Periodic Reporting for period 1 - DIGESTIVO (The DIffuse Galaxy Expansion SignaTures In Various Observables project: understanding the emergence of diffuse, low surface brightness galaxies and the link to their dark matter haloes) Reporting period: 2018-02-01 to 2020-01-31 Summary of the context and overall objectives of the project The DIGESTIVO project has been a joint theoretical and observational effort alongside theoreticians(with me, the fellow, as leader), and observers at the IAC to study the evolution and formation of Low Surface Brightness galaxies (LSBs), including the recentlydiscovered Ultra-Diffuse Galaxies (UDGs).LSBs are extremely dark matter dominated, faint objects hardly distinguishable from the night sky.In the last decade it had became clear that large numbers of LSB galaxies exist, opening a newwindow on galaxy evolution and formation.The specific scientific objectives and questions that the ‘DIGESTIVO’ project aimed to answer were:1. What processes lead to the emergence of such diffuse galaxies? Is the existence of such galaxiespredicted within the current model of galaxy formation, the Λ cold-DM paradigm? How are theylinked to their dark matter haloes?2. What is the DM and baryons content of low surface brightness galaxies? Do they have gas andhow much? What is their HI gas profile? Is it as extended as the one in simulations? What are theirvirial masses? Are they all dwarf-like or is there evidence for some of them being Milky Way-massobjects?3. What is the role of environment in forming LSBs and UDGs? Are UDGs only found in dense regionssuch as clusters of galaxies?To answer these questions, I made use of state-of-the-art, sophisticated hydrodynamical numericalsimulations of galaxies, combined with new observational data of LSBs/UDGs,some of which attained by observers at the host institution (IAC) thanks to new techniques thatpushed the frontier of LSB imaging with optical telescopes. Work performed from the beginning of the project to the end of the period covered by the report and main results achieved so far In this study, led by myself and done in collaboration with theoreticians at the host institutions andin Abu Dhabi, we investigated for the first time the origin of massive Low Surface Brightness (LSB)galaxies in hydrodynamical simulations, and explored their formation mechanism: simulated LSBsform as a result of co-planar co-rotating mergers and aligned accretion of gas at early times, whileperpendicular mergers and mis-aligned gas accretion result in higher SB galaxies by z=0.Interestingly, the formation scenario of such `classical' LSBs differs from the one of less massive,Ultra-Diffuse Galaxies, the latter resulting from the effects of SNae driven gas outflows: a stellarMass of 109 solar masses thus represents the transition regime between a feedback dominated toan angular momentum dominated formation scenario in the LSB realm. Observational predictionswere offered regarding spatially resolved star formation rates through LSB discs: these, togetherwith upcoming surveys, will be used to verify the proposed emergence scenario of LSB galaxies.On the morphology, rotation and kinematics of UDGs.In this work, led by Master student Cardona-Barrero under my supervision, and in collaborationwith observers at host institution, we addressed the topic of kinematical properties of UDGs byanalyzing the stellar kinematics of isolated UDGs formed in the hydrodynamical simulation suiteNIHAO. We found that UDGs cover a broad distribution, ranging from dispersion to rotationsupported galaxies, with similar abundances in both regimes. We demonstrated that the alignmentof the infalling baryons into the protogalaxy at early z is the principal driver of the z=0 stellarkinematic state: pressure supported isolated UDGs form via mis-aligned gas accretion while rotationsupported ones build-up their baryons in an ordered mannerOn the dark matter content of diffuse galaxies.In this work, coauthored by observational and theoretical researchers at the host institution and led by Dr. Trujillo,we haved carried out a careful analysis of all existing data and showed that for this galaxy, the dataconsistently indicated a much shorter distance (13 Mpc) than previously indicated (20 Mpc). Withthis revised distance, the galaxy appears to be a rather ordinary low surface brightness galaxy withplenty of room for dark matter, with a minimum halo mass >109 Msun.On the stellar populations, age and metallicity of LSBs/UDGs.In this observational work led by Dr. Ruiz-Lara and colleagues at the host institution, we have performed one of the mostcomplete characterizations of the stellar component of UDGs to date using deep opticalspectroscopic data from OSIRIS at Gran Telescopio CANARIAS (GTC). We find that their rotationproperties are compatible with dwarf galaxies. We have concluded that the UDGs in our sample areextended dwarfs whose properties are likely the outcome of both internal processes, such as burstySFHs and/or high-spin haloes, as well as environmental effects within the Coma cluster.On the environmental dependence of diffuse galaxies.This work has been led by theoretical colleagues at The Hebrew University of Jerusalem (Dr.Fangzhou and Dekel), with me as co-author. We studied ultra-diffuse galaxies (UDGs) in zoom incosmological simulations, seeking the origin of UDGs in the field versus galaxy groups. We foundthat while field UDGs arise from dwarfs in a characteristic mass range by multiple episodes ofsupernova feedback (as in my original paper Di Cintio et al.2017) group UDGs may also form bytidal puffing up and they become quiescent by ram-pressure stripping.Aside from scientific publications, the results of the DIGESTIVO project were disseminated andpresented in 12 seminars, conferences and workshops, and in several outreach activities such as‘The Researchers Night of Macaronesia’ (La Laguna, Spain, 2018), through virtual visits to spanishschools during the day of girls and women in science (Habla con Ellas: Mujeres en Astronomía,2019) and at university fairs, such as the event ‘La ciencias en porciones’, (La Laguna, Spain, 2020).Furthermore, I have organized 5 international conferences during the fellowship period, 2 of whichdirectly related to the project, such as ‘The Bewildering Nature of Ultra-diffuse Galaxies’, a fullyfunded workshop at Lorentz Center, Leiden, in 2018. Progress beyond the state of the art and expected potential impact (including the socio-economic impact and the wider societal implications of the project so far) Beyond the state-of-the-art, we made specific predictions for how to use and exploit our results inthe light of future observational surveys. Specifically:i) accounting for random inclination effects, we predicted that a comprehensive survey will findnearly half of field UDGs to have rotationally supported stellar disks, when selecting UDGs witheffective radius larger than 1 kpc;ii) observational predictions were offered regarding spatially resolved star formation rates throughLSB discs: these, together with upcoming surveys, will be used to verify the proposed emergencescenario of LSB galaxies.In the 2 years of fellowship I have learnt about observational data, instrumentslimitations and capability, while simultaneously offered my expertise in theoretical astrophysics andgalaxy formation and simulations to observers at IAC.The success of the transfer of knowledge and the vast impact of the project is clear from the largenumber of scientific publications that I have co-authored with the host institution colleagues.This was the first time that a joint theoretical and observational effort on the low surface brightnessuniverse was developed: ultimately, this project has offered invaluable insights on the formation ofsuch elusive galaxies and increased our understanding of the role of baryonic feedback in galaxyformation. digestivo-img.png