Posters
Dear GCF 2021 poster presenters,
please email your poster (main document & thumbnail document) to us at GCF2021@eso.org no later than June 8 at 1 pm UTC (= hard deadline) following the instructions for the format.
Posters will be presented in dedicated poster sessions and also displayed in the GCF2021.Town, which will be activated on Gather ~ 1 week before the conference.
Gather.Town sessions will take place each day 30 minutes prior to the official start of the conference as well as at the end of each day.
Participants can join the GCF2021.Town on Gather in a 2D world with 8-bit graphics, walking around the virtual conference venue by moving their avatar with their keyboard’s arrow keys. Please note that an avatar marked “anonymous” or carrying an invented name such as e.g. “007” does not get interaction, since participants are looking to interact with other participants. We thus encourage you to use your full name.
When creating your poster, please follow these guidelines.
We strongly encourage you to also post your poster on our conference GCF 2021 slack channel which will open ~ 1 week before the conference.
Details on how to access both channels (Gather.Town and Slack) as well as respective links will follow soon.
Nr. |
Last name |
First name |
Affiliation |
Title |
| A1 | Afanasiev | Anton | Universite de Paris | Evolution of the Mass-Size relation in CARLA clusters |
| A2 | Amos | Nicholas | Lancaster University | Resolved spectroscopy of cluster galaxies at z>1 |
| A3 | Ando | Makoto | The University of Tokyo | A systematic search for proto-cluster cores at a transition epoch of star formation activity |
| A4 | Biviano | Andrea | INAF-OATs | GOGREEN: The dynamics of clusters at z>1 |
| A5 | Boehm | Asmus | Institute for Astrophysics | Kinematics of proto-cluster disk galaxies at z=1.5 |
| A6 | Botteon | Andrea | Leiden Observatory | The initial stages of cluster mergers observed in radio and X-rays |
| A7 (Cancelled) | ||||
| A8 | Cairns | Joseph | Imperial College London | Star Formation in SpARCS J0330: Bridging the Gap Between Protoclusters and Clusters |
| A9 | Caretta | César | Departamento de Astronomía, Universidad de Guanajuato | Nucleation zones in superclusters and the future largest galaxy clusters |
| A10 (Cancelled) | ||||
| A11 | Chadayammuri | Urmila | Smithsonian Astrophysical Observatory | Weighing merging galaxy clusters with idealised simulations |
| A12 | Chaturvedi | Avinash | European Southern Observatory | Exploring the mass assembly of the Fornax Galaxy Cluster |
| A13 | Cho | Hyejeon | Yonsei University | First Weak-lensing Analysis of the Double Radio Relic Merging Cluster Abell 1240 |
| A14 | Craig | Jessica | Keele University | Evolution in Clusters and Groups Behind the Magellanic Clouds |
| A15 | Daikuhara | Kazuki | Tohoku University | Environmental dependence in low-mass star-forming galaxies down to 10^8 Msun at z=2.2 |
| A16 | Díaz-Sánchez | Anastasio | Universidad Politécnica de Cartagena | Searching Massive Galaxy Clusters at z~1 with WISE+VISTA+SDSS Catalogues |
| A17 | Dicker | Simon | University of Pennsylvania | High resolution observations of high redshift clusters using the SZE effect and MUSTANG2 |
| B1 | Dole | Herve | Universite Paris-Saclay | Planck-selected z~2 protocluster properties: paving the halo-mass vs redshift vs SFR cube |
| B2 (Cancelled) | ||||
| B3 | Floyd | Benjamin | University of Missouri--Kansas City | Dependence of AGN Activity on Halo Mass and Redshift in the SPT Cluster Surveys |
| B4 | Fukushima | Keita | Osaka University | "Star Formation and Chemical Enrichment in Protoclusters " |
| B5 | Harshan | Anishya | University of New South Wales | The Beginning of the End for Massive Galaxies at z~2 and Why Environment Matters |
| B6 | Hernández | Daniel | Universitäts-Sternwarte München | Clash of Titans: a MUSE dynamical study of the cluster merger SPT-CLJ0307-6225 |
| B7 | Holguin Luna | Priscilla | New Mexico State University | Punishing Environments at low-z: Constraining gaseous conditions in the modern Universe |
| B8 | Hung | Denise | University of Hawai'i | Systematic Optical/NIR Discovery of Large Scale Structure at Intermediate and High Redshift |
| B9 (Cancelled) | ||||
| B10 | Ito | Kei | Sokendai | The rest-frame UV luminosity function of protocluster galaxies at z~4 revealed by HSC-SSP |
| B11 (Cancelled) | ||||
| B12 | Kelkar | Kshitija | Universidad de Valparaíso | Passive spirals and shock-influenced star formation in merging cluster A3376 |
| B13 | Kim | HyeongHan | Yonsei University | Discovery of a Radio Relic in the Merging Cluster SPT-CL J2023-5535 from the ASKAP-EMU Pilot survey |
| B14 | Kim | Jinhyub | Yonsei University | An improved analysis of the galaxy cluster ACT-CL J0102-4915 with new wide-field HST imaging data |
| B15 | Kneissl | Ruediger | ALMA/ ESO | Resolving galaxies in cosmic infrared background peaks of the Planck survey |
| B16 | Ko | Eunhee | Seoul National University | Testing Web Feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field |
| B17 | Laza Ramos | Andrés | Universidad de La Laguna | SCUBA-2 observations of the Spiderweb protocluster at z=2.2 |
| B18 | Lemaux | Brian | University of California, Davis | An Optical/NIR Exploration of Proto-structure Environments at High-Redshift with Keck and VLT |
| C1 | Lorenzoni | Vanessa | Universidade Federal de Santa Maria | Stellar populations and ionised gas in central spheroidal galaxies |
| C2 | Lourenco | Ana Carolina | Universidad de Valparaiso | The environment of jellyfish galaxies in the local universe |
| C3 | Mahler | Guillaume | Centre of Astrophysique | Mass Ratio Evolution in Clusters Between Halos and Sub-halos |
| C4 | Mao | Zhiying | Tohoku University | Revealing galaxy quenching's dependence on stellar mass and environment in galaxy clusters |
| C5 | McConachie | Ian | University of California Riverside | A Protocluster at z=3.37 Around a Massive Quiescent Galaxy with an Elevated Quenched Fraction |
| C6 (Cancelled) | ||||
| C7 | Mernier | Francois | ESA/ ESTEC | Chemical enrichment in clusters (and forming clusters): the curious case of NGC1404 |
| C8 | Monteiro-Oliveira | Rogério | State University of Santa Cruz | Peculiar features arising from merging galaxy clusters: the case of A1644 and A2034 |
| C9 | Moura | Micheli | Universidade Tecnológica Federal do Paraná | The role of gas and dark matter in the dissociative collision of Abell 2034 |
| C10 | Nakano | Satoya | Nagoya University | Environmental Quenching seen in CO Emitting Galaxies in a Massive Cluster SPT-CL J0615－5746 |
| C11 | Nonino | Mario | INAF-OATs | GCAV: Galaxy Clusters At Vircam |
| C12 | Olamaie | Malak | York St. John University | Free-form modelling of the physical properties of proto/clusters-A Bayesian and data driven approach |
| C13 | Olivares | Valeria | University of Kentucky | Unveiling the origin of the cold gas in Brightest Group Galaxies with MUSE |
| C14 | Olivares | Valeria | University of Kentucky | AGN feedback in the Planck selected Clusters: a detailed study of X-ray cavities |
| C15 | Orlowski-Scherer | Jack | University of Pennsylvania | An ACT measurement of the MaDCoWS mass-richness scaling relation |
| C16 | Panko | Elena | I.I. Odessa National University | Markers of Evolution in Rich Galaxy clusters |
| C17 | Pascut | Aurelia | Stefan cel Mare University | Chandra observations of the AS0295 cluster |
| C18 | Qiu | Yu | Kavli Institute for Astronomy and Astrophysics | AGN Feedback: Keeping Clusters Cores in Check for Gigayears |
| D1 | Ricarte | Angelo | Harvard-Smithsonian Center for Astrophysics | Linking Ram Pressure and AGN in the RomulusC Simulation |
| D2 | Shen | Lu | University of Science and Technology of China | Implications of the Environments of Radio-detected AGN in a Complex Proto-structure at z∼3.3 |
| D3 | Souza | Gilvan | Universidade Cidade de São Paulo | The relation between the central galaxy properties and the dynamical state of the cluster |
| D4 | Štofanová | Lýdia | Leiden Observatory | The photoionization by galaxy cluster photons and its impact on the plasma in the cluster vicinity. |
| D5 | Stott | John | Lancaster University | Galaxy overdensities around UV luminous quasars at z = 1 - 2 |
| D6 | Takeda | Yoshihiro | University of Tokyo | VoidNet: Void Galaxy Selection from g-dropout Catalog by Deep Learning |
| D7 (Cancelled) | ||||
| D8 | Tümer | Ayşegül | The University of Utah | NuSTAR and XMM-Newton view of the interaction between A3395 and A3395/A3391 intercluster filament |
| D9 | van Kampen | Eelco | ESO | Building samples of distant cluster galaxies with ALMA |
| D10 | Vigneron | Benjamin | University of Montreal | Analysis of Newly Obtained High Spectral Resolution Data of NGC 1275 |
| D11 (Cancelled) | ||||
| D12 | Zhang | Xiaoyuan | Leiden Observatory/ SRON | Deep Chandra observations of double relic cluster ZwCl 2341+000 |
| D13 | Zhou | Luwenjia | Nanjing University | GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5 |
| D14 | Zhu | Zhenlin | SRON | A shock near the virial radius of the Perseus Cluster |
| D15 | Zuñiga | Johan Manuel | Universidad de Guanajuato | Measuring the dynamical status of the evolving galaxy clusters: |
GCF 2021 channels on
- Youtube: Galaxy Cluster Formation Conference 2021
- Gather.Town
- Slack
- Zenodo
This workshop is supported by ESO and the Smithsonian Astrophysical Observatory.
Keywords: merging clusters | high-z clusters | proto-clusters | detection, classification & comparison | ICM physics | AGN feedback | star formation | galaxy evolution | future facilities
Workshop email: GCF2021@eso.org