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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.
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