NameCountry of originSubject of dissertationConferring universityInstituteThesis committeAgrawal,AniketIndiaNon Gaussianity of Primordial Gravitational Waves and Cosmic Density and Velocity FieldsLMUMPAKomatsuGilfanovSchmidtChacón Tanarro, AnaSpainObservational studies of a dense cloud core on the verge of star formationLMUMPECaselliBizzochhiCoffey, DamienIrelandAGN Physics and Cosmology with Large-Area X-Ray SurveysLMUMPENandraSalvatoBollerMerloniDelvaux, CorentinBelgiumClassification engine for x-ra transients for eROSITATUMMPEGreinerSchadyDiehlGupta, NikhelIndiaHigh Frequency Cluster Radio Galaxies and the Sunyaev-Zel’dovich Effect Properties of Galaxy ClustersLMUUSMMohrHagstotz, SteffenGermanyLarge-Scale Structure Probes of Accelerated ExpansionLMUUSMWellerHeigl, StefanGermanyFragmentation in Interstellar FilamentsLMUUSMBurkertCaselliHacarHuber, KorbinianGermanyMethods for joint cluster reconstructionsLMUExc. Cluster UniverseBrukertHilbertWellerKakkad, DarshanIndiaIonized and Molecular gas studies to unveil AGN feedbackLMUESOBurkertPadovaniMainieriKnust, FabianGermanyApplying the Fireball Model to Short Gamma-Ray Burst Afterglows: Methods, Jet Opening Angles and Plateau PhasesTUMMPEGreinerEerteniOberauerPlewa, PhilippGermanyThe Galactic Center In MotionLMUMPEGenzelGillessenBurtscherTacconiPollina, GiorgiaItalyCosmic voids in large-scale structure surveysLMUUSMWellerPulsoni, ClaudiaItalyStellar halos of massive galaxies: morphology, kinematics, and cosmological originLMUMPEGerhardBurkertArnaboldiPunanova, AnnaRussiaChemistry and Kinematics in Low-Mass Star-Forming RegionsLMUMPECaselliPonPinedaRagagnin, AntonioItalyFrom the mass-concentration relation of haloes to GPUs and into the web: a guide on fully utilizing super computers for the largest, cosmological hydrodynamic simulationsLMUUSMDolagBaderHammerRenneby, MalinSwedenWeak gravitational lensing as a probe of large-scale structure and galaxy formationLMUExc. Cluster UniverseBurkertHilbertKomatsuHenriquezSchulz, ChristineGermanyThe distribution of star formation rates during the assembly of NGC 1399 as deduced from its globular clustersLMUESOBurkertHilkerSokolov, VlasUkraineEarly Stages of Massive Star FormationLMUMPECaselliKissler-PatigTutis, TeaCroatiaFinding halofit for cluster clusteringLMUUSMWellerHoyleSeitzWagstaff, GrahamUKConvective and Atmospheric Boundaries of Asymptotic Giant Branch StarsLMUMPAWeissMuellerGilfanovWiseman, PhilipUKGamma-ray burst host galaxies in absorptionTUMMPEGreinerSchadyPonti
