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Craig D Mackay
https://people.ast.cam.ac.uk/~optics/people/cdm_career_summary.htm16 Jun 2015: I found a British company (now called E2V Technologies ) working on a new detector called the Charge Coupled Device (CCD). -
New Page 1
https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm16 Jun 2015: 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. -
Chapter 1 - Installation
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter1.htm16 Jun 2015: Before you install your software. If you are using a new PC with your system, it is strongly recommended you check your PC system is functioning correctly. -
14.9 n&v MH NEW
https://people.ast.cam.ac.uk/~rgm/Nature_News_DawnDarkAge.pdf30 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 -
DAZLE – the design Introduction DAZLE, the Dark Ages ...
https://people.ast.cam.ac.uk/~optics/dazle/info/DAZLE%20design%20concept.htm16 Jun 2015: In conjunction with the improved image quality now demonstrated with new 6.5-10 m telescopes, DAZLE will be the only instrument well suited to searching for early star-forming systems -
Submission_HoC_NWE
https://people.ast.cam.ac.uk/~nwe/Culture.pdf11 Oct 2023: Astronomy is a collaborative endeavour. At least some fixed-term contracts can be replaced by open-ended contracts, with people moving to new funding sources as they become available. ... a3877756.html. [10] -
XMM SSC Acronym List
https://people.ast.cam.ac.uk/~xmmssc/ssc-acronyms.html8 Jul 2000: Villafranca Station at Villafranca del Castillo, Spain VLA Very Large Array (Radio Telescope in New Mexico) VOB Vertical Optical Branch V&V Validation and Verification WAN Wide Area Network WFC Wide -
Infrared Installation
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/ir_config.htm16 Jun 2015: Parameters. The new parameters are in five groups at end of the pixcel.ini. ... RUN=0 to 9999999. A run number is inserted into the filename of each fits file written, the number is automatically incremented with each new sequence. -
Peer-reviewed Publications See here for latest list of…
https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Publications.html27 Aug 2022: 4355. 91. R. MacDonald and N. Madhusudhan, HD 209458b in New Light: Detection of Nitrogen Chemistry, Patchy. ... Matsumura, T-S. Pyo, Deep Thermal Infrared Imaging of HR 8799 bcde: New. -
Basic Debris Disk Model
https://people.ast.cam.ac.uk/~wyatt/wyat06c.pdf13 Oct 2006: New disks: >30mJy (none), 10-30mJy (5), 3-10mJy (9). • Mean flux of non-detections is 0.3mJy. • ... Expect some structures explained by current models. • For others new dynamical models will be developed.
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