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https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt
https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt17 Mar 2006: o Legacy value, Serendipity and new classes of object. o Maximising the science return from ESA missions, XMM-Newton, Planck, Herschel and GAIA. -
https://people.ast.cam.ac.uk/~rgm/vhs/PSP_feedback_VHS_McMahon.txt
https://people.ast.cam.ac.uk/~rgm/vhs/PSP_feedback_VHS_McMahon.txt18 Jul 2006: The Panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in JK only. -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/26 Jan 2006: The good news is these artefacts are non-astronomical in appearance and do not "talk" across the detector quadrant boundaries, or between detectors; the bad news is that they do not ... Darks. The darks, including new improved residual reset anomaly now -
L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...
https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf19 Apr 2006: All rights reserved. Printed in U.S.A. NEW SUBMILLIMETER LIMITS ON DUST IN THE 55 CANCRI PLANETARY SYSTEM. ... 2000), which was already a factor of 100 below. L96 NEW SUBMILLIMETER OBSERVATIONS OF 55 CNC Vol. -
Dark Exposure Properties of VIRCAM Detectors
https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_darkreport/vircam_darkreport.html21 Oct 2006: The new detector 10 doesn't have this sort of problem nor do any of the others. ... Having this level of redundancy is excellent news if we want to use the data themselves to correct the problem. -
CASU analysis of WFCAM commissioning data - I
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/2 Nov 2006: taken roughly in the middle of the night (and as it happens also taken within 4 days of new moon). -
, EUROPEAN SOUTHERN OBSERVATORY Organisation Européenne pour des…
https://people.ast.cam.ac.uk/~rgm/vhs/eso-p79b-vhs.pdf5 Oct 2006: If yes, explain why the need for new data. Are the data requested in this proposal on the ESO Archive (http://archive.eso.org)? -
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 -
ESO Public Surveys Proposal Form Phase 1 Title: The ...
https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v4p2-Appendix-B-PSP-Response.pdf9 Oct 2006: This required a total time of 7359hrs based on VISTA ETC(v1.1).With the new VISTA ETC(v1.3) this reduces to a total of 6750hrs. ... PSP Panel Issue 5 The Panel strongly recommends that the PI submits a new proposal whichfocused on the science that can be -
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 -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060628.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060628.txt18 Jul 2006: 6. WFCAM news (Non)linearity saga - this one could run for a long time. ... 7. VDFS news PSB reported that he had a productive visit to RAL and that he has returned with 270 files - all with full headers. -
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% -
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). -
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 -
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. -
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. -
THE ASTROPHYSICAL JOURNAL, 530 : 329È341, 2000 February 102000. ...
https://people.ast.cam.ac.uk/~wyatt/tfpk00.pdf19 Apr 2006: 1999). Here we present new 10.8 and 18.2 km images, obtainedat the Keck II telescope, of the HR 4796A debris disk. ... Our new images clarify the structure of the central clear-ing zone, or hole, which may be indirect evidence for aplanet orbiting HR -
SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...
https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf19 Apr 2006: All rights reserved. Printed in U.S.A. et al. 2004). Since the three newly resolved disks are around Gand M stars, these new images are filling in our understanding ofhow ... TheIRAS fluxes were determined from SCANPI (IRAS Scan Pro-cessing and -
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.
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