-
4
-
-
85038317980
-
-
P. Bender et al., LISA Pre-Phase: A Report, 2nd ed., 1998
-
P. Bender et al., LISA Pre-Phase: A Report, 2nd ed., 1998.
-
-
-
-
6
-
-
85038279654
-
-
For details regarding the proposed science for the SIM mission, see Science with the Space Interferometry Mission, edited by S. Unwin and S. Turyshev, 2002; available from the SIM website, http://sim.jpl.nasa.gov/
-
For details regarding the proposed science for the SIM mission, see Science with the Space Interferometry Mission, edited by S. Unwin and S. Turyshev, 2002; available from the SIM website, http://sim.jpl.nasa.gov/.
-
-
-
-
8
-
-
85038267382
-
-
Unless otherwise noted, geometric units where (Formula presented) are used throughout
-
Unless otherwise noted, geometric units where (Formula presented) are used throughout.
-
-
-
-
11
-
-
85038335094
-
-
Note that this value for (Formula presented) is specified for the 1 way position noise budget, as is the expression in Eq. (10), and has many constituent noises. Often, pure shot noise is considered as the limiting source of noise for the LISA floor; in that case, Eq. (10) should be replaced by Eq. (13) of Ref. 10
-
Note that this value for (Formula presented) is specified for the 1 way position noise budget, as is the expression in Eq. (10), and has many constituent noises. Often, pure shot noise is considered as the limiting source of noise for the LISA floor; in that case, Eq. (10) should be replaced by Eq. (13) of Ref. 10.
-
-
-
-
12
-
-
85038271313
-
-
The low frequency approximation is adequate for our purposes here. If one uses the full sensitivity curve (available at http://www.srl.caltech.edu/(Formula presented)shane/sensitivity/) instead, the results obtained differ only insubstantially
-
The low frequency approximation is adequate for our purposes here. If one uses the full sensitivity curve (available at http://www.srl.caltech.edu/(Formula presented)shane/sensitivity/) instead, the results obtained differ only insubstantially.
-
-
-
-
14
-
-
21744454818
-
-
S.F. Anderson, B. Margon, E.W. Deutsch, R.A. Downes, and R.G. Allen, Astrophys. J. Lett. 482, L69 (1997).
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Astrophys. J. Lett.
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Anderson, S.F.1
Margon, B.2
Deutsch, E.W.3
Downes, R.A.4
Allen, R.G.5
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17
-
-
85038307309
-
-
astro-ph/0111358
-
K. Wu et al., astro-ph/0111358.
-
-
-
Wu, K.1
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18
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-
85038321494
-
-
G.L. Israel, W. Hummel, S. Covino, S. Campana, I. Appenzeller, W. Gässler, K.-H. Mantel, G. Marconi, C.W. Mauche, U. Munari, I. Negueruela, H. Nicklas, G. Rupprecht, R.L. Smart, O. Stahl, and L. Stella, astro-ph/0203043
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G.L. Israel, W. Hummel, S. Covino, S. Campana, I. Appenzeller, W. Gässler, K.-H. Mantel, G. Marconi, C.W. Mauche, U. Munari, I. Negueruela, H. Nicklas, G. Rupprecht, R.L. Smart, O. Stahl, and L. Stella, astro-ph/0203043.
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19
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85038343036
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-
astro-ph/0104388
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D.R. Lorimer, astro-ph/0104388.
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-
-
Lorimer, D.R.1
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20
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-
85038302521
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-
astro-ph/0005214
-
V.M. Kaspi, astro-ph/0005214.
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Kaspi, V.M.1
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22
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85038292022
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astro-ph/0111231
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S. Jouteux, R. Ramachandran, B.W. Stappers, P.G. Jonker, and M. van der Klis, astro-ph/0111231.
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Jouteux, S.1
Ramachandran, R.2
Stappers, B.W.3
Jonker, P.G.4
van der Klis, M.5
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24
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0035837719
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M.T. Ruiz, P.M. Rojo, G. Garay, and J. Maza, Astrophys. J. 552, 679 (2001).
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(2001)
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, pp. 679
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Ruiz, M.T.1
Rojo, P.M.2
Garay, G.3
Maza, J.4
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