear X-ray emission. Chandra imaging results for other nearby Compton-thick AGN show structure on a scale of hundreds of pc coincident with the Narrow Line Region gas. Following on from those successful observations we request a 50 ks ACIS-S exposure to trace out the line emitting regions in MCG-03-34-64. We also ask for an HST orbit to map [Oiii] for comparison with the X-ray extent.The acquisition of the HST ACS/WFC [O III]5007A image for MCG -03-34-64 need not be simultaneous
and we simply request that this accompanying exposure be within cycle 22. Thus the Joint Observation
imposes no constraint on the Chandra scheduling. For HST, as our target has a redshift of z = 0.0165, we
will use the FR505N ramp filter. We also propose to obtain a continuum image, to subtract the continuum
contribution from the emission line image. We chose FR647M, with which we can select a region free from
emission lines. We estimate exposure times based previous observations of sources of similar [Oiii] flux
and redshift, where we find a typical 3 sigma surface brightnesses of ~ 10^-15 erg s^ -1 cm^-2 arcsec ^-2 . To
reach this sensitivity, we will require an [O III] exposure of ~ 30 minutes. Based on the archival images, for
the continuum images we will use 5 minutes of integration. The observations will be split into at least 2
exposures per band, to better eliminate cosmic rays, and apply drizzle patterns. Therefore, the imaging will
require 1 orbit in total.n/aSupermassive Black Holes and Active Galaxies6falsefalsefalsefalsefalsefalsefalse50trueSUPPORTEDGALAXYSEYFERTThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000ACS/WFCRampFilterNoNoFR505NACS/WFCRampFilterNoNoFR647MPOS-TARGDITHER3.034LINEfalsefalse285.29ACS-WFC-DITHER-LINE1falsePOS-TARGDITHER3.034LINEfalsefalse285.29ACS-WFC-DITHER-LINE2false/Users/turner/Downloads/OP-cache/MCG-03-34-64TJT-v01.xmlThe scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 16847
:visit-id "01"
:proposal-version -1
:trans-version "20210514"
:date "26-Sep-2021 15:26:45.0"
: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 1136896
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:coron NIL
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(Tic-Orbit
:proposal-id 16847
:visit-id "01"
:orbit-number 1
:pcs-time 383
:si-vis-utilization 2773
: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 3156
:pcs-gap 0
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