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MHONGOOSE MeerKAT HI Observations of Nearby Galactic Objects: - PowerPoint PPT Presentation

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MHONGOOSE MeerKAT HI Observations of Nearby Galactic Objects: Observing Southern Emitters Friday, 7 May 2010 Investigators Name Affiliation Country Name Affiliation Country Erwin de Blok Univ of Cape Town South Africa Stacy McGaugh

  1. MHONGOOSE MeerKAT HI Observations of Nearby Galactic Objects: Observing Southern Emitters Friday, 7 May 2010

  2. Investigators Name Affiliation Country Name Affiliation Country Erwin de Blok Univ of Cape Town South Africa Stacy McGaugh Univ of Maryland USA Gerhardt Meurer ICRAR Australia Philippe Amram Lab. Astroph. Marseille France Martin Meyer ICRAR Australia Lia Athanassoula Lab. Astroph. Marseille France Se-Heon Oh Univ of Cape Town South Africa Chantal Balkowski Obs de Paris France Tom Oosterloo ASTRON Netherlands Matt Bershady Univ of Wisconsin USA D.J. Pisano West Virginia University USA Rob Beswick Jodrell Bank UK Simon Ratcliffe SKA SA South Africa Frank Bigiel Univ Berkeley USA Jerry Sellwood Rutgers Univ USA Sarah Blyth Univ of Cape Town South Africa Eva Schinnerer MPIA Germany Albert Bosma Lab. Astroph. Marseille France Anja Schröder HartRAO South Africa Roy Booth HartRAO South Africa Kartik Sheth NRAO USA Antoine Bouchard McGill Univ Canada Kristine Spekkens RMC Canada Elias Brinks Univ of Hertfordshire UK Snezana Stanimirovic Univ of Wisconsin USA Claude Carignan Univ de Ouagadougou Burkina Faso Kurt van der Heyden Univ of Cape Town South Africa Laurent Chemin Obs de Paris France Wim van Driel Obs de Paris France Françoise Combes Obs de Paris France Lourdes Verdes- IAA, Granada Spain John Conway Chalmers Univ Sweden Montenegro Simon Cross SKA SA South Africa Fabian Walter MPIA Germany Jayanne English Univ Manitoba Canada Bradley Warren ICRAR Australia Benoit Epinat Lab. Astroph. Marseille France Tobias Westmeier ATNF Australia Bradley Frank Univ of Cape Town South Africa Eric Wilcots Univ of Wisconsin USA Jason Fiege Univ Manitoba Canada Ted Williams Rutgers Univ USA Jay Gallagher Univ of Wisconsin USA Patrick Woudt Univ of Cape Town South Africa Brad Gibson Univ Lancaster UK Albert Zijlstra Univ Manchester UK George Heald ASTRON Netherlands Trish Henning Univ New Mexico USA Benne Holwerda Univ of Cape Town South Africa Jasper Horrell SKA SA South Africa Helmut Jerjen RSAA, ANU Australia Hans-Rainer Klöckner Oxford Univ UK 57 investigators from 12 countries Bärbel Koribalski ATNF Australia (SA 14, USA 12, FRA 8, AUS 6, UK 5, ...) Renée Kraan-Korteweg Univ of Cape Town South Africa Stephane Leon ESO Chile Adam Leroy NRAO USA Ilani Loubser UWC South Africa Continued on Next Page. . . Friday, 7 May 2010

  3. Investigators Name Affiliation Country Name Affiliation Country Erwin de Blok Univ of Cape Town South Africa Stacy McGaugh Univ of Maryland USA Gerhardt Meurer ICRAR Australia Philippe Amram Lab. Astroph. Marseille France Martin Meyer ICRAR Australia Lia Athanassoula Lab. Astroph. Marseille France Se-Heon Oh Univ of Cape Town South Africa Chantal Balkowski Obs de Paris France Tom Oosterloo ASTRON Netherlands Matt Bershady Univ of Wisconsin USA D.J. Pisano West Virginia University USA Rob Beswick Jodrell Bank UK Simon Ratcliffe SKA SA South Africa Frank Bigiel Univ Berkeley USA Jerry Sellwood Rutgers Univ USA Sarah Blyth Univ of Cape Town South Africa Eva Schinnerer MPIA Germany Albert Bosma Lab. Astroph. Marseille France Anja Schröder HartRAO South Africa Roy Booth HartRAO South Africa Kartik Sheth NRAO USA Antoine Bouchard McGill Univ Canada Kristine Spekkens RMC Canada Elias Brinks Univ of Hertfordshire UK Snezana Stanimirovic Univ of Wisconsin USA Claude Carignan Univ de Ouagadougou Burkina Faso Kurt van der Heyden Univ of Cape Town South Africa Laurent Chemin Obs de Paris France Wim van Driel Obs de Paris France Françoise Combes Obs de Paris France Lourdes Verdes- IAA, Granada Spain John Conway Chalmers Univ Sweden Montenegro Simon Cross SKA SA South Africa Fabian Walter MPIA Germany Jayanne English Univ Manitoba Canada Bradley Warren ICRAR Australia Benoit Epinat Lab. Astroph. Marseille France Tobias Westmeier ATNF Australia Bradley Frank Univ of Cape Town South Africa Eric Wilcots Univ of Wisconsin USA Jason Fiege Univ Manitoba Canada Ted Williams Rutgers Univ USA Jay Gallagher Univ of Wisconsin USA Patrick Woudt Univ of Cape Town South Africa Brad Gibson Univ Lancaster UK Albert Zijlstra Univ Manchester UK George Heald ASTRON Netherlands Trish Henning Univ New Mexico USA Benne Holwerda Univ of Cape Town South Africa Jasper Horrell SKA SA South Africa Helmut Jerjen RSAA, ANU Australia Hans-Rainer Klöckner Oxford Univ UK 57 investigators from 12 countries Bärbel Koribalski ATNF Australia (SA 14, USA 12, FRA 8, AUS 6, UK 5, ...) Renée Kraan-Korteweg Univ of Cape Town South Africa Stephane Leon ESO Chile Adam Leroy NRAO USA Ilani Loubser UWC South Africa Continued on Next Page. . . Friday, 7 May 2010

  4. Motivation • SKA Key Science Question: “How do galaxies assemble and evolve?” • SKA and precursors will study evolution of HI content over cosmic time • Difficult to study sub-kpc physical processes • Comprehensive study of nearby galaxies to characterise “Galactic Ecosystem” Friday, 7 May 2010

  5. Why MeerKAT? • Excellent column density sensitivity: • low column density HI • outer disks, • infall, outflow, accretion • connection with cosmic web • High resolution • detailed dynamics • relation between gas and star formation Friday, 7 May 2010

  6. Point source sensitivity Sensitivities other telescopes according to their exposure calculators MeerKAT Friday, 7 May 2010

  7. Key Science Questions • The distribution of dark matter in galaxies and comparison with dark matter models • The importance and effects of cold gas accretion • Detection of link between galaxies and cosmic web • Relation between dark and baryonic matter on galactic scales Friday, 7 May 2010

  8. The Sample • Select from HICAT, NHICAT and K04 • Declination < +25 degrees • V LG < 1500 km s -1 (D<20 Mpc) • |b| > 20 degrees • Select equal number in bins of log(M HI ) • 20 galaxies per bin to get good (M HI , cos i) coverage: 301 galaxies Friday, 7 May 2010

  9. Friday, 7 May 2010

  10. Observations • Observe all 301 galaxies for 8 hours • 5 σ of 5 × 10 20 cm -2 at 10” over 16 km s -1 with 5 km s -1 chans • Edge of “star forming disk” • Observe 10% for 200 hours • 5 σ of 1.2 × 10 19 (5 × 10 17 ) cm -2 at 30” (90”) over 16 km s -1 with 5 km s -1 chans • Outer disk, accretion, cosmic web Friday, 7 May 2010

  11. Observations • Total observing time required: 8216 hours • Parallel multi-wavelength effort • Investigate flexible pipelines • Investigate automated galaxy characterization (GALAPAGOS) Friday, 7 May 2010

  12. Why more? • Previous surveys exist: why observe more? • No survey covers complete range in properties • Heterogeneous combination does not work • All THINGS galaxies had already been observed before THINGS Friday, 7 May 2010

  13. Friday, 7 May 2010

  14. Friday, 7 May 2010

  15. • Does an HI selected sample provide a comprehensive view of the local galaxy population? Friday, 7 May 2010

  16. Black: HICAT Red: MHONGOOSE Friday, 7 May 2010

  17. Observations • Observe all 301 galaxies for 8 hours • 5 σ of 5 × 10 20 cm -2 at 10” over 16 km s -1 with 5 km s -1 chans • Edge of “star forming disk” • Observe 10% for 200 hours • 5 σ of 1.2 × 10 19 (5 × 10 17 ) cm -2 at 30” (90”) over 16 km s -1 with 5 km s -1 chans • Outer disk, accretion, cosmic web Friday, 7 May 2010

  18. HALOGAS • HALOGAS at WSRT • low column density detections in ~20 northern spirals and dwarfs Figure 2: Comparison of shallow THINGS and deep HALOGAS observations of NGC 925. Left: The HI distribution in NGC 925 from THINGS, convolved to the WSRT resolution. Lowest contour at 9 · 10 19 cm − 2 , with each contour double the previous value. Center: False-color image of the baryonic components. Colors as in Fig. 1. Right: The HI distribution as observed by the deep WSRT HALOGAS survey. Lowest contour 1.8 · 10 19 cm − 2 with each contour double the previous value. (HI maps: courtesy G.Heald and the HALOGAS collaboration.) Friday, 7 May 2010

  19. HALOGAS coverage HALOGAS MHONGOOSE Friday, 7 May 2010

  20. V LG < 500 km s -1 500 < V LG < 1000 km s -1 1000 < V LG < 500 km s -1 Sky distribution of MHONGOOSE sample Friday, 7 May 2010

  21. MHONGOOSE timeline 2010/ 2012 2013 2014 2015 2016 2017 2011 Observations Deep Survey Test Test MeerKAT observations observations Observing proto-MeerKAT KAT -7 Observations Shallow Survey Develop pipeline Develop pipeline Refine pipeline Data Reduction using KAT -7 data using proto- using MeerKAT (deconvolution Production run MeerKAT data data and related) Shallow survey: Shallow survey: Shallow survey: data release 1 data release 2 data release 3 Data Release Deep survey: data Deep survey: data Deep survey: data release 1 release 2 release 3 SALT ALMA Multi-Wavelength S 4 G 3DNTT Single Dish Survey design Letter with early Letter with First First data paper Final data paper Papers paper results Results shallow survey shallow survey Science Papers Test and optimize Software Production run GalAPAGOS Friday, 7 May 2010

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