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PSF Fitting of WFCAM Data: Tests on realdata Document ...
https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/psf3.pdf17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in yamounting to 0.05 pixel (20 mas) over the observed magnitude range. -
CASU analysis of WFCAM commissioning data - I
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/index.html2 Nov 2006: The above plots are all in the WFCAM instrumental system and the 5-sigma limiting magnitudes for stellar objects in this data in this system are approximately Y = 20.9, J = ... 20.6, H = 19.8, K = 19.1 ,all in a Vega system. -
Modeling the Structures of Dusty Disks: UnseenPlanets? Mark C. ...
https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf19 Apr 2006: Consideration of the collisional lifetime of different sizedbodies in the disk showed that what we are seeing is just the bottom half of the cascade(7 µ m dust to 20 ... C., and Taidakova, T. A., Astrophys. J., 537, L147–L151. (2000).20. Macintosh, B. -
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https://people.ast.cam.ac.uk/~wyatt/wdgj99.pdf19 Apr 2006: 0. 20. 40. Ecl. ipti. c L. atit. ude. 70 80 90 100 110Ecliptic Longitude Relative to Sun. ... 40. -20. 0. 20. 40. 70 80 90 100 110Ecliptic Longitude Relative to Sun. -
Dust_in_the_Debris_Disk_Around_HD69830_09Nov2006
https://people.ast.cam.ac.uk/~wyatt/lbbw07.pdf16 Nov 2006: predominantly Mg-rich olivines (80%) and crystalline pyroxenes (20%) (Figure 3). Unlike our. ... Dark blues - crystalline olivines, forsterite and fayalite, in order of 20 µm amplitude. -
SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...
https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf19 Apr 2006: areconsistent with a ring of radius 150 20 AU seen at 45 25 inclination. ... would migrate from 150to 0 AU (where it would evaporate) on timescales of 20 Myr(Burns et al. -
mnr_7037.tex
https://people.ast.cam.ac.uk/~wyatt/gw03.pdf19 Apr 2006: and Spangler et al. (2000) are also included here – ISO observed 70per cent of the single A stars but only 20 per cent of single G starswithin 25 pc. ... If the r 3 line in Fig. 2 is extrapolatedfrom 20 to 25 pc, the detections should increase to 20 -
PDF/48/aa5873-06.pdf.url
https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf14 Dec 2006: 2004).These two stars are 10–20 Myr old (see Favata et al. ... 1 AU) while (sub)mm surveys probe cold dust (20 K)distant from the star (100’s AU). -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v3p0.pdf6 Jun 2006: The proposed VHS survey will have a 10σ limit in Y of 20.4[Vega]; see Table 1. ... UKIDSS LAS uses SDSS z’ with a median 5σ limit(Vega) of 20.3. -
Calibration of WFCAM data from 2MASS: an investiga-tion and ...
https://people.ast.cam.ac.uk/~wfcam/docs/reports/2masscal_old.pdf6 Jan 2006: We analyse photometry of the UKIRT faint standardsmeasured on 20 photometric nights.
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