All posters will be up all week and can be visited at all times.
The maximum space for poster presentations is A0 portrait format (width: 841 mm, height: 1189 mm). Poster spaces will be available for accepted abstracts only.
In addition, we offer a 1 min poster flash talk for each poster.
For this, please prepare 1 (at most 2) slide(s) as pptx or pdf and name it according to the page in the book of abstracts.
A detailed program and the book of abstract can be downloaded on the right!
A detailed program and the book of abstract can be downloaded below!
| MONDAY, 17 August 2026 / Time: 11:55 – 12:25 | |||
| Poster Flash Presentations: PI | |||
| Identifier | Last name | First name | Title |
| P.2 | Alt | Henrik Silas | Digital Sideband Separation Using Tone-Injection calibration scheme |
| P.3 | Asvany | Oskar | Hyperfine-resolved rovibrational and rotational spectroscopy of OH⁺ |
| P.4 | Bigiel | Frank | mm-spectroscopy across nearby galaxies – dense gas fraction and star formation efficiencies from cloud to galaxy scales |
| P.5 | Böing | Julian | Towards Understanding Leak-Out Spectroscopy (LOS) in Cryogenic Ion Traps |
| P.6 | Bosmann | Jonas | Jet-Cooled Millimeter-Wave Spectroscopy of Circumstellar Refractory Species |
| P.15 | Fuchs | Guido W. | High-Resolution Mid-IR Observations of SiO, H₂O and NH₃ around the Massive Star VY CMa and Others Using EXES/SOFIA and TEXES/IRTF |
| P.16 | García | Pablo | CF⁺ as a C⁺ Proxy in Low Metallicity Environments: Observations Toward the N159-W Region in the LMC |
| P.20 | Grutzeck | Gerrit | The next-generation U-Board – A heterogeneous, closely coupled architecture for radio astronomy |
| P.33 | Misra | Prachi | Rotational Spectroscopy of C₃H₄O₂ using Updated CP-FTMW Spectrometer |
| P.35 | Müller | Holger | Rotational Spectroscopy of Vibrationally Excited States as a Tool for Astrophysics: Investigations of ¹³CH₃CN and CH₃¹³CN up to v₈ = 2 and a Search for v₈ = 2 Transitions Toward Sagittarius B2(N) |
| P.40 | Owen | Morgan | WCCC versus HC chemistry through the lens of deuterium fractionation |
| P.43 | Plaar | Eline | High resolution rovibrational and rotational spectroscopy of HC₃N⁺ |
| P.46 | Röllig | Markus | Updated H₂ ro-vibrational and UV line & continuum physics in the KOSMA-τ PDR code |
| P.49 | Salomon | Thomas | High-resolution laboratory study of the ν2/ν4 bending motion of CH₃⁺ and assignment of its astronomically observed lines |
| P.51 | Schlemmer | Stephan | On the selection of nuclear spin species in an ion trap |
| P.52 | Schneider | Lea | Combining a cryogenic ion trap with a 2 THz multiplier chain source: revisiting the J=1 |
| P.56 | Thorwirth | Sven | Pure-rotational spectroscopy of cis- and trans-1,3-dichloropropene |
| P.57 | Thorwirth | Sven | Laboratory spectroscopic studies of COMs in vibrationally excited states |
| P.63 | Wang | Chenxu | The Rotational Spectrum of trans-2,3-Epoxybutane: A Combined Chirped-Pulse Fourier Transform and Absorption Microwave Study |
| P.47 | Roth | Tim Otto | Solar aesthetics – how other star forms might impact perceptual systems |
| TUESDAY, 18 August 2026 / Time: 12:00 – 12:30 | |||
| Poster Flash Presentations: PII | |||
| Identifier | Last name | First name | Title |
| P.7 | Canal i Saguer | Mar | Systematic study of HII regions in the Magellanic Clouds with eROSITA |
| P.9 | Cheriyan | Amal George | Polarization study toward the massive protostellar jet system HH 80-81 |
| P.12 | Dannhauer | Simon | Disentangling the accretion flow in S106 |
| P.17 | Gebauer Werner | Lucia | Exploring Supernova Remnant Properties Using Pulsars |
| P.19 | Großekathöfer | Lena | A polychromatic analysis of the dissolving stellar association IRS 6 in the center of our Galaxy |
| P.26 | Keilmann | Eduard | An Apparent [C II]-Deficit in S144/RCW79 Caused by Self-Absorption |
| P.27 | Lieb | Emma | Survey of 5 Dust-Producing Wolf-Rayet Binaries Reveals Grain Size and Temperature Variation Across Stellar Environments |
| P.29 | Mehta | Parit | [CII] self-absorption in M17: a large-scale view from SOFIA FEEDBACK |
| P.37 | Nandre | Tanish | The Carbon Budget in the Milky Way |
| P.44 | Rathjen | Tim-Eric | Radiation and cosmic rays shaping the multiphase interstellar medium |
| P.45 | Reyes | Simon | Connecting accretion and ejection rates for massive protostars using JWST/MIRI |
| P.48 | Saha | Himadri | Performance modelling of Integrated Filterbank Spectrometers towards sub-millimetre Line Intensity Mapping surveys |
| P.50 | Sasaki | Kotora | The Role of Hierarchy in Galactic Molecular Clouds: Observational Tests of the Global Hierarchical Collapse |
| P.58 | Ushirogi | Taishi | Mass Budgets of Episodic Protostellar Outflows in an Isolated Turbulent Core |
| P.59 | Vandersnickt | Jelle | Asteroseismic detection of an internal magnetic field inside an evolved massive main sequence star |
| P.61 | Vider | Sebastian | Confronting Observations with Simulations – Blister-Type HII Regions |
| P.62 | Vrancken | Jasmine | Probing Massive‑Star Formation with Intrinsic Multiplicity Constraints from TESS Eclipsing Binaries |
| P.64 | Weng | Jixiang | The Keplerian disk, envelope, and streamers surrounding an early O-type protostar in the Sagittarius C cloud of the Central Molecular Zone |
| P.66 | Yamada | Rin | Formation of the Rich Network of Filaments Driven by an Expanding HI Bubble in the Perseus Molecular Cloud |
| P.67 | Yap | Mervin Zhi Rong | Multidimensional CWENO finite volume method with constrained transport for MHD simulations of shockwaves in the ISM |
| WEDNESDAY, 19 August 2026 / Time: 12:00 – 12:30 | |||
| Poster Flash Presentations: PIII | |||
| Identifier | Last name | First name | Title |
| P.8 | Cheema | Anahat | The frst C-band rotation measure grid through the Galactic plane: Expanding the population of polarized radio sources |
| P.10 | Clarke | Jonathan | Line intensity mapping: Modelling star-forming galaxy emission at the epoch of reionisation for FYST using catalogue data |
| P.21 | Guerrero | Andrea | CIB modeling to constrain the faint-end slope of galaxy number counts |
| P.22 | Hu | Ying-Chi | First look of 18cm OH masers and Zeeman splitting of high-mass star forming regions in MMGPS |
| P.24 | Karoumpis | Christos | Line intensity mapping with the ALMA interferometer |
| P.25 | Kast | Helene | Comparison of X-ray and optical AGN identification methods in local galaxies |
| P.30 | Mertens | Marc | Mini-CHAI, a First Light Heterodyne Instrument for the CCAT Observatory |
| P.31 | Miklósi | Rebeka | Superconducting Intermediate Frequency Circuitry for the CCAT Heterodyne Array Instrument |
| P.34 | Mohammad Bokhari | Nurul Husna | Investigating low and high mass protostellar outflows with ALMA observations |
| P.38 | Okada | Yoko | Operation of Cerro Chajnantor Atacama Telescope (CCAT) Observatory |
| P.41 | Patra | Sudeshna | Exploring the extragalactic dense gas tracers in the Milky Way with APEX |
| P.42 | Peregrina García | Damián | Properties of NbTiN-Nb-Al/AlOx/Nb tunnel junctions in dependence of Nb interlayer thickness |
| P.53 | Schneider | Nicola | Synergy between GEco and FEEDBACK |
| P.54 | Syaifoel | Kian | Probing the Lower Limit of Two-Level System Noise in Parallel-Plate Capacitor Kinetic Inductance Detectors using Crystalline-Silicon Dielectric |
| P.55 | Tanchon | Ella | Decoding Cluster Formation and Evolution through Forward Modelling of PHANGS Star Clusters |
| P.60 | Verbena | Juan Luis | grex: A Python Pipeline for SOFIA/GREAT Spectral Data Reduction |
| P.65 | Woolvett O’Ryan | Vicente José | The APEX Microwave Kinetic Inductance Detector camera (A-MKID): from commissioning to early observations |
| WEDNESDAY, 19 August 2026 / Time: 15:15 – 15:30 | |||
| Poster Flash Presentations: PIV | |||
| Identifier | Last name | First name | Title |
| P.1 | Aberfelds | Artis | Is the CH₃OH maser transition at 6.7 GHz a tracer of the inner outflow cavities near YSOs? |
| P.11 | Coors | Alice | Tracing shock-driven shaping of molecular clouds as a trigger for star formation |
| P.13 | Dincer | Furkan | The role of massive stars in the cluster expansion phase |
| P.14 | Elbakyan | Vardan | Accretion Bursts in High-Mass Stars: Mechanisms and Observational Implications |
| P.18 | Gerasimov | Ivan | Tracing star cluster evolution through PAH morphology |
| P.23 | Kao | Jo-Shui | Testing the polarization-intensity polarization–intensity gradient method in molecular clouds and collapsing dense cores simulation |
| P.28 | Littek | Simon | Synthetic Emission Line Maps as a Benchmark for H II Region Metallicity Diagnostics |
| P.33 | Mills | Jessica | Birth Radii Analysis of Milky Way Disk Stars According to APOGEE DR17 and the NIHAO-UHD Simulation Suite |
| P.36 | Nagar | Chinmaya | A Close Look at the Multiplicity of Young Massive Stars in Galactic Embedded Clusters |
| P.39 | Ortaköse | Nuray | From Flows to Fragments: Tracking Core Evolution in Star-Forming Environments |








