0 Assigned ID: 365 ----- Attempting Submission 1 (Fri Apr 08 03:16:34 GMT 2016) ----- Switched from UVIS1 to UVIS2 for additional sensitivity on the advice of Susana Deustua 612786157 ----- Attempting Submission 1 (Mon Jul 11 16:39:04 GMT 2016) ----- ----- Attempting Submission 2 (Wed Sep 28 22:31:12 GMT 2016) ----- A Local Laboratory for Studying Positive Feedback from Supermassive Black Holes AGN feedback is a critical regulator of galaxy growth. As well as curtailing star formation in diffuse, hot gas, it is increasingly understood to sometimes enhance star formation in the clumpy ISM through shock-induced collapse of clouds. Simulations have shown that such positive feedback may play a significant role in determining the stellar populations of galaxies. Minkowsi's Object (MO) provides an excellent local laboratory to probe this poorly-studied process in detail. The detection of a Type II supernova in MO (unexpected given the low mass of MO) suggests that jet-induced star formation may overproduce massive stars, and that models of the initial mass function in such systems may need to be revised. Recent results also suggest that star formation efficiency is enhanced in MO. Using WFC3, we will obtain morphologies, SEDs, H-a luminosities, equivalent widths, sizes, and population synthesis models of star forming regions across MO in order to address these questions, critical for understanding not just this single object, but the general process: 1. Does jet induced star formation change the luminosities and initial mass functions of star clusters? 2. What do the age gradients of the star clusters tell us about the process of conversion of gas (HI, CO) into stars as the radio jet progressed through the parent cloud? Does this match numerical simulations? 3. By using observations to refine simulations, what can we learn about intrinsic properties of these kinds of radio jets, such as propagation speed, age, pressure and jet energy flux? WFC3 Broad-Band UVIS and IR imaging: one orbit per filter in UVIS F336W, F438W, F555W, F814W and IR F125W. WFC3 Narrow-Band imaging for H-alpha at z = 0.01875, i.e. 6686 Angstroms: 2 orbits in UVIS F665N. Four point dither used. Massive Black Holes and their Hosts Galaxies 12 false true false false false 0.0 0.0 0 0.0 false SUPPORTED GALAXY STARBURST J2000 J2000 WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F438W WFC3/UVIS Imaging No No F555W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F125W WFC3/UVIS Imaging No No F665N POS-TARG DITHER DITHER 4 23.02 WFC3-IR-DITHER-BOX-MIN 35.212 false 74.653 true 0.365 89.287 0.572 4 0.713 POS-TARG WFC3-IR-DITHER-BOX-UVIS 18.528 1 false POS-TARG DITHER 0.173 LINE 0.112 false false 81.785 4 23.884 WFC3-UVIS-DITHER-BOX 2 false /private/var/folders/7w/f1klypgs5cd28l_v14czzw480000gn/T/OPVisit4352692188594098813.xml The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 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(Tic-Visit :proposal-id 14722 :visit-id "04" :proposal-version -1 :trans-version "20160601" :date "28-Sep-2016 15:30:32.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14722 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14722 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2876 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3210 :pcs-gap 0 ) true 1 0 /private/var/folders/7w/f1klypgs5cd28l_v14czzw480000gn/T/OPVisit8880279873628606688.xml The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 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