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LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...
https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf19 Apr 2006: Our observations provide new information aboutthe distribution of the color temperature and optical depthstructure of this region. ... The high resolution of mid-infrared detec-tors on new large telescopes, such as Gemini, VLT, and theGTC, will permit -
L187 The Astrophysical Journal, 619:L187–L190, 2005 February 1� 2005. …
https://people.ast.cam.ac.uk/~wyatt/ghwd05.pdf19 Apr 2006: ABSTRACT. New submillimeter images have been obtained of the dust disk around the nearby K2 V stare Eridani, withthe total data set now spanning 5 yr. ... 4. DISCUSSION. The new images of thee Eri dust ring confirm its structureand dimensions, and the -
SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…
https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf19 Apr 2006: Received 2002 April 17; accepted 2002 September 20. ABSTRACT. New submillimeter images of the cold dust emission around the nearby main-sequence star Fomalhaut arepresented. ... object. 5. CONCLUSIONS. We have presented new, high signal-to-noise ratio sub -
Quasars and Galaxies at the Highest Redshifts
https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt8 Mar 2006: GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad band background. ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of 0.1 per cent are needed compared with 1% -
Oxford Meeting
https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt15 Apr 2006: Infrared OH Sky Observations: Mahaira etal, 1993, PASP. GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of -
L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...
https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf19 Apr 2006: Here we present new mid-IR observations of the Vega-likestar HD 141569 (B9.5 Ve). -
mnr7957.tex
https://people.ast.cam.ac.uk/~wyatt/gwhd04.pdf19 Apr 2006: A new 850-µmimage shows that there is indeed such a debris disc, extending out to 55 au (15 arcsec)radius. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061009.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061009.txt21 Oct 2006: Progress is being made - ongoing EGS has made the new ING archive interface the default one. ... He also noted that various UKIRT new project Letters of Intent were being circulated to those likely to interested. -
Dust_in_the_Debris_Disk_Around_HD69830_09Nov2006
https://people.ast.cam.ac.uk/~wyatt/lbbw07.pdf16 Nov 2006: A set of components was tested. exhaustively before the addition of a new species was allowed, and only species that reduced. ... New work by Wyatt et al. (2007) also demonstrates that it is highly unlikely that an asteroid. -
Pipeline CalibrationSimon Hodgkin(paper in prep) Outline • UKIRT…
https://people.ast.cam.ac.uk/~wfcam/talks/hodgkin_ukidss_jul06.pdf3 Aug 2006: New measures:• MAGZPT• MAGZRR (per frame ‘error’)• NIGHTZPT• NIGHTZRR (per night ‘error’). •
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