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  2. SOMs 4 OGLE

    https://people.ast.cam.ac.uk/~vasily/ogle_som/index.html
    29 Jan 2009: from the list of new eruptive cataclysmic variables toward the Galactic Bulge by Cieslinki et al.
  3. Craig D Mackay

    https://people.ast.cam.ac.uk/~cdm/cdm_career_summary.htm
    14 May 2009: I found a British company (now called E2V Technologies ) working on a new detector called the Charge Coupled Device (CCD).
  4. SOMs 4 OGLE

    https://people.ast.cam.ac.uk/~vasily/ogle_som/map2.html
    29 Jan 2009: from the list of new eruptive cataclysmic variables toward the Galactic Bulge by Cieslinki et al.
  5. New Page 1

    https://people.ast.cam.ac.uk/~cdm/cdm_CV_130509.htm
    14 May 2009: In addition a new detector system that allows the spectrum of the fringe pattern to be detected has been developed. ... Following that a new CCD system was built by CDM and used on the Anglo-Australian Telescope (AAT) in 1981.
  6. 14.9 n&v MH NEW

    https://people.ast.cam.ac.uk/~rgm/Nature_News_DawnDarkAge.pdf
    30 Mar 2009: The new (O2)4 structure is not the lowest-energy structure at this level of theory, demonstrating the need for additional studies. ... sensitive detectors have arrived on wide-field imaging instru-ments, on a new generation of 8-metre-aper-ture telescopes
  7. Craig  Mackay

    https://people.ast.cam.ac.uk/~cdm/cdm_pub_list_130509.htm
    14 May 2009: Moshut. Woodbury, New York : American Institute of Physics, 1998. (AIP conference proceedings ; 428), p.499. ... S. Young, and D. F. Buscher. A new photon counting spectrometer for the COAST.
  8. Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...

    https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf
    12 Jan 2009: Sub-mm. Far-IR. Mid-IR. Good news: different wavelengths see different grain sizes and different structures. ... Bad news: both spatial distribution τ1/r and temperature of far-IR dust implies mass loss of 2M/Myr.
  9. Debris discs around nearby solar analogues

    https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf
    8 Jul 2009: Discs were detected with moderate frequencyfor stars a few hundred Myr old, but no new detections were madefor ages comparable to the Sun’s 4.5 Gyr. ... No new discover-ies were made among the 13 stars observed, but the Infrared SpaceObservatory (ISO)
  10. lecture3_extrasolarplanets

    https://people.ast.cam.ac.uk/~wyatt/lecture3_extrasolarplanets.pdf
    28 Jan 2009: Direct detection techniques are now possible • Direct imaging. New techniques are also being developed • Disk structures.
  11. survey07_rev2.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwbm09.pdf
    21 Jul 2009: 2006) but reanalyzed here in a consistent fashion with the new data of Table 3. ... 2006) but reanalyzed here in a con-sistent fashion with the new data of Tables 3 and 4.
  12. 11626.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh09.pdf
    23 Jun 2009: Insection 4 we present new VISIR imaging of HD69830 showingthat the excess emission at 18.72µm is not-extended, and discussthe implications for the maximum extent of the disc. ... 2008), we have new data obtained on VISIR at. the VLT under proposal 079.C
  13. Planets and Debris Disks: Results from a Spitzer/MIPS Search ...

    https://people.ast.cam.ac.uk/~wyatt/bbcr09.pdf
    15 Sep 2009: or more planets. Combining this new data with 42 already published observa-.
  14. Mon. Not. R. Astron. Soc. 000, 000–000 (2009) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/bwmm09.pdf
    19 Jun 2009: Mon. Not. R. Astron. Soc. 000, 000–000 (2009) Printed 19 June 2009 (MN LATEX style file v2.2). The History of the Solar System’s Debris Disc: ObservableProperties of the Kuiper Belt. Mark Booth1?, Mark C. Wyatt1, Alessandro Morbidelli2, Amaya
  15. arX iv:0 911. 3426 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/pgdm09.pdf
    19 Nov 2009: 1997). HIPgn I/239 Hipparcos General Notes (Perryman et al. 1997)HIPnr I/311 Hipparcos, the New Reduction of the Raw Data (van Leeuwen 2007)LHS I/279 Revised Luyten ... van Leeuwen F., 2007, Hipparcos, the New Reduction ofthe Raw Data, Springer /

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