The Spectral Energy Distribution of high redshift galaxies:
lessons learned and open questions.
Sexten Center for Astrophysics
January 26‐30 2015
Registered Participants
| Oral Presentations | ||
| Ricardo | Amorin | Physical properties and metallicity of strong emission line galaxies out to z~4 from VUDS and VANDELS |
| Nathan | Bourne | Understanding relationships between star formation rate, stellar mass and obscuration at high redshift with the SCUBA-2 Cosmology Legacy Survey |
| Rebecca | Bowler | Rapid evolution in the bright end of the galaxy luminosity function between z = 5, 6 and 7 |
| Gabriel | Brammer | 3D-HST: A slitless spectroscopic survey of distant galaxies with HST grisms |
| Victoria | Bruce | Probing AGN through host galaxy morphologies |
| Fernando | Buitrago | The dichotomy for the mass-size relation for massive galaxies up to z = 4.5 in the HUGS survey |
| Nico | Cappelluti | Early black holes in EBL fluctuations |
| Marco | Castellano | Constraints on the nebular line emission of reionization sources |
| Emanuele | Daddi | A highly deconfused mid-far-IR to submm catalog in GOODS-N: first scientific results |
| James | Dunlop | The Luminosity Function at z=9 |
| David | Elbaz | Targeted discussion |
| Henry | Ferguson | CANDELS from the UV to the far-IR: How to make optimal use of the data |
| Adriano | Fontana | Massive galaxies at high redshift |
| Audrey | Galametz | Photometric redshifts & co for the Euclid Mission |
| Mauro | Giavalisco | The star-formation activity and quenching of massive, compact galaxies and galaxies with a Dominant Central Object |
| Andrea | Grazian | The UltraViolet side of star-forming galaxies with LBC/LBT: the Lyman continuum escape fraction at z~3 |
| LUCIA | GUAITA | Lyman Continuum Signal from z~3 star-forming galaxies with available multi-wavelength coverage. |
| Allison | Kirkpatrick | What Lies Beneath: Probing Dust Obscured Star Formation and AGN Growth |
| Peter | Kurczynski | Sizing Up Dwarf Galaxies at z > 1: UV Colors, Stellar Masses and Star Formation Rates |
| Bomee | Lee | CANDELS: Improved Spectral Energy distribution fitting of galaxies |
| Daizhong | Liu | IR imaging de-confusion |
| Emiliano | Merlin | TPHOT: Advanced Techniques of Precision Photometry for Present and Future Multiwavelength Surveys |
| Alice | Mortlock | Exploring the evolution of the stellar mass function in the redshift range 1 |
| Camilla | Pacifici | On the importance of using appropriate spectral models to derive physical properties of galaxies |
| Naveen | Reddy | Measurements of the Dust Attenuation Curve at z~1.4-2.6 from the MOSDEF Survey |
| Jose Miguel | Rodriguez Espinosa | Episodic star formation in two LAEs at z=5.1 |
| Kate | Rowlands | Properties of dusty massive galaxies at low and high redshifts |
| Brett | Salmon | The Star-Formation and Rate and Stellar Mass Relation of Galaxies at High Redshift in CANDELS |
| Paola | Santini | The evolution of the dust and gas content in galaxies |
| Daniel | Schaerer | Properties of the Lyman Break Galaxy population at high-z and new constraints from IR/mm observations |
| Corentin | Schreiber | The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day |
| Xinwen | Shu | Distant Herschel 500um Sources Revealed with Color-deconfusion |
| Panos | Sklias | Constraining Star Formation Histories of IR-luminous high-z Galaxies with Herschel |
| Mimi | Song | The Evolution of Galaxy Stellar Mass Functions at z=4-7 |
| Romanin | Thomas | Using galaxy ages to constrain the epoch of galaxy formation |
| Elena | Tundo | The GEMMA project |
| Eros | Vanzella | – |
| Fabian | Walter | Molecular Deep Fields |
| Tao | WANG | A census of massive galaxy population at z~4 |
| Other Participants | ||
| Rosa | Calvi | |
| Koryo | Okumura | |
| Stefano | Pilo | |