SINFONI observations of massive galaxies from the GMASS sample at z~2

Slides:

Advertisements

Similar presentations

PI: Michele Cirasuolo Royal Observatory Edinburgh Collaborators: J. Dunlop, R. McLure, F. Cullen, R. Maiolino, R. Ivison, G. Wright, M. Swinbank, R. Sharples,

Advertisements

Daniel Ceverino (HU) Potsdam, 2009 Avishai Dekel (HU), Reem Sari(HU), Tobias Goerdt(HU), Anatoly Klypin (NMSU) High-Redshift Clumpy Disks & Bulges in Cosmological.

Ultra-Deep galaxy surveys with the early build-up of galaxies Olivier Le Fèvre With the DIORAMAS team (F, IT, CH, SP)

Angela Bongiorno Max Planck Institut fuer Extraterrestrische Physik (MPE) Collaborators: Marco Mignoli (INAF-Osservatorio Astronomico di Bologna) Gianni.

Extragalactic AO Science James Larkin AOWG Strategic Planning Meeting September 19, 2004.

Searching for massive galaxy progenitors with GMASS (Galaxy Mass Assembly ultradeep Spectroscopic Survey) (a progress report) Andrea Cimatti (INAF-Arcetri)

Luminous obscured quasars in the HELLAS2XMM survey: the Spitzer perspective Cristian Vignali Dipartimento di Astronomia, Universita`degli Studi di Bologna.

RESULTS AND ANALYSIS Mass determination Kauffmann et al. determined masses using SDSS spectra (Hdelta & D4000) Comparison with our determination: Relative.

Gamma-ray Bursts in Starburst Galaxies Introduction: At least some long duration GRBs are caused by exploding stars, which could be reflected by colours.

Venice – Gregory RudnickMarch 2006 The Mean SED and Stellar Mass Density at z

Star Formation Rates, Ages and Masses of Massive Galaxies in the FORS Deep and GOODS South fields R. Bender, A. Bauer, N. Drory, G. Feulner, A. Gabasch,

High Redshift Massive Galaxies (BzKs & EIS-Deep3a and COSMOS Xu KONG collaborators ：

C. Halliday, A. Cimatti, J. Kurk, M. Bolzonella, E. Daddi, M. Mignoli, P. Cassata, M. Dickinson, A. Franceschini, B. Lanzoni, C. Mancini, L. Pozzetti,

Venice – March 2006 Discovery of an Extremely Massive and Evolved Galaxy at z ~ 6.5 B. Mobasher (STScI)

G. Zamorani On behalf of the VVDS-SWIRE collaboration PI : Carole Lonsdale PI O. Le Fèvre Co-PI G. Vettolani Evolutionary properties of galaxies and mass.

The Properties of LBGs at z>5 Matt Lehnert (MPE) Malcolm Bremer (Bristol) Aprajita Verma (MPE) Natascha Förster Schreiber (MPE) and Laura Douglas (Bristol)

Probing the formation and evolution of massive galaxies with near- to mid-infrared surveys Scuola Nazionale di Astrofisica VIII Ciclo ( ): I Corso.

1 High-z galaxy masses from spectroastrometry Alessio Gnerucci Department of Physics and Astronomy University of Florence 13/12/2009- Obergurgl Collaborators:

Optical Spectroscopy of Distant Red Galaxies Stijn Wuyts 1, Pieter van Dokkum 2 and Marijn Franx 1 1 Leiden Observatory, P.O. Box 9513, 2300RA Leiden,

The assembly of stellar mass during the last 10 Gyr: VVDS results B.Garilli on behalf of the VVDS consortium 1 topic, 4 approaches, concordant results.

Luminosity and Mass functions in spectroscopically-selected groups at z~0.5 George Hau, Durham University Dave Wilman (MPE) Mike Balogh (Waterloo) Richard.

Obscured AGN in the (z)COSMOS survey AGN9, Ferrara, May Angela Bongiorno Max-Planck-Institut für extraterrestrische Physik, Garching, GERMANY AND.

Massive galaxies at z ~ 2 from K20+ Preamble: (Cimatti, Daddi, Fontana, Arimoto, GOODS, GRAPES, COSMOS ) Looking at z~2 massive galaxies gives us more.

Black Hole Growth and Galaxy Evolution Meg Urry Yale University.

Next generation redshift surveys with the ESO-VLT

The Extremely Red Objects in the CLASH Fields The Extremely Red Galaxies in CLASH Fields Xinwen Shu (CEA, Saclay and USTC) CLASH 2013 Team meeting – September.

1 VVDS: Towards a complete census of star formation at 1.4

KASI Galaxy Evolution Journal Club The Morphology of Passively Evolving Galaxies at z~2 from Hubble Space Telescope/WFC3 Deep Imaging in the Hubble Ultra.

AGN 8 - Torino A Panchromatic view of the evolution of Supermassive Black Holes Elisabeta Lusso Dip. di Astronomia, Università di Bologna -

Naoyuki Tamura (University of Durham) The Universe at Redshifts from 1 to 2 for Early-Type Galaxies ~ Unveiling “Build-up Era” with FMOS ~

1 Deep spectroscopic redshift surveys are a central tool to modern Astrophysics Deep redshift surveys (z>0.3) have shaped our current understanding: 

MAMBO 1.2 mm observations of BzK-selected star-forming galaxies at z~2 MAMBO 1.2 mm observations of BzK-selected star-forming galaxies at z~2 H. Dannerbauer.

Metallicity and Black Hole Masses of Redshift 6 Quasars Jaron Kurk (MPIA, D) The evening star (Mucha, 1902) The moon (Mucha, 1902) Fabian Walter, Dominik.

How do galaxies accrete their mass? Quiescent and star - forming massive galaxies at high z Paola Santini Roman Young Researchers Meeting 2009 July 21.

Z-FOURGE - the FourStar Galaxy Evolution Survey Status Report at the 1.3-year mark.

HST Workshop Bologna Jan 31, 2008 Heavily obscured SMBH at high redshift Andrea Comastri INAF - OABologna C. Vignali, R. Gilli, K. Iwasawa, F. Civano,

Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg. 2 !

High-Redshift Galaxies from HSC Deep Surveys Kazuhiro Shimasaku (University of Tokyo) 1. Galaxy Evolution 2. Dropout Galaxies and Lyman α Emitters 3. Observing.

Clustering of BzK-selected galaxies in the COSMOS field Xu KONG collaborators ： A. Renzini, E. Daddi, N. Arimoto, A. Cimatti ， COSMOS.

Clustering and dusty high-z galaxies Emanuele Daddi ESO-Garching (  NOAO-Tucson) Properties of K-selected z=2 galaxies (K20/GOODS/other surveys)  dusty.

High-z AGN Candidates in COSMOS Anton Koekemoer (STScI) + F. Civano, M. Elvis, V. Mainieri, J. Trump, E. Treister, T. Murayama, T. Nagao, Y. Oyama, Y.

How do galaxies accrete their mass? Quiescent and star - forming massive galaxies at high z Paola Santini THE ORIGIN OF GALAXIES: LESSONS FROM THE DISTANT.

David R. Law Hubble Fellow, UCLA The Physical Structure of Galaxies at z ~ John McDonald, CFHT Galaxies in the Distant Universe: Ringberg Castle.

Galactic Astronomy 銀河物理学特論 I Lecture 3-2: Evolution of Luminosity Functions of Galaxies Seminar: Lily et al. 1995, ApJ, 455, 108 Lecture: 2011/12/12.

Formation and evolution of early-type galaxies Pieter van Dokkum (Yale)

X-ray selected Type-2 QSOs and their host galaxies Vincenzo Mainieri with A. Bongiorno, A. Merloni, M. Bolzonella, M. Brusa, M. Carollo, G. Hasinger, K.

SWIRE view on the "Passive Universe": Studying the evolutionary mass function and clustering of galaxies with the SIRTF Wide-Area IR Extragalactic Survey.

Galaxy evolution at high z from mass selected samples. Adriano Fontana (INAF Rome Obs) Thanks to: E. Giallongo, N. Menci, A. Cavaliere, Donnarumma,

The evolution of galaxy sizes since z=3 Ignacio Trujillo (MPIA) & the FIRES team (Trujillo et al. 2004, ApJ, 604, 521) (Trujillo et al. 2005, ApJ, submitted,

Evidence for a Population of Massive Evolved Galaxies at z > 6.5 Bahram Mobasher M.Dickinson NOAO H. Ferguson STScI M. Giavalisco, M. Stiavelli STScI Alvio.

Star Forming Proto-Elliptical z>2 ? N.Arimoto (NAOJ) Subaru/Sup-Cam C.Ikuta (NAOJ) X.Kong (NAOJ) M.Onodera (Tokyo) K.Ohta (Kyoto) N.Tamura (Durham)

Competitive Science with the WHT for Nearby Unresolved Galaxies Reynier Peletier Kapteyn Astronomical Institute Groningen.

What can we learn from High-z Passive Galaxies ? Andrea Cimatti Università di Bologna – Dipartimento di Astronomia.

Understanding the assembly of massive galaxies at z ~ : mid-infrared view from the Spitzer First Look Survey Lin Yan Spitzer Science Center Caltech.

AKARI Spectroscopic Study of the Rest-frame Optical Spectra of Quasars at 3.5 < z < 6.5 Hyunsung Jun¹, Myungshin Im¹, Hyung Mok Lee², and the QSONG team.

Epoch of Reionization  Cosmic Reionization: Neutral IGM ionized by the first luminous objects at 6 < z < 15 Evidence: CMB polarization (Komatsu+2009)

AGN in the VVDS (Bongiorno, Gavignaud, Zamorani et al.) 1.What has been done: main results on Type 1 AGN evolution and accretion properties of faint AGN.

Galaxy Evolution and WFMOS

Observing the formation and evolution of massive galaxies

Subaru UM 2010 on Mitaka First Unbiased Estimates of the Metallicity and Star-Formation Activity of Lyman Alpha Emitters Kimihiko Nakajima(U.

Nobunari Kashikawa （National Astronomical Observatory of Japan）

Probing the Faint Radio Population

The Evolving Luminosity Function of Red Galaxies

The Presence of Massive Galaxies at z>5

Emanuele Daddi ESO K20 survey PI: A Cimatti (Arcetri) Collaborators:

The Starburst-AGN Connection Among COSMOS (U)LIRGs

Kinemetry of High-Redshift Galaxies

Specific Star Formation Rates to z=1.5

QSO2 and their host galaxies

Authod: Ryan L. Sanders et al.(2018)

Presentation transcript:

SINFONI observations of massive galaxies from the GMASS sample at z~2 GMASS3D Jaron Kurk - MPIA, Heidelberg A. Cimatti (P.I.), N. Foerster Schreiber, N. Bouche, G. Cresci, R. Genzel, E. Daddi, A. Renzini, L. Pozzetti, G. Zamorani, M. Mignoli, P. Cassata, A. Franceschini, G. Rodighiero, P. Rosati, M. Dickinson 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) GMASS2D Galaxy Mass Assembly ultra-deep Spectroscopic Survey Ha in H and K band Sample selected with m(4.5mu)<23.0, B<26.5, I<26.5, zphot>1.4, avoid known redshifts. Goals: study galaxies selected on mass, explore redshift desert, high-z LF. Method: SED fitting, up to 30h optical spectroscopy with FORS, total of 145h. Results: ~150 redshifts out of 170 observed, >130 at z>1.4. 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) The 3D sample 18.2 < K < 20.9 9.6 < log M* < 11.0 Selection on exact redshift, estimate of SFR, ACS/NICMOS morphology. Blue: z=1.5, red: z=2.4. 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) GMASS1084 K=19.6 z=1.552 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) GMASS2113 K=20.2 z=1.613 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) GMASS2363 K=21.0 z=2.448 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) GMASS2471 K=20.9 z=2.430 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) Outlook Uniqueness of GMASS SINFONI sample selection in MIR (better measure of mass) deep optical spectroscopy HST optical and (some) NIR coverage deep IRAC and MIPS coverage also includes faint (K>20) targets SINS integration Velocity differences between optical and NIR lines Derive metallicity from (stacked) optical spectra and NIR spectra 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)

Jaron Kurk (MPIA, Heidelberg) 3D2008, Garching Jaron Kurk (MPIA, Heidelberg)