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Durham August 07 Wide-field surveys, and opportunities in the near-infrared Steve Warren Imperial College London UKIDSS Survey Scientist Homework: Lawrence ‘Wide Field Surveys and Astronomical Discovery Space’ arXiv:0704.0809
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Durham August 07 A lovely bunch
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Durham August 07 1.What are surveys useful for? 2. The current state of the art 3. Some highlights from SDSS and 2MASS 4. Opportunities in the near-infrared with UKIDSS - What is the near-infrared good for? - Technical issues - Two headline science goals 5. The near future
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Durham August 07 What are surveys useful for? 1. Efficient use of telescope time 2. Archive - things you haven’t thought of 3. Serendipitous discoveries
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Durham August 07 What are surveys useful for? Discovery of Uranus (1781)
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Durham August 07 Sandage (telescope proposal) “Not all astronomical sources have been observed at all wavelengths. We propose to remedy this.”
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Durham August 07
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HUDF contains 10040 sources (galaxies) Area 3.2x10 -3 deg 2 Area sky 41253 deg 2 Sandage’s goal is detection of 10 11 galaxies (and 10 11 stars) at all wavelengths
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Durham August 07 Current state of the art in surveys
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Durham August 07 Highlights from SDSS 1. Baryonic acoustic oscillations
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Durham August 07 Highlights from SDSS 2. High-redshift z>6 quasars
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Durham August 07 Highlights from SDSS 3. Structure in the Milky Way halo
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Durham August 07 1,2,3 made possible by archive tool
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Durham August 07 Highlights from 2MASS 1. All sky atlases
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Durham August 07 Highlights from 2MASS 2. Brown dwarfs
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Durham August 07 Highlights from 2MASS 2. Brown dwarfs
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Durham August 07 Opportunities in the near-infrared with UKIDSS 1. What is the near-infrared good for? 2. Technical issues 3. Two headline science goals
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Durham August 07 1. What is the near-infrared good for? Near-infrared explores the cool, the dust-obscured, and the high-redshift universe
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Durham August 07 2MASS too shallow cf SDSS LAS best for rare objects DXS, UDS well suited to old stellar pops at high z DXS, SWIRE well matched
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Durham August 07 2. Technical issues
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Durham August 07 2. Technical issues 4x2048x2048 Hawaii II arrays 0.4 arcsec pixels 0.21 sq.degs / exposure Filters: Z,Y,J,H,K,H 2 -S(1),Br-g 1 deg 2 K=19.5 / hr (5sig) etendue 2.38 m 2 deg 2
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Durham August 07 UKIRT Wide Field Camera (WFCAM)
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Durham August 07 UKIDSS design 5 elements of UKIDSS Large Area SurveyLASYJHK18.4K4000 s.d.262nExGal Deep Extragalactic SurveyDXSJK21.035118ExGal Ultra Deep SurveyUDSJHK23.00.77296ExGal Galactic Plane SurveyGPSJHK19.01800186Gal Galactic Clusters SurveyGCSZYJHK18.7120084Gal
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Durham August 07 UKIDSS design Large Area SurveySDSS near-ir photom, Y dwarfs, KX quasars, z=7 quasars Deep Extragalactic SurveyMultiwavelength fields, the Universe at 1<z<1.5, FMOS spec Ultra Deep SurveyMultiwavelength field SXDS, the Universe at z=3 Galactic Plane SurveyGalactic-plane atlas -5<b<+5 Galactic Clusters SurveyUniversality of the stellar IMF
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Durham August 07 UKIDSS design ESO public survey 1000 nights UKIRT over 7yrs UKIDSS = 100 X 2MASS near-ir SDSS began 2005 May 13 surveyP/P 2MASS V/V 2MASS LAS297.0 GPS407.2 GCS122.5 DXS312.2 UDS270.8 total13919.7
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Durham August 07 2MASS
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Durham August 07 Headline science: z>6.4 quasars SDSS limit z=6.4 z=6 quasar spectra indicate reionisation nearly complete by z=6.2
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Durham August 07 Headline science: z>6.4 quasars At Y<19.5 expect: 1 quasar z>6 in 150 sq degs 1 quasar z>6.4 in 300 sq degs EDR indicates contamination only 20:1
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Durham August 07 Headline science: the search for Y dwarfs
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Durham August 07 Headline science: the search for Y dwarfs
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Durham August 07 Headline science: the search for Y dwarfs ULAS J0034 the coolest brown dwarf
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Durham August 07 Data access http://surveys.roe.ac.uk/wsa Flexible query tool providing access to: Images Detection tables Source tables Registration by institution, with approved list monitored by community contact. e.g. imperial.ac.uk get username and pwd from SJW
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Durham August 07 The near future VISTA near-ir WISE mid-ir Herschel far-ir 2008 2009 2008
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