Abadie, J.et al. (LIGO and Virgo Collaborations) (2010a). Search for gravitational-wave inspiral signals associated with short gamma-ray bursts during LIGO's fifth and Virgo's first science run. ApJ, 715, 1453–1461.CrossRefGoogle Scholar

Abadie, J.et al. (LIGO and Virgo Collaborations) (2010b). All-sky search for gravitationalwave bursts in the first joint LIGO-GEO-Virgo run. Phys. Rev. D, 81, 102001.CrossRefGoogle Scholar

Abadie, J.et al. (2010c). Calibration of the LIGO gravitational wave detectors in the fifth science run. Nucl. Instrum. Methods Phys. Res. A, 624, 223–240.CrossRefGoogle Scholar

Abbasi, R. U.et al. (High Resolution Fly's Eye Collaboration) (2005). A study of the composition of ultra-high-energy cosmic rays using the High-Resolution Fly's Eye. ApJ, 622, 910–926.CrossRefGoogle Scholar

Abbasi, R. U.et al. (High Resolution Fly's Eye Collaboration (2008a). First observation of the Greisen-Zatsepin-Kuzmin suppression. Phys. Rev. Lett., 100, 101101.CrossRefGoogle ScholarPubMed

Abbasi, R. U.et al. (High Resolution Fly's Eye Collaboration (2008b). An upper limit on the electron-neutrino flux from the HiRes detector. ApJ, 684, 790–793.CrossRefGoogle Scholar

Abbasi, R. U.et al. (High Resolution Fly's Eye Collaboration) (2010a). Indications of proton-dominated cosmic-ray composition above 1.6 EeV. Phys. Rev. Lett., 104, 161101.Google ScholarPubMed

Abbasi, R. U.et al. (High Resolution Fly's Eye Collaboration) (2010b). Analysis of largescale anisotropy of ultra-high energy cosmic rays in HiRes data. ApJ, 713, L64–L68.CrossRefGoogle Scholar

Abbott, B.et al. (LIGO and TAMA Collaborations) (2005). Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts. Phys. Rev. D, 72, 122004.Google Scholar

Abdurashitov, J. N.et al. (1994). Results from SAGE (The Russian-American gallium solar neutrino experiment). Phys. Lett. B, 328, 234–248.CrossRefGoogle Scholar

Abraham, J.et al. (Pierre Auger Collaboration) (2008a). Observation of the suppression of the flux of cosmic rays above 4 × 1019eV. Phys. Rev. Lett., 101, 061101.CrossRefGoogle Scholar

Abraham, J.et al. (Pierre Auger Collaboration) (2008b). Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei. Astropart. Phys., 29, 188–204.CrossRefGoogle Scholar

Abraham, J.et al. (Pierre Auger Collaboration) (2010). Measurement of the depth of maximum of extensive air showers above 1018eV. Phys. Rev. Lett., 104, 091101.CrossRefGoogle Scholar

Abramowitz, M. & Stegun, I. A. (1970). Handbook of mathematical functions. Washington: National Bureau of Standards.Google Scholar

Accadia, T.et al. (2010). Status and perspectives of the Virgo gravitational wave detector. J. Phys. Conf. Ser., 203, 012074.CrossRefGoogle Scholar

Achterberg, A.et al. (IceCube Collaboration) (2006). First year performance of the IceCube neutrino telescope. Astropart. Phys., 26, 155–173.CrossRefGoogle Scholar

Achterberg, A.et al. (IceCube Collaboration) (2007). Detection of atmospheric muon neutrinos with the IceCube 9-string detector. Phys. Rev. D, 76, 027101.CrossRefGoogle Scholar

Agresti, J. (2008). Researches on non-standard optics for advanced gravitational wave interferometers. Ph.D. thesis, University of Pisa.

Aharmim, B.et al. (SNO Collaboration) (2005). Electron energy spectra, fluxes, and daynight asymmetries of 8B solar neutrinos from measurements with NaCl dissolved in the heavy-water detector at the Sudbury Neutrino Observatory. Phys. Rev. C, 72, 055502.CrossRefGoogle Scholar

Ahlen, S. P. (1980). Theoretical and experimental aspects of the energy loss of relativistic heavily ionizing particles. Rev. Mod. Phys., 52, 121–173.CrossRefGoogle Scholar

Ahmad, Q. R.et al. (SNO Collaboration) (2001). Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory. Phys. Rev. Lett., 87, 071301.CrossRefGoogle Scholar

Ahmed, S. N.et al. (SNO Collaboration) (2004). Measurement of the total active 8B solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity. Phys. Rev. Lett., 92, 181301.CrossRefGoogle ScholarPubMed

Ahn, H. S.et al. (CREAM Collaboration) (2007). The cosmic ray energetics and mass (CREAM) instrument. Nucl. Instrum. Methods Phys. Res. A, 579, 1034–1053.CrossRefGoogle Scholar

Ahrens, J.et al. (IceCube Collaboration) (2001). IceCube preliminary design document (revision 1.24; www.icecube.wisc.edu/science/publications/pdd/pdd.pdf).

Allen, C. W. (2001). Allen's astrophysical quantities, 4th edn., A. N., Cox, ed. New York: Springer.Google Scholar

Amblard, A., Cooray, A., & Kaplinghat, M. (2007). Search for gravitational waves in the CMB after WMAP3: foreground confusion and the optimal frequency coverage for foreground minimization. Phys. Rev. D, 75, 083508.CrossRefGoogle Scholar

Antonucci, R. (1993). Unified models for active galactic nuclei and quasars. ARA&A, 31, 473–521.CrossRefGoogle Scholar

Armstrong, J. W., Estabrook, F. B., & Tinto, M. (1999). Time-delay interferometry for space-based gravitational wave searches. ApJ, 527, 814–826.CrossRefGoogle Scholar

Arqueros, F., Hörandell, J. R., & Keilhauer, B. (2008). Air fluorescence relevant for cosmic-ray detection. Summary of the 5th fluorescence workshop, El Escorial, 2007. Nucl. Instrum. Methods Phys. Res. A, 597, 1–22.CrossRefGoogle Scholar

Ashie, Y.et al. (Super-Kamiokande Collaboration) (2005). Measurement of atmospheric neutrino oscillation parameters by Super-Kamiokande I. Phys. Rev. D, 71, 112005.CrossRefGoogle Scholar

The astronomical almanac for the year 2009 (2009). US Naval Observatory and HM Nautical Almanac Office (also http://asa.usno.navy.mil).

Bahcall, J. N., Pinsonneault, M. H., & Basu, S. (2001). Solar models: current epoch and time dependences, neutrinos, and helioseismological properties. ApJ, 555, 990–1012.CrossRefGoogle Scholar

Bahcall, J. N., Serenelli, A. M., & Basu, S. (2005). New solar opacities, abundances, helioseismology, and neutrino fluxes. ApJ, 621, L85–L88.CrossRefGoogle Scholar

Ballardin, G.et al. (2001). Measurement of the VIRGO superattenuator performance for seismic noise suppression. Rev. Sci. Instrum., 72, 3643–3652.CrossRefGoogle Scholar

Beatty, J. J. & Westerhoff, S. (2009). The highest-energy cosmic rays. Annu. Rev. Nucl. Part. Sci., 59, 319–345.CrossRefGoogle Scholar

Bennett, C. L.et al. (2003). The microwave anisotropy probe mission. ApJ, 583, 1–23.CrossRefGoogle Scholar

Bessell, M. S. & Brett, J. M. (1988). JHKLM photometry: standard systems, passbands, and intrinsic colors. PASP, 100, 1134–1151.CrossRefGoogle Scholar

Bessell, M. S., Castelli, F., & Plez, B. (1998). Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O-M stars. A&A, 333, 231–250.Google Scholar

Bevington, P. R. & Robinson, D. K. (2003). Data reduction and error analysis for the physical sciences, 3rd edn. New York: McGraw-Hill.Google Scholar

Bildsten, L. (1998). Gravitational radiation and rotation of accreting neutron stars. ApJ, 501, L89–L93.CrossRefGoogle Scholar

Blair, D. G., ed. (1991). The detection of gravitational waves. Cambridge: Cambridge University Press.CrossRefGoogle Scholar

Born, M. & Wolf, E. (1999). Principles of optics, 7th edn. Cambridge: Cambridge University Press.CrossRefGoogle Scholar

Boyer, J. H., Knapp, B. C., Mannel, E. J., & Seman, M. (2002). FADC-based DAQ for HiRes Fly's Eye. Nucl. Instrum. Methods Phys. Res. A, 482, 457–474.CrossRefGoogle Scholar

Braccini, S.et al. (WG2 Suspension group) (2009). Superattenuator seismic isolation measurements by Virgo interferometer: a comparison with the future generation antenna. Einstein Telescope scientific note ET-025-09.

Bracewell, R. N. (2000). The Fourier transform and its applications, 3rd edn. New York: McGraw-Hill.

Burke, B. E., Mountain, R.W., Harrison, D. C.et al. (1991). An abuttable CCD imager for visible and X-ray focal plane arrays. IEEE Trans. Electron Dev., 38, 1069–1076.CrossRefGoogle Scholar

Callen, H. & Welton, T. (1951). Irreversibility and generalized noise. Phys. Rev., 83, 34–40.CrossRefGoogle Scholar

Caves, C. M. (1980a). Quantum-mechanical radiation-pressure fluctuations in an interferometer. Phys. Rev. Lett., 45, 75–79.CrossRefGoogle Scholar

Caves, C. M., Thorne, K. S., Drever, R. W. P., Sandberg, V. D., & Zimmermann, M. (1980b). On the measurement of a weak classical force coupled to a quantummechanical oscillator. I. Issues of principle. Rev. Mod. Phys., 52, 341–392.CrossRefGoogle Scholar

Caves, C. M. (1981). Quantum-mechanical noise in an interferometer. Phys. Rev. D, 23, 1693–1708.CrossRefGoogle Scholar

Cesarsky, C. J. (1980). Cosmic-ray confinement in the galaxy. ARA&A, 18, 289–319.CrossRefGoogle Scholar

Chang, F.-Y., Chen, P., Lin, G.-L., Noble, R., & Sydora, R. (2009). Magnetowave induced plasma wakefield acceleration for ultrahigh energy cosmic rays. Phys. Rev. Lett., 102, 111101.CrossRefGoogle ScholarPubMed

Cherry, M. L., Hartmann, G., Müller, D., & Prince, T. A. (1974). Transition radiation from relativistic electrons in periodic radiators. Phys. Rev. D, 10, 3594–3607.CrossRefGoogle Scholar

Chiang, H. C.et al. (2010). Measurement of cosmic microwave background polarization power spectra from two years of BICEP data. ApJ, 711, 1123–1140.CrossRefGoogle Scholar

Cleveland, B. T.et al. (1998). Measurement of the solar electron neutrino flux with the Homestake chlorine detector. ApJ, 496, 505–526.CrossRefGoogle Scholar

Corbitt, T., Chen, Y., Khalili, F.et al. (2006). Squeezed-state source using radiationpressure-induced rigidity. Phys. Rev. A, 73, 023801.CrossRefGoogle Scholar

Cox, R. T. (1946). Probability, frequency, and reasonable expectation. Am. J. Phys., 14, 1–13.CrossRefGoogle Scholar

Crutcher, R. M., Troland, T. H., Goodman, A. A.et al. (1993). OH Zeeman observations of dark clouds. ApJ, 407, 175–184.CrossRefGoogle Scholar

Crutcher, R. M., Troland, T. H., Lazareff, B., Paubert, G., & Kazès, I. (1999). Detection of the CN Zeeman effect in molecular clouds. ApJ, 514, L121–L124.CrossRefGoogle Scholar

Cutler, C. & Thorne, K. S. (2002). An overview of gravitational-wave sources. In Proceedings of 16th international conference on general relativity and gravitation (GR16), N., Bishop & S. D., Maharaj, eds., 72–111, Singapore: World Scientific.CrossRefGoogle Scholar

Cuttaia, F.et al. (2004). Analysis of the pseudocorrelation radiometers for the low frequency instrument onboard the PLANCK satellite. Proc. SPIE, 5498, 756–767.CrossRefGoogle Scholar

Davis, L. Jr. & Greenstein, J. L. (1951). The polarization of starlight by aligned dust grains. ApJ, 114, 206–240.CrossRefGoogle Scholar

den Herder, J. W.et al. (2001). The reflection grating spectrometer on board XMM-Newton. A&A, 365, L7–L17.Google Scholar

Diaconis, P. & Efron, B. (1983). Computer-intensive methods in statistics. Sci. Am., 248, 116–130.CrossRefGoogle Scholar

Efron, B. (1981). Censored data and the bootstrap. J. Am. Stat. Assoc., 76, 312–319.CrossRefGoogle Scholar

ESA/NASA (2009a). Laser Interferometer Space Antenna (LISA) Mission Concept, LISA-PRJ-RP-0001.

ESA/NASA (2009b). Laser Interferometer Space Antenna (LISA) Measurement Requirements Flowdown Guide, LISA-MSE-TN-0001.

Esposito, J. A.et al. (1999). In-flight calibration of EGRET on the Compton gamma-ray observatory. ApJS, 123, 203–217.CrossRefGoogle Scholar

Estabrook, F. B. & Wahlquist, H. D. (1975). Response of Doppler spacecraft tracking to gravitational radiation. Gen. Relativ. Gravit., 6, 439–447.CrossRefGoogle Scholar

Estabrook, F. B., Tinto, M., & Armstrong, J.W. (2000). Time-delay analysis of LISA gravitational wave data: elimination of spacecraft motion effects. Phys. Rev. D, 62, 042002.CrossRefGoogle Scholar

Falta, D., Fisher, R., & Khanna, G. (2010). Gravitational wave emission from the singledegenerate channel of type Ia supernovae. arXiv:1011.6387v1.

Forward, R. L. (1978). Wideband laser-interferometer gravitational-radiation experiment. Phys. Rev. D, 17, 379–390.CrossRefGoogle Scholar

Fryer, C. & Kalogera, V. (1997). Double neutron star systems and natal neutron star kicks. ApJ, 489, 244–253.CrossRefGoogle Scholar

Fukuda, Y.et al. (1998). Evidence for oscillation of atmospheric neutrinos. Phys. Rev. Lett., 81, 1562–1567.CrossRefGoogle Scholar

Fukuda, S.et al. (2001). Solar 8B and hep neutrino measurements from 1258 days of Super-Kamiokande data. Phys. Rev. Lett., 86, 5651–5655.CrossRefGoogle ScholarPubMed

Gahbauer, F., Hermann, G., Hörandel, J. R., Müller, D., & Radu, A. A. (2004). A new measurement of the intensities of the heavy primary cosmic-ray nuclei around 1 TeV amu-1. ApJ, 607, 333–341.CrossRefGoogle Scholar

Gaisser, T. & Stanev, T. (2008). Cosmic rays. In Review of particle physics. Phys. Lett. B, 667, 254–260.Google Scholar

Gelman, A., Roberts, G. O., & Gilks, W. R. (1996). Efficient Metropolis jumping rules. In Bayesian statistics, Vol. 5, J., Bernardo, J., Berger, A., Dawid, & A., Smith, eds., 599–607, Oxford: Oxford University Press.Google Scholar

Gelman, A., Carlin, J. B., Stern, H. S., & Rubin, D. B. (2004). Bayesian data analysis, 2nd edn. Boca Raton: CRC Press.Google Scholar

Genzel, R. & Karas, V. (2007). The galactic center. Proc. Int. Astron. Union Symp., 238, 173–180.Google Scholar

Ghez, A. M., Klein, B. L., Morris, M., & Becklin, E. E. (1998). High proper-motion stars in the vicinity of Sagittarius A*: evidence for a supermassive black hole at the center of our galaxy. ApJ, 509, 678–686.CrossRefGoogle Scholar

Gillespie, A. & Raab, F. (1993). Thermal noise in the test mass suspensions of a laser interferometer gravitational-wave detector prototype. Phys. Lett. A, 178, 357–363.CrossRefGoogle Scholar

Ginzburg, V. L. & Tsytovich, V. N. (1979). Several problems of the theory of transition radiation and transition scattering. Phys. Rep., 49, 1–89.CrossRefGoogle Scholar

Giunti, C. & Kim, C. W. (2007). Fundamentals of neutrino physics and astrophysics. Oxford:Oxford University Press.CrossRefGoogle Scholar

Goda, K., Mikhailov, E. E., Miyakawa, O.et al. (2008). Generation of a stable low-frequency squeezed vacuum field with periodically poled KTiOPO4 at 1064 nm. Opt. Lett., 33, 92–94.CrossRefGoogle ScholarPubMed

Goldreich, R. & Kylafis, N. D. (1981). On mapping the magnetic field direction in molecular clouds by polarization measurements. ApJ, 243, L75–L78.CrossRefGoogle Scholar

Gorbunov, D. S., Tinyakov, P. G., Tkachev, I. I., & Troitsky, S. V. (2004). Testing the correlations between ultrahigh-energy cosmic rays and BL Lac-type objects with HiRes stereoscopic data. JETP Lett., 80, 145–148.CrossRefGoogle Scholar

Goßler, S.et al. (2003). Mode-cleaning and injection optics of the gravitational-wave detector GEO600. Rev. Sci. Instrum., 74, 3787–3795.CrossRefGoogle Scholar

Gradshteyn, I. S. & Ryzhik, I. M. (1980). Table of integrals, series, and products (corrrected and enlarged edition), A., Jeffrey, ed. New York: Academic Press.Google Scholar

Gross, E. P. (1955). Shape of collision-broadened spectral lines. Phys. Rev., 97, 395–403.CrossRefGoogle Scholar

Hamaker, J. P. & Bregman, J. D. (1996). Understanding radio polarimetry. III. Interpreting the IAU/IEEE definitions of the Stokes parameters. A&AS, 117, 161–165.Google Scholar

Hamaker, J. P., Bregman, J. D., & Sault, R. J. (1996). Understanding radio polarimetry. I. Mathematical foundations. A&AS, 117, 137–147.Google Scholar

Hamamatsu, Photonics (2006). Photomultiplier tubes: basics and applications, 3rd edn.

Hampel, W.et al.(GALLEX Collaboration) (1999). GALLEX solar neutrino observations: results for GALLEX IV. Phys. Lett. B, 447, 127–133.CrossRef

Hanbury Brown, R., Jennison, R. C., & Das Gupta, >M. K. (1952). Apparent angular sizes of discrete radio sources: observations at Jodrell Bank, Manchester. Nature, 170, 1061–1063.CrossRefGoogle Scholar

Hecht, E. (2002). Optics, 4th edn. Reading: Addison-Wesley.Google Scholar

Helstrom, C. W. (1991). Probability and stochastic processes for engineers, 2nd edn. New York: Macmillan.Google Scholar

Hild, S., Chelkowski, S., Freise, A.et al. (2010). A xylophone configuration for a third generation gravitational wave detector. Class. Quantum Grav., 27, 015003.CrossRef

Hillas, A. M. (1984). The origin of ultra-high-energy cosmic rays. ARA&A, 22, 425–444.CrossRefGoogle Scholar

Hillas, A. M. (1996). Differences between gamma-ray and hadronic showers. Space Sci. Rev., 75, 17–30.CrossRefGoogle Scholar

Hopkins, A. M. & Beacom, J. F. (2006). On the normalization of the cosmic star formation history. ApJ, 651, 142–154.CrossRefGoogle Scholar

Horiuchi, S., Beacom, J. F., & Dwek, E. (2009). Diffuse supernova neutrino background is detectable in Super-Kamiokande. Phys. Rev. D, 79, 083013.CrossRefGoogle Scholar

Hu, W. & White, M. (1997). CMB anisotropies: total angular momentum method. Phys. Rev. D, 56, 596–615.CrossRefGoogle Scholar

Hughes, S. A. (2001). Evolution of circular, nonequatorial orbits of Kerr black holes due to gravitational-wave emission. II. Inspiral trajectories and gravitational waveforms. Phys. Rev. D, 64, 064004.CrossRefGoogle Scholar

Hulse, R. A. & Taylor, J. H. (1975). Discovery of a pulsar in a binary system. ApJ, 195, L51–L53.CrossRefGoogle Scholar

IAU (1974). Polarization definitions (Commission 40). Trans. Int. Astron. Union, 15B, 166.

IEEE (1969). IEEE standard #211: definitions of terms for radio wave propagation. IEEE Trans. Antennas Propag., AP-17, 270–275.

In't Zand, J. J. M. (1992). A coded-mask imager as monitor of galactic X-ray sources. Ph.D. thesis, University of Utrecht.

Irwin, K. D. & Hilton, G. C. (2005). Transition-edge sensors. In Cryogenic particle detection, C., Enss, ed. Topics in Applied Physics, 99, 63–149, Berlin: Springer.Google Scholar

Jackson, J. D. (1998). Classical electrodynamics, 3rd edn. New York: Wiley.Google Scholar

Jahoda, K., Markwardt, C. B., Radeva, Yet al. (2006). Calibration of the Rossi x-ray timing explorer proportional counter array. ApJS, 163, 401–423.CrossRefGoogle Scholar

Jansen, R. A. (2006). Astronomy with charged coupled devices (e-book: www.public.asu.edu/∼rjansen/ast598/ast598_jansen2006.pdf).

Jansen, F., Lumb, D., Altieri, B.et al. (2001). XMM-Newton observatory. I. The spacecraft and operations. A&A, 365, L1–L6.Google Scholar

Johnson, H. L. (1966). Astronomical measurements in the infrared. ARA&A, 4, 193–206.CrossRefGoogle Scholar

Johnson, H. L. & Morgan, W. W. (1953). Fundamental stellar photometry for standards of spectral type on the revised system of the Yerkes spectral atlas. ApJ, 117, 313–352.CrossRefGoogle Scholar

Kitchin, C. R. (2009). Astrophysical techniques, 5th edn. Boca Raton: CRC Press.Google Scholar

Kliger, D. S., Lewis, J. W., & Randall, C. E. (1990). Polarized light in optics and spectroscopy. Boston: Academic Press.Google Scholar

Kuroda, K.et al.(LCGT Collaboration) (2010). Status of LCGT. Class. Quantum Grav., 27, 084004.

Lamarre, J. M.et al. (2003). The Planck high frequency instrument, a third generation CMB experiment, and a full sky submillimeter survey. New Astron. Rev., 47, 1017–1024.CrossRefGoogle Scholar

Larson, D.et al. (2011). Seven-year Wilkinson microwave anisotropy probe (WMAP) observations: power spectra and WMAP-derived parameters. ApJS, 192, 16.CrossRefGoogle Scholar

Lazarian, A. & Cho, J. (2005). Grain alignment in molecular clouds. In Astronomical polarimetry: current status and future directions, ASP Conference Series, 343 A. Adamson, C. Aspin, C. J. Davis, , & T., Fujiyoshi, eds. 333–345.

Lazarian, A., Goodman, A. A., & Myers, P. C. (1997). On the efficiency of grain alignment in dark clouds. ApJ, 490, 273–280.CrossRefGoogle Scholar

Lèna, P., Lebrun, F., & Mignard, F. (1998). Observational astrophysics, 2nd edn. Berlin: Springer.CrossRefGoogle Scholar

Loredo, T. J. (1992). Promise of Bayesian inference for astrophysics. In Statistical challenges in modern astronomy, E. D., Feigelson & G. J., Babu, eds., 275–306. New York: Springer-Verlag.CrossRefGoogle Scholar

Lyons, L. (1991). A practical guide to data analysis for physical science students. Cambridge: Cambridge University Press.CrossRefGoogle Scholar

MacKay, D. J. C. (2003). Information theory, inference, and learning algorithms. Cambridge: Cambridge University Press.Google Scholar

Mathews, J. (1962). Gravitational multipole radiation. J. Soc. Indust. Appl. Math., 10, 768–780.CrossRefGoogle Scholar

Mathews, J. & Walker, R. L. (1970). Mathematical methods of physics. Menlo Park: Benjamin.

Matthews, J. N. (2010). Overview of the high resolution fly's eye: some results from the HiRes experiment. In Proc. 2009 Snowbird particle astrophysics and cosmology workshop, ASP Conference Series, 426, D. B., Kieda & P., Gondolo, eds., 3–10.Google Scholar

McKenzie, K., Grosse, N., Bowen, W. P.et al. (2004). Squeezing in the audio gravitationalwave detection band. Phys. Rev. Lett., 93, 161105.

Meers, B. J. (1988). Recycling in laser-interferometric gravitational-wave detectors. Phys. Rev. D, 38, 2317–2326.CrossRefGoogle ScholarPubMed

Mie, G. (1908). Beiträge zur optik trüber medien, speziell kolloidaler Metallösungen. Ann. Physik, 330, 377–445.CrossRefGoogle Scholar

Misner, C. W., Thorne, K. S., & Wheeler, M. A. (1973). Gravitation. San Francisco:Freeman.Google Scholar

Nyquist, H. (1928). Thermal agitation of electric charge in conductors. Phys. Rev., 32, 110–113.CrossRefGoogle Scholar

Ogliore, R. (2007). The sulfur, argon, and calcium isotopic composition of the galactic cosmic ray source. Ph.D. thesis, Caltech.

Oke, J. B. (1964). Photoelectric spectrophotometry of stars suitable for standards. ApJ, 140, 689–693.CrossRefGoogle Scholar

Oppenheimer, B. R. & Hinkley, S. (2009). High-contrast observations in optical and infrared astronomy. ARA&A, 47, 253–289.CrossRefGoogle Scholar

Papoulis, A. (1991). Probability, random variables, and stochastic processes, 3rd edn. New York: McGraw-Hill.Google Scholar

Perryman, M. A. C.et al. (1997). The HIPPARCOS catalogue. A&A, 323, L49–L52.Google Scholar

Peters, P. C. & Mathews, J. (1963). Gravitational radiation from point masses in a Keplerian orbit. Phys. Rev., 131, 435–440.CrossRefGoogle Scholar

Press, W. H. (1997). Understanding data better with Bayesian and global statistical methods. In Unsolved problems in astrophysics, J. N., Bahcall & J. P., Ostriker, eds., pp. 49–60, Princeton: Princeton University Press.Google Scholar

Press, W. H., Teukolsky, S. A, Vetterling, W. T., & Flannery, B. P. (2007). Numerical recipes: the art of scientific computing, 3rd edn. Cambridge: Cambridge University Press.Google Scholar

Price, P. B. & Fleisher, R. L. (1971). Identification of energetic heavy nuclei with solid dielectric track detectors: applications to astrophysical and planetary studies. Annu. Rev. Nucl. Sci., 21, 295–334.CrossRefGoogle Scholar

Prior, G.(for SNO Collaboration) (2009). Results from the Sudbury Neutrino Observatory phase III. Nucl. Phys. B (Proc. Suppl.), 188, 96–100.CrossRef

Raffelt, G. (1996). Stars as laboratories for fundamental physics. Chicago: University of Chicago Press.Google Scholar

Ramsey, N. F. (1949). A new molecular beam resonance method. Phys. Rev., 76, 996.CrossRefGoogle Scholar

Reitz, J. R., Milford, F. J., & Christy, R.W. (1979). Foundations of electromagnetic theory, 3rd edn. Reading: Addison-Wesley.Google Scholar

Rieke, G. H. (2002). Detection of light: from the ultraviolet to the submillimeter, 2nd edn. Cambridge: Cambridge University Press.CrossRefGoogle Scholar

Roberts, G. O., Gelman, A., & Gilks, W. R. (1997). Weak convergence and optimal scaling of random walk Metropolis algorithms. Annu. Appl. Prob., 7, 110–120.Google Scholar

Röser, S. & Bastian, U., eds. (1991). PPM star catalogue. Heidelberg: Spektrum Akademischer Verlag.Google Scholar

Saikia, D. J. & Salter, C. J. (1988). Polarization properties of extragalactic radio sources. ARA&A, 26, 93–144.CrossRefGoogle Scholar

Sault, R. J.Hamaker, J. P., & Bregman, J. D. (1996). Understanding radio polarimetry. II. Instrumental calibration of an interferometer array. A&AS, 117, 149–159.Google Scholar

Schönfelder, V.et al. (1993). Instrument description and performance of the imaging gamma-ray telescope COMPTEL aboard the Compton gamma-ray observatory. ApJS, 86, 657–692.CrossRefGoogle Scholar

Schroeder, D. J. (2000). Astronomical optics, 2nd edn. San Diego: Academic Press.Google Scholar

Seidelmann, P. K. (2006). Explanatory supplement to the astronomical almanac, rev. edn. Mill Valley: University Science Books.Google Scholar

Sivia, D. S. (1996). Data analysis: a Bayesian tutorial. Oxford: Clarendon Press.Google Scholar

Soffitta, P.et al. (2003). Techniques and detectors for polarimetry in X-ray astronomy. Nucl. Instrum. Meth. A, 510, 170–175.CrossRefGoogle Scholar

Stone, E. C.et al. (1998). The solar isotope spectrometer for the Advanced Composition Explorer. Space Sci. Rev., 86, 357–408.CrossRefGoogle Scholar

Streetman, B. G. & Banerjee, S. K. (2005). Solid state electronic devices, 6th edn. Englewood Cliffs: Prentice Hall.Google Scholar

Strömgren, B. (1966). Spectral classification through photoelectric narrow-band photometry. ARA&A, 4, 433–472.CrossRefGoogle Scholar

Strüder, L., Briel, U., Dennerl, K.et al. (2001). The European photon imaging camera on XMM-Newton: the pn-CCD camera. A&A, 365, L18–L26.Google Scholar

Sutton, E. C. & Wandelt, B. D. (2006). Optimal image reconstruction in radio interferometry. ApJS, 162, 401–416.CrossRefGoogle Scholar

Sze, S. M. & Ng, K wok K. (2006). Physics of semiconductor devices, 3rd edn. Hoboken:Wiley.CrossRefGoogle Scholar

Tatarskii, V. I. (1971). The effects of the turbulent atmosphere on wave propagation. Jerusalem: Israel Program for Scientific Translations.Google Scholar

Thompson, A. R., Moran, J. M., & Swenson, G. W. (2001). Interferometry and synthesis in radio astronomy, 2nd edn. New York: Wiley.CrossRefGoogle Scholar

Thorne, K. S. (1987). Gravitational radiation. In Three hundred years of gravitation, S. W., Hawking & W., Israel, eds., 330–458. Cambridge: Cambridge University Press.Google Scholar

Timothy, J. G. (1983). Optical detectors for spectroscopy. PASP, 95, 810–834.CrossRefGoogle Scholar

Tinbergen, J. (1996). Astronomical polarimetry. Cambridge: Cambridge University Press.CrossRefGoogle Scholar

Tinto, M. & Armstrong, J. W. (1999). Cancellation of laser noise in an unequal-arm interferometer detector of gravitational radiation. Phys. Rev. D, 59, 102003.CrossRefGoogle Scholar

Tinto, M. & Dhurandhar, S. V. (2005). Time-delay interferometry. Living Rev. Relativity, 8, 4 (http://www.livingreviews.org/lrr-2005-4).

Tretyakov, M. Yu., Koshelev, M. A., Dorovskikh, V. V., Makarov, D. S., and Rosenkranz, P. W. (2005). 60-GHz oxygen band: precise broadening and central frequencies of fine-structure lines, absolute absorption profile at atmospheric pressure, and revision of mixing coefficients. J. Mol. Spectrosc., 231, 1–14.CrossRefGoogle Scholar

Turner, M. J. L., Abbey, A., Arnaud, M., et al. (2001). The European photon imaging camera on XMM-Newton: the MOS cameras. A&A, 365, L27–L35.Google Scholar

Vahlbruch, H., Khalaidovski, A., Lastzka, N.et al. (2010). The GEO 600 squeezed light source. Class. Quantum Grav. 27, 084027.CrossRefGoogle Scholar

Vallerga, J. V., Kaplan, G. C., Siegmund, O. H. W.et al. (1989). Imaging characteristics of the extreme ultraviolet explorer microchannel plate detectors. IEEE Trans. Nucl. Sci., 36, 881–886.CrossRefGoogle Scholar

van de Hulst, H. C. (1957). Light scattering by small particles. New York: Dover.Google Scholar

Virtue, C. J.(SNO Collaboration) (2001). SNO and supernovae. Nucl. Phys. B Proc. Suppl., 100, 326–331.CrossRef

Wakely, S. P. (2002). Precision x-ray transition radiation detection. Astropart. Phys., 18, 67–87.CrossRefGoogle Scholar

Wang, L. & Wheeler, J. C. (2008). Spectropolarimetry of supernovae. ARA&A, 46, 433–474.CrossRefGoogle Scholar

Weber, J. (1966). Observation of the thermal fluctuations of a gravitational-wave detector. Phys. Rev. Lett., 17, 1228–1230.CrossRefGoogle Scholar

Weisberg, J. M. & Taylor, J. H. (2005). The relativistic binary pulsar B1913+16: thirty years of observations and analysis. In Binary radio pulsars, ASP Conference Series, 328, F. A., Razio & I. H., Stairs, eds., 25–31.

Wilson, R. N. (1996). Reflecting telescope optics I. Berlin: Springer.CrossRefGoogle Scholar

Wilson, R. N. & Delabre, B. (1995). New optical solutions for very large telescopes using a spherical primary. A&A, 294, 322–338.Google Scholar

Wolf, E. (2007). Introduction to the theory of coherence and polarization of light. Cambridge: Cambridge University Press.Google Scholar

Zuber, K. (2004). Neutrino physics. Bristol: Institute of Physics Publishing.CrossRefGoogle Scholar