0
Assigned ID: 5427
----- Attempting Submission 1 (Tue Mar 26 14:32:27 GMT 2024) -----
HOPR 92995 - approved to repeat two exposures from the failed visit 18. I have copied the failed exposures to a new visit 20.
-690801099
----- Attempting Submission 1 (Tue Jul 09 16:00:32 GMT 2024) -----
----- Attempting Submission 2 (Fri Jul 12 10:42:31 GMT 2024) -----
----- Attempting Submission 3 (Fri Nov 22 15:09:21 GMT 2024) -----
GHOSTBUSTERS: Determining the origin of tidal disruption events with a high-resolution survey of their host galaxies
Tidal disruption events (TDEs) of stars by supermassive black holes offer an unprecedented opportunity to map the properties of otherwise quiescent (and intermediate mass) black holes, including their mass distribution, occupation fraction, and growth over cosmic history, as well as studying disk formation, accretion and the launching of jets in real time. However, the observed properties of TDEs have posed several challenges, chief among which is the unexpected nature of their host galaxies. Up to 30% of TDEs occur in quiescent Balmer-strong (or post-starburst) galaxies - a class that makes up ~1% of the general galaxy population. Explanations include disturbed radial density profiles, nuclear starbursts, and recent mergers, but distinguishing between these channels is only possible by resolving structure on scales <100 pc. We propose a new survey, Galaxies HOSting Tdes: BUlges, STarbursts and mergERS (GHOSTBUSTERS), to fully map the properties of TDE hosts with a volume-limited sample out to ~200 Mpc, increasing by a factor 6 the TDE host sample with HST imaging and halving the median distance. Maximising the UV and high-resolution abilities of HST uniquely allows us to (i) measure the radial density profiles and stellar mass within <100pc of the SMBH, determining whether central over-densities drive the TDE rate; and (ii) map the spatial distribution of star formation to determine whether it shuts off from the inside-out or outside-in, and whether any residual star-formation is important to the rate of TDEs, and (iii) detect low surface-brightness features (shells, tails) indicating past mergers, while deliver a legacy data set with high value to the community.
Imaging survey of TDE host galaxies. These are extended sources, varying from ~10-30 arcseconds. Want to acquire WFC3 UVIS images in F225W, F438W and F625W, using standard 4-point dithering. Should fit galaxy on one chip to avoid gaps, and place on optimal position for charge transfer.
This proposal represents a broad community effort, with representation from a large number of groups working on TDEs.
Our team have extensive expertise in the study of transients - including TDEs, SNe and GRBs - and their hosts (Nicholl, Berger, Alexander, Blanchard, Gomez, Hosseinzadeh, Gompertz, Oates, Hiramatsu). Many of us are members of the TDE group within the ePESSTO+ (Nicholl, Short, Leloudas, Wevers, Onori, Gromadzki, Arcavi, Mattila, Perez-Torres, Mandel, Horesh, Ridley, Jonker), ZTF (Nicholl, van Velzen, Gezari, Veilleux, Hammerstein, Cenko, Stein, Somalwar), and ATLAS (Nicholl, Smartt, Srivastav, Moore, Fulton, McCollum) surveys that have classified and published many of the TDEs in this proposal. We also have experience in studying the relevant aspects of galactic and stellar evolution (McGee, French, Stevance) and AGN (Lawrence). The data in this program would form the basis of the PhD project of Co-I Ramsden.
We have substantial experience using HST for studying transient host galaxies (Nicholl et al. 2018, 2020, Blanchard et al. 2017, 2018, Hosseinzadeh et al. 2019...), and analysing galaxy properties such as star-formation history (Blanchard et al. 2017b, Nicholl et al. 2019, Gomez et al. 2020) and relations between SMBHs and their environments (McGee 2013). In particular, co-I French is a leader in QBS galaxies and conducted the previous work on TDE hosts with HST (French et al. 2020). Co-I Graur produced the largest statistical sample of TDE hosts to date. Several Co-Is (Nicholl, Leloudas) are also conducting a MUSE survey with complementary IFU spectroscopy, covering several of the same galaxies targeted in this proposal.
Co-Is Lu and Mummery are experts in the theoretical modeling of tidal disruption events and black hole accretion disks.
Stellar Physics and Stellar Types
Supermassive Black Holes and Active Galaxies
6
false
false
true
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No
No
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