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VISTA
• Managed: UK Astronomy Technology Center (Edinburgh)
• 4-m telescope
• being built at Paranal
• 16 NIR detectors 2k x 2k
• 0.34”/pix
• f.o.v 0.6 deg2, tile into 1.6deg2
Visual Infrared Survey Telescope for Astronomy
ESO Public Surveys• 75% of ESO time on VST (optical) & VISTA (near-infrared) will be devoted to public surveys
• ESO does not have the man-power, open surveys to the community
ESO Public Surveys Policies• ESO issue Call for Public Surveys, periodicity not fixed
• At no time 2 active PS at same RA
• Public Survey Panel (PSP) review proposals
• ESO informs PI’s of PSP recommendations and invites successful PI’s to submit proposals for OPC consideration.
• OPC evaluate
ESO VST Approved PS• KIDS: The Kilo Degree Survey PI: K Kuijken (Leiden + 18 co-I’s). 1500 deg2 in 4 bands in two large areas. Weak lensing is major goal.
• VST Atlas. PI: T Shanks (Durham + 25 co-I’s) 4500 deg2 at SDSS depths. Main goal DE with LRGs (AAOmega)
• VPHAS+ VST photometric H and broad-band survey of the Southern Galactic Plane. PI J Drew (Imperial College + 27 co-I’s). ugri
ESO Announcement of Opportunity for VISTA PS
• January 15: Call for proposals
• March 15: Deadline for submission
• End April: PSP meets
• June: PSP meets with PI’s
• September 29: final proposals deadline
• End October PSP recommendations
• End November OPC recommendations
VDES collaboration• UK and Spain DES participants explore collaborations with already organized groups
• Spain joins ESO
• Decide to put a proposal ourselves
• 37 collaborators, 5 countries, 15 institutions
VISTA Dark Energy Survey• VISTA Public Survey proposal sent to ESO to image the DES area in the near infrared
• Science goals:
Study Dark Energy
Legacy value
• Depth J~21 & Ks~19
• Exposure: J~300s Ks~320s
• 240 nights in 5 years
VISTA Dark Energy SurveyClusters of Galaxies
• Emphasize the improvement in photo-z at high redshift and coverage of the SPT area
VISTA Dark Energy SurveyIntegrated Sachs-Wolfe
• Emphasize again photo-z and the possibility to do ISW tomography
VISTA Dark Energy SurveyLegacy
• 5 magnitudes deeper than 2MASS• galaxy studies: stellar mass• provide sources for VLT instruments (KMOS)• QSOs• Cool objects: low mass stars and solar system objects
VISTA Public Surveys Panel Outcome
• “Interesting proposal”• “it does not optimally match other relevant proposals (SDSS, VST Atlas, KIDS)”• “most of the scientific objectives could be achieved within a revised proposal by McMahon. The PI is encouraged to contact McMahon”
VISTA Public Surveys Panel Outcome
• “The proposal aims to image the entire Southern celestial hemisphere in four bands” (Z,Y,J,K)• “The panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in J+K only”• “The Panel asks the PI to contact Castander …”
VHS: VISTA HEMISPHERE SurveyVHS: VISTA HEMISPHERE Survey
• PI: Richard McMahon (Cambridge)
• Deputy/co-PI: Andy Lawrence (Edinburgh)
• 95 coI’s
VHS: VISTA HEMISPHERE SurveyVHS: VISTA HEMISPHERE Survey
• Southern Hemisphere (20000 deg2) in four bands
• Depth : Z~21.9 (22.4 AB), Y~21.2 (21.8 AB), J~20.2 (21.6 AB) & Ks~18.1 (20.0 AB)
• Exposure: Z~180s, Y~180s, J~60s, K~60s
• 7500 hours => 750 nights
• 7 years
VHS: VISTA HEMISPHERE SurveyVHS: VISTA HEMISPHERE Survey
• legacy ~4 magnitudes deeper than 2MASS
• low mass stars
• LSS out z~1 & DE
• High z QSO’s -> baryonic content during the era of reionization
• merger history and Genesis of our galaxy
• support to ESA cornerstone missions: XMM-Newton, Planck, Herschel & GAIA
VHS-VDES proposal mergingAdapt to ESO’s recommendations
• Explore collaborative proposals
• VHS drops Z & Y over the whole area
• VHS increases time in DES area (VDES reduces time and incorporates H)
• DES provides Y in DES area
• VHS: 800nights 7yr ; VDES: 240nights 5yr;
newVHS: 350nights 5yr
VHS-VDES proposal mergingVHS defines three areas
• VHS-Atlas: 6000 deg2 YJHK 60s : 1120h
• VHS-DES: 4500 deg2 JHK 120s (2nd epoch): 1225h
• VHS-GPS: 8500 deg2 JK 60s : 760h
VISTA Public Surveys Panel & Observing Programme Committee Outcome
• “We are pleased to inform you that based on the feedback of the VISTA Public Survey panel, the Observing Programmes Committee has made to ESO the recommendation to implement your Public Survey proposal: The VISTA Hemisphere Survey (VHS)”
VISTA Public Surveys Panel & Observing Programme Committee Outcome
• Surveys approved: Ultra deep; VIDEO; VIKING; VHS; Magellanic Clouds; Galactic Plane
VISTA Hemisphere SurveyThe Future• Submit a Survey Management Plan Survey observing strategy
Survey data calibration needs
Data reduction process
Manpower & hardware
Data quality assessment process
Data products and VO compliance
Timeline for delivery to ESO archive
VISTA Hemisphere SurveyThe Future
• Schedule:
SMP submission: 2/16/2007
Review by ESO Survey Team feedback: 3/7/2007
SMP resubmission: 4/2/2007
End of SMP review and approval by ESO Director General: end May 2007