-
8
-
-
85035219649
-
-
appear in the Proceedings of PASCOS 1995 (World Scientific, Singapore
-
MACHO Collaboration, K. Griest, et al., to appear in the Proceedings of PASCOS 1995 (World Scientific, Singapore, 1995);
-
(1995)
K. Griest, et al.
-
-
-
10
-
-
85035222053
-
-
Report No. astro-ph/9512146, unpublished
-
C. Alcock, et al., Report No. astro-ph/9512146, 1995 (unpublished).
-
(1995)
-
-
Alcock, C.1
-
11
-
-
85035217961
-
-
private communication
-
C. Alcock (private communication).
-
-
-
Alcock, C.1
-
14
-
-
0027319141
-
-
Evidence for the existence of dark halos is discussed byV. Rubin, Proc. Natl. Acad. Sci. USA 90, 4814 (1993);
-
(1993)
Proc. Natl. Acad. Sci. USA
, vol.90
, pp. 4814
-
-
Rubin, V.1
-
29
-
-
85035198287
-
-
Report No. astro-ph/9509009, unpublished
-
A. Gould, Report No. astro-ph/9509009, 1995 (unpublished).
-
(1995)
-
-
Gould, A.1
-
31
-
-
85035214348
-
-
edited by H. Böhringer, G. Morfill, and J. Trümper (New York Academy of Sciences, New York
-
R. Ansari, et al., in Proceedings of the 17th Texas Symposium on Relativistic Astrophysics and Cosmology, edited by H. Böhringer, G. Morfill, and J. Trümper (New York Academy of Sciences, New York, 1995).
-
(1995)
Proceedings of the 17th Texas Symposium on Relativistic Astrophysics and Cosmology
-
-
Ansari, R.1
-
37
-
-
0009758052
-
-
F. De Paolis, G. Ingrosso, Ph. Jetzer and M. Ronadelli, Comments Astrophys. 18, 87 (1995).
-
(1995)
Comments Astrophys.
, vol.18
, pp. 87
-
-
De Paolis, F.1
Ingrosso, G.2
Jetzer, P.3
Ronadelli, M.4
-
40
-
-
0039820966
-
-
278, edited by S. S. Holt and F. Verter (AIP, New York
-
L. Blitz, in Back to the Galaxy, AIP Conf. Proc. 278, edited by S. S. Holt and F. Verter (AIP, New York, 1993), p. 98
-
(1993)
Back to the Galaxy, AIP Conf. Proc
, pp. 98
-
-
Blitz, L.1
-
42
-
-
85035228223
-
-
Report No. astro-ph/9508008, unpublished
-
K. Z. Stanek et al., Report No. astro-ph/9508008, 1995 (unpublished)
-
(1995)
-
-
Stanek, K.Z.1
-
43
-
-
85035217794
-
-
Report No. astro-ph/9508132, unpublished
-
K. Kuijken, Report No. astro-ph/9508132, 1995 (unpublished).
-
(1995)
-
-
Kuijken, K.1
-
47
-
-
11944266095
-
-
E. Dwek, et al., Astrophys. J. 445, 716 (1995).
-
(1995)
Astrophys. J.
, vol.445
, pp. 716
-
-
Dwek, E.1
-
53
-
-
85035191208
-
-
Taking a smaller value for (formula presented) would allow for larger (formula presented) and hence larger (formula presented
-
Taking a smaller value for (formula presented) would allow for larger (formula presented) and hence larger (formula presented);
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-
-
-
54
-
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85035245230
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however, taking (formula presented)=0 only increases (formula presented) by 0.3×(formula presented
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however, taking (formula presented)=0 only increases (formula presented) by 0.3×(formula presented).
-
-
-
-
55
-
-
85035208479
-
-
Omitted end note
-
Omitted end note.
-
-
-
-
58
-
-
12044249940
-
-
P. Sackett, H. Rix, B. J. Jarvis and K. C. Freeman, Astrophys. J. 436, 629 (1994).
-
(1994)
Astrophys. J.
, vol.436
, pp. 629
-
-
Sackett, P.1
Rix, H.2
Jarvis, B.J.3
Freeman, K.C.4
-
59
-
-
85035239777
-
-
See, e.g, edited by L. Blitz (Kluwer Academic
-
See, e.g., H. Rix, in Unsolved Problems of the Milky Way, IAU Symposium No. 169, edited by L. Blitz (Kluwer Academic, 1994).
-
(1994)
Unsolved Problems of the Milky Way, IAU Symposium No. 169
-
-
Rix, H.1
-
60
-
-
0000950958
-
-
C. S. Frenk, S. D. M. White, M. Davis and G. Efstathiou, Astrophys. J. 327, 507 (1988);
-
(1988)
Astrophys. J.
, vol.327
, pp. 507
-
-
Frenk, C.S.1
White, S.D.M.2
Davis, M.3
Efstathiou, G.4
-
65
-
-
85035199912
-
-
Omitted end note
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Omitted end note.
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-
-
-
67
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85035221641
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The range we adopt for (formula presented) is the 95% confidence range derived from the likelihood function based upon 3 events assuming Poisson statistics. However, the issue of uncertainties is far more complicated and the true 95% confidence range is probably larger
-
The range we adopt for (formula presented) is the 95% confidence range derived from the likelihood function based upon 3 events assuming Poisson statistics. However, the issue of uncertainties is far more complicated and the true 95% confidence range is probably larger;
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69
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85035222660
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For example, the measured optical depth (formula presented) =(π/4E)(formula presented), where the sum i runs over events, t-|(formula presented) is the duration of event i, and (formula presented) is the “efficiency” of detecting an event of duration t-|(formula presented). The MACHO efficiency drops significantly for t-|(formula presented)<10da and (formula presented) could be larger than reported due to short-duration events. However, because of the null results of the EROS CCD search for short-duration events and the MACHO spike analysis it seems unlikely that this is the case
-
For example, the measured optical depth (formula presented) =(π/4E)(formula presented), where the sum i runs over events, t-|(formula presented) is the duration of event i, and (formula presented) is the “efficiency” of detecting an event of duration t-|(formula presented). The MACHO efficiency drops significantly for t-|(formula presented)<10da and (formula presented) could be larger than reported due to short-duration events. However, because of the null results of the EROS CCD search for short-duration events and the MACHO spike analysis it seems unlikely that this is the case.
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81
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85035200482
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Backer, Unsolved Problems of the Milky Way, IAU Symposium No. 169, edited by L. Blitz (Kluwer Academic
-
Backer, Unsolved Problems of the Milky Way, IAU Symposium No. 169, edited by L. Blitz (Kluwer Academic, 1994).
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(1994)
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|