CAPAK |
Peter |
Caltech |
USA |
Talk |
Next Generation Galaxy Statistics |
SANDERS |
David |
University of Hawaii, Institute for Astronomy |
USA |
Talk |
TBD |
NAGAO |
Tohru |
Ehime Univ. |
JAPAN |
|
|
UEDA |
Yoshihiro |
Department of Astronomy, Kyoto University |
JAPAN |
|
|
STOCKMANN |
Mikkel |
Dark Cosmology Centre, Niels Bohr Institute |
DENMARK |
Talk |
14 Spectroscopically Confirmed Massive Quenched Galaxies at z>2 |
GÓMEZ-GUIJARRO |
Carlos |
Dark Cosmology Centre |
DENMARK |
Talk |
Submillimeter to quiescent galaxy evolution from HST/ALMA |
FAISST |
Andreas |
Caltech/IPAC |
USA |
Talk |
Galaxies at z = 6: Hot and turbulent? |
MIYAJI |
Takamitsu |
IA-UNAM Ensenada |
MEXICO |
Poster |
CSTACK:Stacking Analysis of Chandra Images on the Web |
MURAYAMA |
Takashi |
Tohoku University |
JAPAN |
|
|
HEMMATI |
Shoubaneh |
Caltech/IPAC |
UNITED STATES |
Talk |
Neural Network Self Organizing Maps to revolutionize the measurement of Physical Properties of Galaxies |
SCUDDER |
Jillian |
University of Sussex |
USA |
Talk |
Understanding galaxies in the confused FIR sky |
RIECHERS |
Dominik |
Cornell University |
USA |
Talk |
The VLA CO Luminosity Density at High Redshift (COLDz) Survey |
HIRANO |
Kou |
Tohoku Univ. |
JAPAN |
Poster |
Survey for low-z strong emission line galaxies by COSMOS 20 |
NISHIDUKA |
Takuma |
Master' course of astronomy , Graduate school of Science , Tohoku University |
JAPAN |
Poster |
Clustering property and environment of extremely emission-line galaxy |
SCOVILLE |
Nick |
Caltech |
USA |
Talk |
Evolution of ISM from ALMA Observations |
MOROKUMA |
Kana |
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency |
JAPAN |
|
|
KASHINO |
Daichi |
ETH Zurich |
SWITZERLAND |
Talk |
Clustering and host dark halo properties of star-forming galaxies at z~1.6 |
DELHAIZE |
Jacinta |
University of Zagreb |
CROATIA |
Talk |
Update: Studies of the infrared-radio correlation behaviour with redshift using the VLA-COSMOS 3GHz Large Project |
SCHULZE |
Andreas |
NAOJ |
JAPAN |
Talk |
The active black hole mass function at z~4 from COSMOS and SDSS |
CASEY |
Caitlin |
UT Austin |
USA |
Talk |
TBD |
LANG |
Philipp |
Max-Planck-Institute for Astronomy |
GERMANY |
Talk |
Uncovering stellar mass distributions of distant SMGs at z~2 |
BARNES |
Joshua |
Institute for Astronomy, University of Hawaii |
USA |
|
|
CHANG |
Yu-Yen |
ASIAA |
TAIWAN |
Talk |
Obscured AGNs by Infrared Selection |
MC CRACKEN |
Henry Joy |
Institut d'Astrophysique de Paris |
FRANCE |
Talk |
Latest UltraVISTA / COSMOS news I guess |
LIU |
Daizhong |
Max-Planck-Institut für Astronomie |
GERMANY |
Talk |
Super-deblended dust emission in galaxies and the cosmic star formation rate density evolution |
LESLIE |
Sarah |
Max Planck Institute for Astronomy |
GERMANY |
Talk |
The Star Formation History of Mass-selected Galaxies with VLA-COSMOS 3GHz Large Project. |
STAGUHN |
Johannes |
JHU & NASA/GSFC |
USA |
Talk |
The Origins Space Telescope (OST) |
BARISIC |
Ivana |
Max-Planck Institut für Astronomie |
GERMANY |
Talk |
Stellar dynamics and star-formation histories of z~1 radio-loud galaxies |
TISANIC |
Kresimir |
Department of Physics, Faculty of Science, University of Zagreb |
CROATIA |
Talk |
Average radio spectral energy distribution of highly star forming galaxies |
CERAJ |
Lana |
Department of Physics, Faculty of Science, University of Zagreb |
CROATIA |
Talk |
Radio luminosity functions of AGN with moderate-to-high radiative luminosities out to z~6 in the COSMOS field |
MARCHESI |
Stefano |
Clemson University |
UNITED STATES |
Talk |
Charactering the AGN population with Chandra COSMOS Legacy: an X-ray spectral approach |
COOKE |
Kevin |
Rochester Institute of Technology |
USA |
Talk |
The Effect of Environment on ULIRGs and Massive Galaxies between 2 < z < 3 |
KROLEWSKI |
Alex |
UC Berkeley |
UNITED STATES |
Talk |
Mapping the z~2 universe using IGM tomography |
COUPON |
Jean |
University of Geneva |
SWITZERLAND |
Talk |
The star formation efficiency in satellite galaxies up to redshift 6 |
NOVAK |
Mladen |
Department of Physics, Faculty of Science, University of Zagreb |
CROATIA |
Talk |
Constraints on nano-Jy radio source populations based on VLA-COSMOS luminosity functions |
MAGNELLI |
Benjamin |
Argelander Institut für Astronomie |
GERMANY |
Talk |
TBD |
HARRINGTON |
Kevin |
Argelander Institute for Astronomie |
GERMANY |
Talk |
Using CO as a Physical Probe of the SF Supply in the Extremely IR-Luminous Planck-Herschel-LMT Detected Galaxies |
KARIM |
Alexander |
AIfA Bonn / ARC Node Germany |
GERMANY |
Talk |
COSMOS ALMA archive -- part I |
JIMÉNEZ-ANDRADE |
Eric Faustino |
Argelander-Institut für Astronomie, Universität Bonn |
GERMANY |
Talk |
Radio continuum size evolution of star forming galaxies in the COSMOS field |
VARDOULAKI |
Eleni |
Argelander-Institut für Astronomie Bonn |
GERMANY |
Talk |
FR-type radio sources in COSMOS: relation to accretion mode and environment |
TYLER |
Krystal |
Rochester Institute of Technology |
USA |
Talk |
The Effect of Environment on Merger Activity, Star Formation, and AGN Activity in the COSMOS Field |
KAJISAWA |
Masaru |
Ehime University |
JAPAN |
|
|
HIMOTO |
Kazuharu |
Ehime University |
JAPAN |
Poster |
Quantitative morphological classification for merging/interacting galaxies at 0.7<z<0.9 in COSMOS |
SATOH |
Yuki |
Ehime University |
JAPAN |
Poster |
The evolution of axial ratio of passive and star-forming galaxies at z<1 in COSMOS |
LAIGLE |
Clotilde |
Sub-department of Astrophysics, department of Physics, University of Oxford |
UNITED KINGDOM |
Talk |
COSMOS2015 probes the impact of filaments on galaxy properties |
NAYYERI |
Hooshang |
UCI |
USA |
Talk |
Massive Galaxies in the COSMOS at z>~3 |
KARTALTEPE |
Jeyhan |
Rochester Institute of Technology |
USA |
Talk |
Morphologies of Luminous Infrared Galaxies at z~2 |
BANDO |
Takuya |
Ehime University |
JAPAN |
Poster |
Clustering properties of passive and star-forming galaxies at z<1.2 in COSMOS as a function of stellar mass |
MCPARTLAND |
Conor |
Inistitute for Astronomy: University of Hawaii at Manoa |
UNITED STATES |
Talk |
TBD |
LANZUISI |
Giorgio |
DIFA-University of Bologna |
ITALY |
Talk |
AGN vs. host galaxy properties in the COSMOS field |
SCHINNERER |
Eva |
MPIA |
GERMANY |
Talk |
COSMOS ALMA archive -- part II |
MOLNAR |
Daniel |
University of Sussex |
UNITED KINGDOM |
Talk |
The infrared-radio correlation of spheroid- and disk-dominated star-forming galaxies to z ~ 1.5 in the COSMOS field |
ODA |
Saeko |
Kyoto University |
JAPAN |
Poster |
Shedding Light on the Compton-thick AGN in the Ultra-luminous Infrared Galaxy UGC 5101 with Broadband X-ray Spectroscopy |
YAMADA |
Satoshi |
Kyoto University |
JAPAN |
Poster |
Broadband X-ray spectral analysis of the double-nucleus LIRG Mrk 463 |
MAEDA |
Fumiya |
Department of Astronomy, Kyoto Univ. |
JAPAN |
Poster |
Evolution of Cosmic Molecular Gas Mass Density from z ∼ 0 to z = 1–1.5 |
STEINHARDT |
Charles |
DARK Cosmology Centre |
DENMARK |
Talk |
Using the Thermal Sunyaev-Zel\'dovich Effect to Measure the Masses of the First Halos |
ILBERT |
Olivier |
LAM |
FRANCE |
|
|
TOFT |
Sune |
Dark Cosmology Centre |
DENMARK |
Talk |
TBD |
DAVIDZON |
Iary |
Caltech |
US |
Talk |
COSMOS galaxy stellar mass function & Co. |
MORITA |
Takashi |
Kyoto univercity |
JAPAN |
|
|
TANIMOTO |
Atsushi |
Kyoto University |
JAPAN |
Poster |
TBD |
SILVERMAN |
John |
Kavli IPMU |
JAPAN |
Talk |
A quintessential merger-induced starburst at z=1.52 with ALMA |
UMEHATA |
Hideki |
Open University of Japan |
JAPAN |
|
|
JIN |
Shuowen |
CEA Saclay |
FRANCE |
Talk |
Super-deblended far-IR to mm photometry in the COSMOS field: catalog and selection of very high redshift candidates |
TANAKA |
Masayuki |
NAOJ |
JAPAN |
Talk |
Hyper Suprime-Cam Subaru Strategic Program |
MAINIERI |
Vincenzo |
ESO |
GERMANY |
Talk |
AGN feedback studies at z~2: combining SINFONI and ALMA |
NEL |
Karel |
University of Witwatersrand Johannesburg |
SOUTH AFRICA |
Talk |
TBD |
SHOPBELL |
Patrick |
Caltech |
USA |
|
|
KIMURA |
Yuki |
Tohoku University |
JAPAN |
Poster |
HSC Variability Research for AGN in the COSMOS field |
INOUE |
Akio |
Osaka Sangyo University |
JAPAN |
Talk |
CHORUS in COSMOS |
NAKAJIMA |
Tadashi |
Astrobiology Center/NAOJ |
JAPAN |
Talk |
Brown dwarf candidates from Hyper Suprime Cam Subaru Strategic Program |
GOZALIASL |
Ghassem |
Finnish Centre for Astronomy with ESO, University of Turku |
FINLAND |
Talk |
Brightest group galaxies: stellar properties and contribution of BGGs to the total baryon content of halos over z<1.3 |
MAWATARI |
Ken |
Osaka Sangyo University |
JAPAN |
Talk |
Balmer break galaxy candidates at z ~ 6 |
HASINGER |
Guenther |
Institute for Astronomy, University of Hawaii |
USA |
Talk |
New Chandra counterparts from ultradeep HSC Imaging in the COSMOS Field |
LI |
Yanxia |
IfA, University of Hawaii at Manoa |
UNITED STATES |
Talk |
Cosmic infrared background fluctuations of the COSMOS field in the SPLASH survey |
YUN |
Min |
University of Massachusetts |
UNITED STATES |
Talk |
COSMOS at LMT |
FUJIMOTO |
Seiji |
University of Tokyo |
JAPAN |
Poster |
DANCING-ALMA I. FIR Size and Luminosity Relation at z = 0 -6 |
KITADA |
Chihiro |
Open University Of Japan |
JAPAN |
|
|
KONISHI |
Jiro |
The Open University of Japan |
JAPAN |
|
|
SUZUKI |
Nao |
Kavli IPMU, University of Tokyo |
JAPAN |
|
|