16837( 2) - 24-Sep-2021 16:48:23 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 16837 Version: 2 Check-in Time: 24-Sep-2021 16:48:23 STScI Edit Number: 0 Title Mapping the Activity of the LINER I NGC 5005 from ~30 pc out to kpc scales ------------------------------------------------------------------------------------ Type Cycle GO 29 ------------------------------------------------------------------------------------ Investigators Contact? PI: Dr. Giuseppina Fabbiano Smithsonian Institution Astrophysical Y Observatory CoI: Dr. Martin Elvis Smithsonian Institution Astrophysical N Observatory CoI: Dr. Walter Peter Maksym III Smithsonian Institution Astrophysical N Observatory CoI: Dr. Alessandro Paggi University of Torino N CoI: Dr. Jingzhe Ma Smithsonian Institution Astrophysical N Observatory CoI: Dr. Margarita Karovska Smithsonian Institution Astrophysical N Observatory CoI: Dr. Aneta Siemiginowska Smithsonian Institution Astrophysical N Observatory CoI: Dr. Chiara Feruglio INAF, Osservatorio Astronomico di Trieste N ------------------------------------------------------------------------------------ Abstract 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. ------------------------------------------------------------------------------------ Observations Description ------------------------ 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 16837( 2) - 24-Sep-2021 16:48:23 - [ 2] 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. ------------------------------------------------------------------------------------ 16837( 2) - 24-Sep-2021 16:48:23 - [ 3] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-5005 GALAXY, EMISSION LINE RA=13H10M56.3120S, J2000 V = 13.67 NEBULA, LINER, NLR, DEC=+37D03'32.19" NUCLEUS Reference Frame: Other: SIMBAD Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2015.5 0.0 0.0 0.0 ------------------------------------------------------------------------------------------------------------------------------------ 16837( 2) - 24-Sep-2021 16:48:23 - [ 4] Patterns ------------------------------------------------------------------------------------------------------------------------------------ Pattern_Number: 1 Primary_Pattern Secondary_Pattern Pattern_Type WFC3-UVIS-DITHER-BOX Pattern_Purpose DITHER Number_Of_Points 4 Point_Spacing 0.173 Line_Spacing 0.112 Coordinate_Frame POS-TARG Pattern_Orient 23.884 Angle_Between_Sides 81.785 Center_Pattern NO ------------------------------------------------------------------------------------------------------------------------------------ 16837( 2) - 24-Sep-2021 16:48:23 - [ 5] Visit: 01 (NGC 5005 [O III]) Visit Requirements: On Hold Comments: Additional Comments: 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-5005 WFC3/UVI ACCUM UVIS F502N FLASH=17 1 1300 S PATTERN 1 1-2 S see below (5928 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-5005 WFC3/UVI ACCUM UVIS F502N FLASH=17 1 1000 S S see below (4728 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-5005 1 WFC3/UVI ACCUM UVIS F502N 1 none none none 1 1485.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F502N 2 none none none 2 1481.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F502N 3 none none none 3 1481.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F502N 4 none none none 4 1481.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F502N 1 none none none 1 1185.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F502N 2 none none none 2 1181.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F502N 3 none none none 3 1181.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F502N 4 none none none 4 1181.0 S S 16837( 2) - 24-Sep-2021 16:48:23 - [ 6] Visit: 02 (NGC 5005 H-beta) Visit Requirements: On Hold Comments: Additional Comments: 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-5005 WFC3/UVI ACCUM UVIS F487N FLASH=17 1 1300 S PATTERN 1 1-2 S see below (5928 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-5005 WFC3/UVI ACCUM UVIS F487N FLASH=17 1 1000 S S see below (4728 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-5005 1 WFC3/UVI ACCUM UVIS F487N 1 none none none 1 1485.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F487N 2 none none none 2 1481.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F487N 3 none none none 3 1481.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F487N 4 none none none 4 1481.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F487N 1 none none none 1 1185.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F487N 2 none none none 2 1181.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F487N 3 none none none 3 1181.0 S S NGC-5005 2 WFC3/UVI ACCUM UVIS F487N 4 none none none 4 1181.0 S S 16837( 2) - 24-Sep-2021 16:48:23 - [ 7] Visit: 03 (NGC 5005 [S II]) Visit Requirements: On Hold Comments: Additional Comments: 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-5005 WFC3/UVI ACCUM UVIS F673N FLASH=17 1 1300 S PATTERN 1 1 S see below (5333 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-5005 1 WFC3/UVI ACCUM UVIS F673N 1 none none none 1 1353.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F673N 2 none none none 1 1318.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F673N 3 none none none 2 1331.0 S S NGC-5005 1 WFC3/UVI ACCUM UVIS F673N 4 none none none 2 1331.0 S S 16837( 2) - 24-Sep-2021 16:48:23 - [ 8] Visit: 04 (NGC 5005 H-alpha) Visit Requirements: On Hold Comments: Additional Comments: 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. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-5005 WFC3/UVI ACCUM UVIS F658N FLASH=17, CR-SPLIT=2 1 695 S (695 S S) ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-5005 WFC3/UVI ACCUM UVIS F547M FLASH=17, CR-SPLIT=2 1 695 S (695 S S) ------------------------------------------------------------------------------------------------------------------------------------ 3 NGC-5005 WFC3/UVI ACCUM UVIS F814W FLASH=12, CR-SPLIT=2 1 695 S S (680.5 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-5005 1 WFC3/UVI ACCUM UVIS F658N none none none 1 1 N/A S NGC-5005 1 WFC3/UVI ACCUM UVIS F658N none none none 2 1 N/A S NGC-5005 2 WFC3/UVI ACCUM UVIS F547M none none none 1 1 N/A S NGC-5005 2 WFC3/UVI ACCUM UVIS F547M none none none 2 1 N/A S NGC-5005 3 WFC3/UVI ACCUM UVIS F814W none none none 1 1 N/A S NGC-5005 3 WFC3/UVI ACCUM UVIS F814W none none none 2 1 333.0 S S 16837( 2) - 24-Sep-2021 16:48:23 - [ 9] Summary Form for Proposal 16837 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures UVIS ------------------------------------------------------------------------------------------------------------------------------------ Configurations WFC3/UVIS ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACCUM ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters CR-SPLIT=2, FLASH=12, FLASH=17 ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements PATTERN 1 1, PATTERN 1 1-2 ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements F487N, F502N, F547M, F658N, F673N, F814W ------------------------------------------------------------------------------------------------------------------------------------ Target Names NGC-5005 ------------------------------------------------------------------------------------------------------------------------------------