Subaru Weak Lensing Survey: Hyper Suprime-Cam

Slides:



Advertisements
Similar presentations
EUCLID : From Dark Energy to Earth mass planets and beyond Jean-Philippe Beaulieu Institut dAstrophysique de Paris Dave Bennett University of Notre Dame.
Advertisements

Yuichi Matsuda (NAOJ) 松田 有一(国立天文台) Ly-alpha morphology-density high-z 1.
1 COSMOS Dark Matter Maps with COSMOS Jason Rhodes (JPL) January 11, 2005 San Diego AAS Meeting For the COSMOS WL team : (Justin Albert, Richard.
ASIAA Research Highlights and Prospects with HSC Keiichi Umetsu, ASIAA SAC HSC Science Workshop
CLASH: Cluster Lensing And Supernova survey with Hubble ACS Parallels WFC3 Parallels 6 arcmin. = 2.2 z=0.5 Footprints of HST Cameras: ACS FOV in.
Weak Lensing Study of DM sub halos in Coma Cluster T. Futamase Astronomical Institute, Tohoku University, Sendai, Japan 29 th Apr. Collaborators:
R. Pain9/18/2008 LSST-SNAP complementarity Reynald Pain IN2P3/LPNHE Paris, France Page 1.
General introduction: HSC collaboration meeting at Princeton Yasushi Suto Department of Physics, The University of Tokyo (Global Scholar, Dept. of Astrophys.
Weak lensing mass-selected cluster catalogues Richard Massey (CalTech) with Justin Albert (CalTech), Joel Berge (Saclay), Richard Ellis (CalTech), Takashi.
Nikos Nikoloudakis and T.Shanks, R.Sharples 9 th Hellenic Astronomical Conference Athens, Greece September 20-24, 2009.
Statistics of the Weak-lensing Convergence Field Sheng Wang Brookhaven National Laboratory Columbia University Collaborators: Zoltán Haiman, Morgan May,
WISH upon a first galaxy….. WISH Wide-field Imaging Surveyor for High-Redshift WISH Working Group M31 Phot: R.Gendler.
Non-Gaussian signatures in cosmic shear fields
14-16 January, 2009Subaru User’s Meeting (NAOJ) Possible Collaboration between Seoul National University and Subaru Myungshin Im (CEOU/Astronomy Seoul.
FMOS で探る Extremely Red Universe II. FMOS で探る Extremely Red Universe II. Extremely Red Universe Probed with FMOS Extremely Red Universe Probed with FMOS.
Non-Gaussian signatures in cosmic shear fields Masahiro Takada (Tohoku U., Japan) July 6 th IAP Based on collaboration with Bhuvnesh Jain (Penn) (MT.
Observational test of modified gravity models with future imaging surveys Kazuhiro Yamamoto (Hiroshima U.) Edinburgh Oct K.Y. , Bassett, Nichol,
Report from Subaru Advisory Committee The main issues of the current SAC: ・ Extensive (strategic) program of Subaru telescope ・ International collaborations.
Upgrade plan of the MOA 1.8-m telescope F. Abe MOA collaboration 19 Jan. 2009, 13th Microlensing Paris.
Dark Energy Probes with DES (focus on cosmology) Seokcheon Lee (KIAS) Feb Section : Survey Science III.
PAU survey collaboration: Barcelona (IFAE, ICE(IEEC/CSIC), PIC), Madrid (UAM & CIEMAT), València (IFIC & UV), Granada (IAA) PAU survey Physics of the Accelerating.
Testing the Shear Ratio Test: (More) Cosmology from Lensing in the COSMOS Field James Taylor University of Waterloo (Waterloo, Ontario, Canada) DUEL Edinburgh,
The FMOS Facility for the SUBARU telescope Gavin Dalton Oxford/RAL.
Data Analysis Software Development Hisanori Furusawa ADC, NAOJ For HSC analysis software team 1.
Subaru Galaxy Surveys: Hyper-Suprime Cam & WFMOS (As an introduction of next talk by Shun Saito) Masahiro Takada (Tohoku Univ., Sendai, Japan) Sep
Michael Levi (Lawrence Berkeley National Laboratory), M. Lampton (UCBerkeley Space Sciences Lab), and M. Sholl (UCBerkeley Space Sciences Lab) WFIRST:
Initial Results from the Chandra Shallow X-ray Survey in the NDWFS in Boötes S. Murray, C. Jones, W. Forman, A. Kenter, A. Vikhlinin, P. Green, D. Fabricant,
1 Optical observations of asteroids – and the same for space debris… Dr. D. Koschny European Space Agency Chair of Astronautics, TU Munich Stardust school.
Wide-field Weak Lensing Mass Reconstructions of Merging Galaxy Clusters Brett Ragozzine, Douglas Clowe Ohio University, Department of Physics & Astronomy,
Array for Microwave Background Anisotropy AMiBA SZ Science AMiBA Team NTU Physics Figure 4. Simulated AMiBA deep surveys of a 1deg 2 field (no primary.
INFRARED-BRIGHT GALAXIES IN THE MILLENNIUM SIMULATION AND CMB CONTAMINATION DANIEL CHRIS OPOLOT DR. CATHERINE CRESS UWC.
Precision Studies of Dark Energy with the Large Synoptic Survey Telescope David L. Burke SLAC for the LSST Collaboration Rencontres de Moriond Contents.
BAOs SDSS, DES, WFMOS teams (Bob Nichol, ICG Portsmouth)
The Large Synoptic Survey Telescope and Precision Studies of Cosmology David L. Burke SLAC C2CR07 Granlibakken, California February 26, 2007 Brookhaven.
Weak Lensing Alexandre Refregier (CEA/Saclay) Collaborators: Richard Massey (Cambridge), Tzu-Ching Chang (Columbia), David Bacon (Edinburgh), Jason Rhodes.
Brenna Flaugher for the DES Collaboration; DPF Meeting August 27, 2004 Riverside,CA Fermilab, U Illinois, U Chicago, LBNL, CTIO/NOAO 1 Dark Energy and.
Probing Dark Energy with Cosmological Observations Fan, Zuhui ( 范祖辉 ) Dept. of Astronomy Peking University.
A Search for High Redshift Galaxies behind Gravitationally Lensing Clusters Kazuaki Ota (Kyoto U) Johan Richard (Obs.Lyon), Masanori Iye (NAOJ), Takatoshi.
Cluster Catalogs from 161 deg 2 of CFHTLS-Wide gri imaging Karun Thanjavur Supervisors:Dr. David Crampton, HIA/ UVic Dr. Jon Willis, UVic SL2S Meeting,
Jochen Weller Decrypting the Universe Edinburgh, October, 2007 未来 の 暗 黒 エネルギー 実 験 の 相補性.
Cosmological Inference from Imaging Surveys Bhuvnesh Jain University of Pennsylvania.
1 Near-Earth objects – a threat for Earth? Or: NEOs for engineers and physicists Lecture 2 – From observations to measurements Dr. D. Koschny (ESA) Prof.
Z Equals Twenty from Antarctica Lifan Wang. 宇宙学 Type Ia SNe at Maximum.
Galaxy Evolution and WFMOS
LSST Commissioning Overview and Data Plan Charles (Chuck) Claver Beth Willman LSST System Scientist LSST Deputy Director SAC Meeting.
The Dark Energy Survey Probe origin of Cosmic Acceleration:
LSST Commissioning Overview and Data Plan Charles (Chuck) Claver Beth Willman LSST System Scientist LSST Deputy Director SAC Meeting.
Weak Lensing Flexion Alalysis by HOLICs
A photometric method to classify high-z supernovae found with HSC
DEEP LENS SURVEY Long term dual hemisphere campaign
The influence of Dark Energy on the Large Scale Structure Formation
Review of Gravitational Lensing:
Cosmological Constraints from the Double-
Subaru UM 2010 on Mitaka First Unbiased Estimates of the Metallicity and Star-Formation Activity of Lyman Alpha Emitters Kimihiko Nakajima(U.
The LSST and Observational Cosmology
The FLAMINGOS Extragalactic Survey
Nobunari Kashikawa (National Astronomical Observatory of Japan)
Clustering of galaxies around AGN in the HSC Wide survey
in a Large-Scale Structure at z=3.1
Complementarity of Dark Energy Probes
Probing the Dark Universe with Weak Gravitational Lensing
(Science Operation Division Chief)
Hint something is wrong with cluster evolution model:
Subaru Weak Lensing Study of Seven Merging Clusters of Galaxies
OWLS Pipeline Status Report
Extragalactic Background Fluctuation from the Numerical Galaxies
Cluster Cosmology in Deep Fields
Solar System Science with Subaru and HSC
Multi-Messenger Astronomy with Subaru II
6-band Survey: ugrizy 320–1050 nm
Presentation transcript:

Subaru Weak Lensing Survey: Hyper Suprime-Cam Masahiro Takada (Tohoku U.) Takashi Hamana (NAOJ) Satoshi Miyazaki (NAOJ) on behalf of HSC WLWG Aug ? 07 @ JPL

Hyper Suprime-Cam (HSC) Replace the Subaru prime focus camera with the new one (HSC) PI: S. Miyazaki (NAOJ) The grant (~$15M) to build the new camera was approved in 2006 Construction: 2006-2011 FoV: 1.5 - 2.0 degrees in diameter (~10  the Suprime-Cam’s FoV) 4 - 5 broad band filters (BVRiz) available The first light in 2010 - 2011 Plan to conduct a wide-field survey (primarily for WL); hopefully starting from 2011 for 3-5 years

Suprime-Cam From Y. Komiyama 2 degree FoV option

HSC observing conditions for WL HSC is designed to preserve image quality of the current Suprime-Cam Galaxy number density usable for WL as a function of exposure time Typical seeing size ~ 0.6’’

One case for survey parameters Area: ~2,000 deg^2 Limiting Mag. (AB): B~26,V~26,R~26, i’~25.8, z’~24.3 Exposure time (min): 15(B, V, R, z’), 30 (i’) Nights: 150-300 nights (starting from 2011 for 3-5 years) Targeted Fields: TBD *Limiting mag. is for 10 detection of 1 square arcsecond aperture *i’-band data is used for weak lensing analysis Survey parameters above are preliminary and DE case is considered here because it is primary science case However, survey must be eventually optimized to also achieve several other science cases including “galaxy evolution study” in order to obtain final acceptance from Japanese astronomy community An optimal survey design for DE case is being carefully investigated using the Suprime-Cam data

HSCWLS performance (WLT+CC+CMB) 9 parameters (_de, w0, wa, A_s, ns, alpha, wm, wb, tau) within a CDM model The forecasts are for WLT + CMB (blue), cluster counting (CC) + CMB (green), WLT + CC + CMB (orange) (w_constant)~0.05 Include the non-Gaussian errors of WLT (MT & Jain 07 in prep.) and the covariance between CC and WLT (MT & Bridle 07) However, not include model systematics of each experiment