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dc.contributor.author
Kashino, Daichi
dc.contributor.author
More, Surhud
dc.contributor.author
Silverman, John D.
dc.contributor.author
Daddi, Emanuele
dc.contributor.author
Renzini, Alvio
dc.contributor.author
Sanders, David B.
dc.contributor.author
Rodighiero, Giulia
dc.contributor.author
Puglisi, Annagrazia
dc.contributor.author
Kajisawa, Masaru
dc.contributor.author
Valentino, Francesco
dc.contributor.author
Kartaltepe, Jeyhan S.
dc.contributor.author
Le Fèvre, Olivier
dc.contributor.author
Arimoto, Nobuo
dc.contributor.author
Sugiyama, Naoshi
dc.date.accessioned
2018-01-10T15:57:50Z
dc.date.available
2017-12-15T13:33:04Z
dc.date.available
2018-01-10T15:57:50Z
dc.date.issued
2017-06
dc.identifier.other
10.5281/zenodo.808227
en_US
dc.identifier.uri
http://hdl.handle.net/20.500.11850/221606
dc.identifier.doi
10.3929/ethz-b-000221606
dc.description.abstract
We investigate the properties of dark matter halos that contain "main-sequence" star-forming galaxies at 1.43<z<1.74 using the FMOS-COSMOS survey. The projected correlation function is measured for 516 galaxies down to stellar mass of 109.57 M⦿ and SFR 15 M⦿ yr-1, for which the Hα emission line is detected. We find that these galaxies live in halos of Mh=5×1012 M⦿ on average, which will likely become present-day halos equivalent to the typical mass scale of galaxy groups. We then constrain the stellar-to-halo mass ratio at Mh<1012 M⦿, finding a systematically lower mass ratio than those measured at higher masses.
en_US
dc.language.iso
en
en_US
dc.publisher
ETH Zurich
en_US
dc.rights.uri
http://creativecommons.org/licenses/by/4.0/
dc.title
The FMOS-COSMOS Survey: Properties Of Dark Matter Halos Of Main-Sequence Star-Forming Galaxies At Z 1.6
en_US
dc.type
Conference Poster
dc.rights.license
Creative Commons Attribution 4.0 International
ethz.version.deposit
publishedVersion
en_US
ethz.event
Galaxy Evolution Across Time Conference 2017
en_US
ethz.event.location
Paris, France
en_US
ethz.event.date
June 12-16, 2017
en_US
ethz.publication.place
Zurich
en_US
ethz.publication.status
published
en_US
ethz.leitzahl
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02010 - Departement Physik / Department of Physics::03613 - Lilly, Simon
en_US
ethz.leitzahl.certified
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02010 - Departement Physik / Department of Physics::03613 - Lilly, Simon
en_US
ethz.relation.isVariantFormOf
handle/20.500.11850/227316
ethz.date.deposited
2017-12-15T13:33:05Z
ethz.source
FORM
ethz.eth
yes
en_US
ethz.availability
Open access
en_US
ethz.rosetta.installDate
2018-01-10T15:58:05Z
ethz.rosetta.lastUpdated
2018-01-10T15:58:05Z
ethz.rosetta.versionExported
true
ethz.COinS
ctx_ver=Z39.88-2004&amp;rft_val_fmt=info:ofi/fmt:kev:mtx:journal&amp;rft.atitle=The%20FMOS-COSMOS%20Survey:%20Properties%20Of%20Dark%20Matter%20Halos%20Of%20Main-Sequence%20Star-Forming%20Galaxies%20At%20Z%201.6&amp;rft.date=2017-06&amp;rft.au=Kashino,%20Daichi&amp;More,%20Surhud&amp;Silverman,%20John%20D.&amp;Daddi,%20Emanuele&amp;Renzini,%20Alvio&amp;rft.genre=unknown&amp;rft.btitle=The%20FMOS-COSMOS%20Survey:%20Properties%20Of%20Dark%20Matter%20Halos%20Of%20Main-Sequence%20Star-Forming%20Galaxies%20At%20Z%201.6
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