| Monday, 27.07. | MORNING 10:00 10:30 10:45 AFTERNOON 14:00 15:30 | Earliest galaxies COFFEE/TEA Introductions Presentations (<30min/talk) Rychard Bouwens "The evolution of the cosmic ionising emissivity at z>6 and comparisons to new determinations of the galaxy UV luminosity density at z>6” Naveen Reddy "Dust Attenuation Curves and their Implications for High-Redshift Galaxies" Kirsten Knudsen “Submillimeter galaxies in the early universe” Earliest galaxies Discussion leader: Rychard Bouwens discussion topic ideas (1) High Ionization Fluxes from z>4 Galaxies: Do we understand the stellar populationsand hence SFRs of the earliest galaxies (2) Contribution of the Faint End of the LF to the SFR Density: What are some Challenges in Establishing the Faint End of the LF from the Hubble Frontier Fields Program (3) Intrinsically Luminous Galaxies at Very High Redshift: What are they and is their nature easily understood within standard galaxy formation models? COFFEE/TEA |
| Tuesday, 28.07. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 | Structure of galaxies COFFEE/TEA Presentations (<30min/talk) Michele Cappellari "Mass and dynamics of galaxies out to their stellar halos" Eric Emsellem "From high to low luminosity early-type galaxies" Lucio Mayer "The physics of disk galaxy formation at high and low redshift; instabilities, feedback and stellar mass assembly histories" David Fiacconi "The development of galaxy morphology: a high-redshift perspective" Structure of galaxies Discussion leader: Lucio Mayer discussion topic ideas (1) What is different and what is not different in the mode of (disk) galaxy formation at high vs. low redshift,and what does that imply about star formation properties? (2) Which component traces best the early stellar assembly phase in disk galaxies? The bulge or the thick disk? What do they tell us in general about conditions of galaxy formation at hi-z? (3a) What is the dominant mechanism for the formation of bulges of spirals? (3b)How can we exploit bulge properties to constrain the effect of feedback(s) and the amount of star formation at high vs. low z? (4) Is there any evidence that AGN feedback plays an important role in the formation of spiral galaxies (eg bulge properties, SF history)? Or is it a second-order ingredient? (5) Clumpy galaxies at high-z; where are they today and which property of low-z galaxies carries the imprint of a past clumpy phase? COFFEE/TEA |
| Wednesday, 29.07. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 | ISM, part I COFFEE/TEA Presentations (<30min/talk) Alexia Lewis "Challenges of studying the ISM on sub-kpc scales" Mei-Ling Huang "The variation in molecular gas depletion time among nearby galaxies" Kyle Penner "The assumptions we make when we study dust through attenuation" slides ISM, part I Discussion leader:Naveen Reddy discussion topic ideas (1) What do we learn by tracking the concomitant evolution of dust mass and stellar metallicity? (2) What is the fraction of metals in the gas vs. locked into dust grains? COFFEE/TEA |
| Thursday, 30.07. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 | Environments of forming massive galaxies COFFEE/TEA Presentations (<30min/talk) Caitlin Casey “Rare starbursts as protocluster probes” William Cowley "What halo masses dominate the cosmic infrared background?" Paola Popesso "The role of massive halos in the cosmic star formation history" Environments of forming massive galaxies Discussion leader:Caitlin Casey discussion topic ideas TBA COFFEE/TEA |
| Monday, 03.08. | MORNING 10:00 10:30 10:45 AFTERNOON 14:00 15:30 | Lyman alpha emitters COFFEE/TEA Introductions Presentations (<30min/talk) Lennox Cowie "How are Lyman alpha emitters drawn from the general galaxy population?" Isak Wold "Lyman alpha emitters at z~1" Yuichi Matsuda "Lyman alpha blobs" Nick Gnedin "Why we should not study Lyman alpha emitters" slides Lyman alpha emitters Discussion leader: Lennox Cowie discussion topic ideas (1) How do Lyman alpha blobs relate to submm galaxies? (2) What is the ionizing radiation from Lyman alpha emitters? (3) How much can you tell about winds and infall from the Lyman alpha emission? COFFEE/TEA |
| Tuesday, 04.08. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 18:00 | Properties of massive galaxies COFFEE/TEA Presentations (<30min/talk) Laura Morselli “Bulges and disks in the SFR-M* plane at z<0.1” Julie Wardlow "Lensed star formation in dusty galaxies: results from Herschel wide field surveys" slides Maurillio Pannella "The Main Sequence of star-forming galaxies as seen by the deepest Herschel, JVLA and ALMA data" slides galaxies Discussion leaders Julie Wardlow, Stefano Berta and Kyle Penner discussion topic ideas (1) Bursty galaxies and main sequence galaxies: two modes of star formation? (2) Solutions to the "dust budget crisis" in high-redshift SMGs and low-redshift ellipticals Stefano Berta: Dust Gas COFFEE/TEA BBQ |
| Wednesday, 05.08. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 | Star formation history, part I COFFEE/TEA Presentations (<30min/talk) Madusha Gunawardhana "The star formation rate history of the local universe" Jacinta Delhaize "Examining the infrared-radio correlation and the cosmic star formation history with sensitive radio continuum surveys" Bruno Henriques "AGN and environmental quenching and their impact on the star formation" Cedric Lacey "Cosmic star formation history: predictions from semi-analytical models" slides Star formation history, part I Discussion leaders: Bruno Henriques, Yannick Bahe, and Paola Popesso discussion topic ideas Star formation quenching in dense environments COFFEE/TEA |
| Thursday, 06.08. | MORNING 10:00 10:30 10:55 11:20 11:45 12:10 | MaNGA/IFU COFFEE/TEA all speakers are kindly requested to **keep to their allotted time slots** so that we do get to the discussion in time. Richard D'Souza "The stellar haloes of galaxies through MaNGA" Amy Jones Ionized gas outside the disks of spirals as seen by MaNGA Miranda Jarvis WIFIS: The Wide Integral Field Infrared Spectrograph and the Image Simulator Eva Wuyts Galaxy evolution studies with KMOS Discussion Ric Davies and Guinevere Kauffmann What analysis techniques are needed for meaningful comparisons of the stellar populations, structure, kinematics and environments of galaxies at different redshifts |
| Monday, 10.08. | MORNING 10:00 10:30 10:45 AFTERNOON 14:00 15:30 | ISM, part II COFFEE/TEA Introductions Presentations (<30min/talk) Thorsten Naab "Feedback and wind driving in the ISM" Philipp Girichidis The Impact of Cosmic Rays in the ISM Structure and Outflows Thomas Peters "Impact of supernova and cosmic ray driving on the Galactic Halo in soft X-Rays" ISM, part II Discussion leader: Thorsten Naab discussion topic ideas What are the relevant physical processes and spatial scales setting the stage for star formation and galactic winds? How important is H2 formation? How important are non-thermal components: magnetic field, cosmic rays? How reliable are the star formation and feedback sub-resolution models used in galaxy formation simulations? What is the role of ‘convergence’ in galaxy formation simulations? COFFEE/TEA |
| Tuesday, 11.08. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 | Gas in and around galaxies COFFEE/TEA Presentations (<30min/talk) Ali Rahmati "Simulating the cosmic distribution of gas and its connection with galaxies" Yannick Bahe "The distribution of atomic hydrogen in the EAGLE simulations at z=0" Guinevere Kauffmann "Linking the CGM to the outskirts of galactic disks" Amy Barger “Is star formation in the host galaxies of X-ray luminous AGN suppressed?” slides COFFEE/TEA |
| Wednesday, 12.08. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 18:00 | Star formation history, part II COFFEE/TEA Presentations (<30min/talk) Stefano Berta "Gas and dust content of (z>0.5) galaxies as seen by Herschel/ALMA” slides Carlotta Gruppioni "Herschel monsters and AGN: their role in the cosmic star formation history and comparison with SAMs" Alvio Renzini "Breaking down the cosmic star formation history" Star formation history, part II Discussion leaders: Carlotta Gruppioni & Alvio Renzini discussion topic ideas "Quenching, AGN & the Like! COFFEE/TEA "BBQ" |
| Friday, 14.08. | 8:30 | excursion to the Wendelstein observatory Meeting Point: Munich Main Station, Main Entrance guided tour: 12:45-14:00 |
| Monday, 17.08. | MORNING 10:00 10:30 10:45 AFTERNOON 14:00 15:30 | Kinematics and ISM COFFEE/TEA Introductions Presentations (<30min/talk) Yanmei Chen "MaNGA galaxies with decoupled kinematics between gas and stars” slides Alexei Kritsuk "Turbulent cascades and star formation in galactic disks" Guang-Xing Li "Gravitational acceleration in molecular clouds" Kinematics and ISM Discussion leader: Nick Gnedin discussion topic ideas TBA COFFEE/TEA |
| Tuesday, 18.08. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 | Galaxies and AGN COFFEE/TEA Presentations (<30min/talk) Alice Concas "A Galaxy History, as told by its Optical Spectrum" Li-Yen Hsu "Overlapping the UV and FIR stra-forming Galaxy Populations with a SCUBA-2 Lensing Cluster Survey" David Rosario "AGN-galaxy co-evolution with a Herschel focus" Galaxies and AGN Discussion leader: David Rosario discussion topic ideas Building on the legacy of multi-wavelength surveys to unravel the crucial drivers of the AGN-galaxy connection COFFEE/TEA |
| Wednesday, 19.08. | MORNING 10:00 10:30 AFTERNOON 14:00 15:30 | Population of massive galaxies COFFEE/TEA Presentations (<30min/talk) Karina Caputi "Are there massive galaxies at z>6?" Harry Ferguson “Massive Galaxy Evolution from CANDELS” Benjamin Magnelli "Evolution of the physical properties of galaxies in the SFR-M* plane: evidences for secular and starburst modes of star formation?" Population of massive galaxies Discussion leaders: Karina Caputi, Maurillio Pannella, and Harry Ferguson discussion topic ideas (1) UV dust attenuation and sample selection biases (2) Massive galaxies at high redshifts (3) What is the connection between dusty starbursts, quenched galaxies, and blue or red nuggets among massive galaxies at z=2-5? WINE & CHEESE |
| Thursday, 20.08. | MORNING 10:00 10:30 | COFFEE/TEA Presentations (<30min/talk) Allison Mann “Explaining the discrepancy in galaxy merger rate measurements at z=0-3” and “Are quiescent galaxies really devoid of star formation? The mid-infrared, far-infrared, and radio properties of massive quiescent galaxies at z=0.1-3" Rychard Bouwens “Extreme Galaxies: On the Brightest, Most Massive Galaxies at z>=6.5 from CANDELS and Cautious Use of Gravitational Lensing to Study Ultra-Faint Galaxies from the Hubble Frontier Fields Program” Nick Gnedin "Reionization" |