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Dark Exposure Properties of VIRCAM Detectors
https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_darkreport/vircam_darkreport.html21 Oct 2006: Figure 24 below shows this for detector 15 on the mean dark frame. ... Figure 24 A hot pixel cluster on a mean dark frame for detector 15. -
L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...
https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf19 Apr 2006: 24(40 AU) in ground-based, near-infrared, coronagraphic images.They estimated the disk position angle as , inclination50 1027 deg, and minimum dust mass 0.4 M. ... Trilling &2. Brown (1998) report an H-band disk surface brightness thatfalls below 24 mag -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7. -
CASU analysis of WFCAM commissioning data - I
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/index.html2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. -
{\bf WFCAM Catalogues}
https://people.ast.cam.ac.uk/~wfcam/docs/catalogues.html4 Feb 2006: 24 Aperture flux 3 Recommended if a single number is required to represent the flux for ALL. ... 24 arcsec diameter. 45 Error in flux The aperture fluxes can be combined with later-derived aperture. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt9 Aug 2006: 3. Report from VDMT MJI and STH attended the VDMT meeting in Edinburgh on 24 July. ... MJI reported on the main points: The UK review of VDFS will be held in Cambridge on 24/25 October. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060919.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060919.txt1 Oct 2006: JRL volunteered. MJI gave further details of the review. Planned Start 24 October Tuesday 10:30 End 25 October Wednesday 15:30 Lunch will be provided on both days and it ... APM3: We were reminded that the home disks of apm3 have now been united with -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt6 Nov 2006: The UK VDFS review was held on 24/25 October at Cambridge. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060105.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060105.txt9 Jan 2006: The last GANTT chart we have says 24 March, but it is unclear if this is the current target date. -
Flat Exposure Properties of VIRCAM Detectors
https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/vircam_flatreport.html8 Dec 2006: 1.32 /- 0.05. 0.53 /- 0.01. 8. 2.23 /- 0.24. 0.61 /- 0.03. ... figure 5.10 Detector 10 (0.10%). figure 5.11 Detector 11 (0.24%). figure 5.12 Detector 12 (0.22%). -
Placing Our Solar System in Context:[A 12 step program ...
https://people.ast.cam.ac.uk/~wyatt/mmeyer_etal_ppv.pdf19 Apr 2006: MIR.but more common around stars < 100 Myr. MIPS 24 um image of Vega disk. ... MIPS-24 MIPS-70. MIPS-160 JCMT-450CSO-350. HST. Do Stars with Inner Planets (< 5 AU) Also Have Kuiper Disks? -
..............................................................…
https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf19 Apr 2006: Corresponding peak. signal-to-noise ratios are 27, 48, 24 and 15, respectively. ... We used thestandard g Reticulum to determine the PSF at 24.6 mm. -
Pipeline CalibrationSimon Hodgkin(paper in prep) Outline • UKIRT…
https://people.ast.cam.ac.uk/~wfcam/talks/hodgkin_ukidss_jul06.pdf3 Aug 2006: The observations span 05A and 05B, and comprise around 21 obs for the P272 field, and 24 for the P545 field. -
mnr9848.tex
https://people.ast.cam.ac.uk/~wyatt/gfw05.pdf19 Apr 2006: This latter study is based on weak IRAS excesses,and four of the six systems identified with IRAS at 25 µm do nothave 24-µm excesses on re-examination by Spitzer -
mnr_7037.tex
https://people.ast.cam.ac.uk/~wyatt/gw03.pdf19 Apr 2006: G8V 1HD 18757 22.9 G4V 2 Wide binaryHD 19373 10.5 G0V 1HD 20407 24.4 G3V 1HD 20766 12.1 G2V 2,‘B’ Wide binary (secondary)HD 20807 ... 1 G1V 2 Wide binary (primary); IRAS discHD 20619 24.7 G5V 1HD 20630 9.2 G5V 1 YoungHD 20794 6.1 G8V 1 ISO discHD -
arX iv:a stro -ph/ 0504 086 v1 4 A ...
https://people.ast.cam.ac.uk/~wyatt/srms05.pdf19 Apr 2006: 6 Su et al. Fig. 9.— Radial dependent [24][70] distribution for the Vegadisk. ... To produce the observed [24][70]color, additional components must be invoked. 4.4. -
Modeling the Structures of Dusty Disks: UnseenPlanets? Mark C. ...
https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf19 Apr 2006: to the Sun, at about 23 AU, then migratedoutward to its current 30 AU orbit [24]. ... Sci., 27, 287–312 (1999).24. Malhotra, R., Astron. J., 110, 420–429 (1995).25. -
PDF/48/aa5873-06.pdf.url
https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf14 Dec 2006: 2 0.8 0.8 150 20 <1.9GJ 9809 M0 23 06 04.8 63 55 34 24.9 29.43 Loc Ass. ... 23 06 04.8 63 55 34 24.9 29.43 Loc Ass 0.5 7 0.36 2.2 2.2 7 26 <10. -
aa2073.dvi
https://people.ast.cam.ac.uk/~wyatt/wyat05b.pdf19 Apr 2006: A&A 433, 1007–1012 (2005)DOI: 10.1051/0004-6361:20042073c ESO 2005. Astronomy&. Astrophysics. The insignificance of P-R drag in detectableextrasolar planetesimal belts. M. C. Wyatt. UK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 -
NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE ...
https://people.ast.cam.ac.uk/~wyatt/bbsg06.pdf28 Nov 2006: a Significance of 24 m excess (eq. [1]).b Significance of 70 m excess (eq. ... 2000). Finally,HD 23249 and HD 55892 have 2 < 24 < 3 and 70 < 2. -
Dust_in_the_Debris_Disk_Around_HD69830_09Nov2006
https://people.ast.cam.ac.uk/~wyatt/lbbw07.pdf16 Nov 2006: 2.46 Diopside (CaMgSi2O6) 0.05 3.3 216 0.075 340 1.53 Carbonates Magnesite (MgCO3) 0.07 3.1 84 0.24 370 1.54 Dolomite (CaMgC2O6) d ... 12 and 25 um photometry (Mannings and Barlow 1998), and Spitzer 24 and 70 um photometry. -
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: ESO Public Surveys Proposal Form Phase 1. reaching 10sigma limits[AB mags] in g, r, i and z of 24.1, 23.7, 23.3 and 22.6 respectively. ... with 10sigma limit of 24.6, 24.1, 24.3 and 23.9. -
Evolution of Circumstellar Disks Around Normal Stars:Placing Our…
https://people.ast.cam.ac.uk/~wyatt/mbww07.pdf19 Apr 2006: Surprisingly, however, the 24 and 70 µm images of Vegaactually have larger radii than the submillimeter ring or mil-limeter clumps (Su et al., 2005). ... Emission (Additional)Vega A0 200 >90 23,24,25 Eridani K2 <1000 60 26,27η Corvi F2 1000 100 28τ -
SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...
https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf19 Apr 2006: The total measured flux was 1:51 0:24 Jy (S=N 7);the dominant uncertainty in this flux estimate is the calibrationuncertainty. -
��������� ��� ������������������� ������� ������� ��!�� #"$��…
https://people.ast.cam.ac.uk/~wyatt/wyat99.pdf19 Apr 2006: 2/)C"C$ )!1-N. 2#1 D 4'@! 24"BC #" 1 9 #"S243! S'@ #3<TU,3- #"D32#!24"24,! :<')("!-! ... $-"8 =H0,"80 N,'<Q ; 3j Y-. ) ,"8 2MP 24 3j ;2)! -
THE ASTROPHYSICAL JOURNAL, 530 : 329È341, 2000 February 102000. ...
https://people.ast.cam.ac.uk/~wyatt/tfpk00.pdf19 Apr 2006: d)Logarithmic 18.2 km levels : 8.0, 10.6, 13.9, 18.4, 24.3, 32.1, 42.3, 55.9, and 73.7. -
Submitted to ApJ 16 July 2006, Accepted 3 October ...
https://people.ast.cam.ac.uk/~wyatt/wsgb07.pdf2 Nov 2006: 0.5M2v2rel = M1Q? D whereas DD03 define S to be the specific bind-ing energy of the two objects (giving their equation 24). ... dNc(D > Dpb)/dt = 1000r13/3(dr/r)t2ageDcD. 3pb. M4/3? Q? D. 5/6e5/3, (24). -
arX iv:a stro -ph/ 0311 593 v1 26 N ...
https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf19 Apr 2006: 32 0.02 0.13 0.04 < 0.5HD207129 0.60 0.03 0.15 0.02 0.31 0.04 < 0.24. ... However, sub-mm observations made withSCUBA on the JCMT indicate a diameter of 24 3 arc-sec (Holland et al. -
58419 1321..1340
https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf19 Apr 2006: Crosses show the location of a planetesimal in the different resonances (2 : 1, 5 : 3, 3 : 2, and 4 : 3,from top to bottom) at intervals of 1/24 of the ... l1:24. e0:42. ; ð33Þ. D5 :3h i 13:2 þ 290:0=l1:33. ; ð34Þ. -
Oxford Meeting
https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt15 Apr 2006: B440022.122.24.82.6. V550021.321.49.63.5. R600020.420.817.93.9. I750019.520.035.25.2. Z890018.218.7117.26.3. J12,50016.016.9609.39.3. -
Mon. Not. R. Astron. Soc. 334, 589–607 (2002) Collisional ...
https://people.ast.cam.ac.uk/~wyatt/wd02.pdf19 Apr 2006: 25 1.24 0.6 IRAS60 9.80 0.62 IRAS60 7.51 0.92 ISO80 8.86 0.87 ISO100 10.95 0.66 IRAS100 11.04 2.0 ISO120 -
arX iv:a stro -ph/ 0601 592 v1 26 J ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/hewettetal.pdf28 Sep 2006: 4.162 2.130 5.626 2.349 -0.529 -0.117 -0.293 0.074 0.105 24.4 2 8.5 283 3.57. ... 4.190 0.301 2.457 1.409 -0.147 0.092 -0.288 0.074 0.132 14.6 10 8.0 859 4.24. -
THE ASTROPHYSICAL JOURNAL, 527 : 918È944, 1999 December 20The ...
https://people.ast.cam.ac.uk/~wyatt/wdtf99.pdf19 Apr 2006: e5pr. [(a/a2)2.5e/(1 [ e2)1@2 [2.5ae/a2 ] O(e2) , (24). where AU2 yr1. ... P-R draga 6.24 ] 104(M/M. _)b. does not change the plane of the particleÏs orbit, I0pr. -
arX iv:a stro -ph/ 0603 608 v2 1 Se ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/dye.pdf28 Sep 2006: 35 K multiple 20.8. J multiple 24.8UDS 0.77 H multiple 23.8. ... SFA 04:30,25:00 ZY JHK cen. 24. Orion SFA 05:29,02:36 ZY JHK cen. -
��������� �� ��� ������� ������������������������� � � �!� � ...
https://people.ast.cam.ac.uk/~wyatt/wdg03.pdf19 Apr 2006: FX 4V = $= ,d$4 o 24 V4 3 LB44 o -%3-[ 4-C T #"B4V-,d$4 EWVFX -- 44-,"ng$ #"B4V-,d$4E E@$dX 3 ,,3 3V o V234 4 LM,> o ... 3-[ 43 VT #"-_$3-_$ EWVFX ,- 34 #"-_$3-_$E 3FX =., 3 44 o 24 -% $= f 33 o 4-[ --C $FT #"%4 V EW= VFX ,,, 3=4"ng$ #"%4 VE 3FX -
VDF-WFA-VSA-004-I1.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-WFA-VSA-004-I1.pdf29 Sep 2006: MAGZPT = 24.16 / Photometric ZP (mags) for default extinction. MAGZRR = 0.01 / Photometric ZP error (mags). ... ELLIPTIC= 0.2457458 / Ellipticity estimate from IMCORE. MAGZPT = 24.16 / Photometric ZP (mags) for default extinction. -
VDFS UK VISTA User Requirements
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-SPE-IOA-00009-0001.pdf28 Sep 2006: 18 5 General Requirements.19 6 Astrometric Requirements. 24 7 Photometric Requirements.25 8 Tiling, Stacking, Microstepping. ... Date: 05/07/2005 Issue: 3.0 Page: Page 24 of 33 Author: W. -
Document Title: VISTA Infra Red Camera Calibration Plan Document ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0002.pdf28 Sep 2006: 22 4.4 Dome flats. 23 4.5 Detector Noise. 24 4.6 Linearization Measurements. ... 24 4.7 Twilight Flats. 25 4.8 Illumination Correction Measurement. 26 4.9 Image Persistence Measurements. -
Data Flow System Document Title: VISTA Data Reduction Library ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010.pdf28 Sep 2006: 0001, issue 3.2 2005-02-24. [RD 3] VISTA Science Requirements Document, VIS-SPE-VSC-00000-0001, issue. ... 13 / kk leads to a relative area of. )41()31).(1( 222 rkrkrk ′′′ (2-24).
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