Sesto 2015 – Participants


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 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