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https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt
https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt3 Jun 2011: 200.76777495 3.7214707 25.29 24.61 23.14 23.00 19.97 4 140.21862225 30.4611002 23.07 23.08 22.58 20.84 19.00 5 ... 85138 51.536387 24.02 23.72 23.09 21.47 20.74. -
CASU WFCAM/VISTA Documentation
https://people.ast.cam.ac.uk/~wfcam/documentation.html1 Mar 2011: 23-10-2002. 24-01-2003 [ps]. ... Pipeline document (old version submitted to CDR). 23-10-2002. 24-01-2003 [ps]. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt19 Dec 2011: September data was released to PIs and WFAU earlier this week and the first grumbles, in this case about 2 missing tiles arrived within 24 hours. -
Astroparticle_15
https://people.ast.cam.ac.uk/~gpe/Astroparticle_15.pdf25 Mar 2011: 103( )4 = 10. 24 GeV -2. R = 1012 GeV -1 = 2 "10#4 m. ... SM fields are confined to. brane! 3/21/11! Astroparticle! 24! Standard Model fields on branes! -
The problem with neutrinos… Neutrino oscillation data has ...
https://people.ast.cam.ac.uk/~gpe/Astroparticle_13.pdf25 Mar 2011: 2/22/10 Astroparticle 24. Torsion balance method? • Use two materials with same density but different neutrino scattering cross-sections, suspended from SC magnetic bearing. -
arX iv:1 102. 4341 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/kwg11.pdf23 Feb 2011: Also plotted are the detection limits at both 24 and70µm, given by Eq. ... Older disks must therefore have larger radii tobe detected at both 24 and 70µm. -
Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...
https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf5 Jul 2011: The MICHELLE fieldof view is 32”24”, but the chop throw of 15” limits the usableregion. ... The MIPS 24 µm image is shownin the first panel of Figure 3. -
arX iv:s ubm it/03 5390 2 [ astr o-ph ...
https://people.ast.cam.ac.uk/~wyatt/bw11.pdf8 Nov 2011: arX. iv:s. ubm. it/03. 5390. 2 [. astr. o-ph. EP]. 8 N. ov 2. 011. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 8 November 2011 (MN LATEX style file v2.2). The scattering of small bodies in planetary systems:. constraints on the possible -
Noname manuscript No.(will be inserted by the editor) DEBRIS ...
https://people.ast.cam.ac.uk/~wyatt/wcb11.pdf28 Mar 2011: αa = (7 a/3)/(2 a/3), (24). in the strength regime and αb = α given by equation (14) in the gravity regime. -
arX iv:1 107. 1239 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/vwmb11.pdf16 Nov 2011: 0 values of fbif if Ψbif < Ψbif,fmin (24). 1 value of fbif if Ψbif = Ψbif,fmin (25). ... fbif which satisfy Eq. (22). Figure 6 demonstrates Eqs.(24)-(26) graphically by plotting Ψbif vs. -
arX iv:1 104. 0007 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/ramb11.pdf5 Apr 2011: 2009; Carpenter et al. 2009). A stars havea significantly higher fraction of dust excesses at both 24 and70µm and the excesses themselves are brighter than for FGKstars but the dust lifetime ... These values are broadly consistentwith the fluxes
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