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Changeset 4050 in Sophya
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- Feb 13, 2012, 7:44:48 PM (12 years ago)
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trunk/Cosmo/RadioBeam/sensfgnd21cm.tex (modified) (13 diffs)
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trunk/Cosmo/RadioBeam/sensfgnd21cm.tex
r4049 r4050 145 145 % aims heading (mandatory) 146 146 {We study the sensitivity of different radio interferometer configurations, or multi-beam 147 instruments for observing LSS and BAO oscillations in 21 cm, and we discuss the problem of foreground removal. } 147 instruments for observing LSS and baryon acoustic oscillations (BAO) in 21 cm, and we 148 discuss the problem of foreground removal. } 148 149 % methods heading (mandatory) 149 150 { For each configuration, we determined instrument response by computing the $(\uv)$ or Fourier angular frequency … … 184 185 Evidence of the acceleration in the expansion of the universe has 185 186 accumulated over the last twelve years, thanks to the observation of 186 distant supernovae and CMBanisotropies and to detailed analysis of the LSS.187 distant supernovae and cosmic microwave background (CMB) anisotropies and to detailed analysis of the LSS. 187 188 A cosmological constant ($\Lambda$) or new cosmological 188 189 energy density called {\em dark energy} has been advocated as the origin of this acceleration. … … 1841 1842 %%%% LSST Science book 1842 1843 \bibitem[Abell et al. 2009]{lsst.science} 1843 Abell, P.A. {\it et al.} {\it LSST Science book}, LSST Science Collaborations, {\it et al.} 2009,arXiv:0912.02011844 Abell, P.A. et al. 2009, LSST Science book, arXiv:0912.0201 1844 1845 1845 1846 %% reference SKA - BAO / DE en radio avec les sources … … 1847 1848 1848 1849 % reference DETF - DE eq.state parameter figure of merit 1849 \bibitem[Albrecht et al. 2006]{DETF} Albrecht, A., Bernstein, G., Cahn, R. {\it et al.} (Dark Energy Task Force), 2006, arXiv:astro-ph/0609591 1850 \bibitem[Albrecht et al. 2006]{DETF} Albrecht, A., Bernstein, G., Cahn, R. et al. 2006, 1851 (Dark Energy Task Force) arXiv:astro-ph/0609591 1850 1852 1851 1853 % Papier sensibilite/reconstruction CRT (cylindres) ansari et al 2008 … … 1861 1863 1862 1864 % WiggleZ BAO observation ( arXiv/1105.2862 ) 1863 \bibitem[Blake et al. 2011]{blake.11} Blake, Davis, T., Poole, G.B. {\it et al.} 2011, \mnras, 415, 2892-29091865 \bibitem[Blake et al. 2011]{blake.11} Blake, Davis, T., Poole, G.B. et al. 2011, \mnras, 415, 2892 1864 1866 1865 1867 % Galactic astronomy, emission HI d'une galaxie 1866 \bibitem[Binney \& Merrifield 1998]{binney.98} Binney J. \& Merrifield M. , 1998 {\it Galactic Astronomy} Princeton University Press1868 \bibitem[Binney \& Merrifield 1998]{binney.98} Binney J. \& Merrifield M. 1998, Galactic Astronomy (Princeton University Press) 1867 1869 % 21cm reionisation P(k) estimation and sensitivities 1868 \bibitem[Bowman et al. 2006]{bowman.06} Bowman, J.D., Morales, M.F., Hewitt, J.N. 2006, \apj, 638, 20 -261870 \bibitem[Bowman et al. 2006]{bowman.06} Bowman, J.D., Morales, M.F., Hewitt, J.N. 2006, \apj, 638, 20 1869 1871 % MWA description 1870 \bibitem[Bowman et al. 2007]{bowman.07} Bowman, J. D., Barnes, D.G., Briggs, F.H. {\it et al.} 2007, \aj, 133, 1505-15181872 \bibitem[Bowman et al. 2007]{bowman.07} Bowman, J. D., Barnes, D.G., Briggs, F.H. et al. 2007, \aj, 133, 1505 1871 1873 1872 1874 %% Soustraction avant plans ds MWA 1873 \bibitem[Bowman et al. (2009)]{bowman.09} Bowman, J. D., Morales, M., Hewitt, J.N., 2009, \apj, 695, 183 -1991875 \bibitem[Bowman et al. (2009)]{bowman.09} Bowman, J. D., Morales, M., Hewitt, J.N., 2009, \apj, 695, 183 1874 1876 1875 1877 %%% SKA-Science Elsevier, December 2004 http://www.skatelescope.org/pages/page\_sciencegen.htm 1876 1878 \bibitem[Carilli et al. 2004]{ska.science} 1877 {\it Science with the Square Kilometre Array}, eds: C. Carilli, S. Rawlings, 2004, New Astronomy Reviews, 481879 Science with the Square Kilometre Array, eds: C. Carilli, S. Rawlings, 2004, New Astronomy Reviews, 48 1878 1880 1879 1881 % Intensity mapping/HSHS … … 1881 1883 1882 1884 % Mesure 21 cm avec le GBT (papier Nature ) 1883 \bibitem[Chang et al. 2010]{chang.10} Chang T-C, Pen U-L, Bandura K., Peterson J.B., 2010, \nat, 466, 463 -4651885 \bibitem[Chang et al. 2010]{chang.10} Chang T-C, Pen U-L, Bandura K., Peterson J.B., 2010, \nat, 466, 463 1884 1886 1885 1887 % 2dFRS BAO observation 1886 \bibitem[Cole et al. 2005]{cole.05} Cole, S. Percival, W.J., Peacock, J.A. {\it et al.}2005, \mnras, 362, 5051888 \bibitem[Cole et al. 2005]{cole.05} Cole, S. Percival, W.J., Peacock, J.A. et al. 2005, \mnras, 362, 505 1887 1889 1888 1890 % NVSS radio source catalog : NRAO VLA Sky Survey (NVSS) is a 1.4 GHz … … 1891 1893 1892 1894 % Effet des radio-sources sur le signal 21 cm reionisation 1893 \bibitem[Di Matteo et al. 2002]{matteo.02} Di Matteo, T., Perna R., Abel T., Rees M.J. 2002, \apj, 564, 576 -5801895 \bibitem[Di Matteo et al. 2002]{matteo.02} Di Matteo, T., Perna R., Abel T., Rees M.J. 2002, \apj, 564, 576 1894 1896 1895 1897 % Parametrisation P(k) - (astro-ph/9709112) 1896 \bibitem[Eisenstein \& Hu 1998]{eisenhu.98} Eisenstein D. \& Hu W. 1998, \apj, 496, 605 -6141898 \bibitem[Eisenstein \& Hu 1998]{eisenhu.98} Eisenstein D. \& Hu W. 1998, \apj, 496, 605 1897 1899 1898 1900 % SDSS first BAO observation 1899 \bibitem[Eisenstein et al. 2005]{eisenstein.05} Eisenstein D. J., Zehavi, I., Hogg, D.W. {\it et al.}, (the SDSS Collaboration)2005, \apj, 633, 5601901 \bibitem[Eisenstein et al. 2005]{eisenstein.05} Eisenstein D. J., Zehavi, I., Hogg, D.W. et al. 2005, \apj, 633, 560 1900 1902 1901 1903 % SDSS-III description 1902 \bibitem[Eisenstein et al. 2011]{eisenstein.11} Eisenstein D. J., Weinberg, D.H., Agol, E. {\it et al.}, 2011, arXiv:1101.1529 \\1903 { \tt http://www.sdss3.org/ }1904 \bibitem[Eisenstein et al. 2011]{eisenstein.11} Eisenstein D. J., Weinberg, D.H., Agol, E. et al. 2011, arXiv:1101.1529 1905 % { \tt http://www.sdss3.org/ } 1904 1906 1905 1907 % Papier de Field sur la profondeur optique HI en 1959 1906 1908 \bibitem[Field 1959]{field.59} Field G.B., 1959, \apj, 129, 155 1907 1909 % 21 cm emission for mapping matter distribution 1908 \bibitem[Furlanetto et al. 2006]{furlanetto.06} Furlanetto, S., Peng Oh, S. \& Briggs, F. 2006, \physrep, 433, 181 -3011910 \bibitem[Furlanetto et al. 2006]{furlanetto.06} Furlanetto, S., Peng Oh, S. \& Briggs, F. 2006, \physrep, 433, 181 1909 1911 1910 1912 % Mesure 21 cm a 610 MHz par GMRT 1911 \bibitem[Ghosh et al. 2011]{ghosh.11} Ghosh A., Bharadwaj S., Ali Sk. S., Chengalur J. N., 2011, \mnras, 411, 2426 -24381913 \bibitem[Ghosh et al. 2011]{ghosh.11} Ghosh A., Bharadwaj S., Ali Sk. S., Chengalur J. N., 2011, \mnras, 411, 2426 1912 1914 1913 1915 … … 1921 1923 1922 1924 % WMAP 7 years cosmological parameters 1923 \bibitem[Komatsu et al. 2011]{komatsu.11} E. Komatsu, K. M. Smith, J. Dunkley {\it et al.} 2011, \apjs, 192, p.181925 \bibitem[Komatsu et al. 2011]{komatsu.11} E. Komatsu, K. M. Smith, J. Dunkley et al. 2011, \apjs, 192, 18 1924 1926 % \mbox{\tt http://lambda.gsfc.nasa.gov/product/map/current/params/lcdm\_sz\_lens\_wmap7.cfm} 1925 1927 1926 1928 % HI mass in galaxies 1927 \bibitem[Lah et al. 2009]{lah.09} Philip Lah, Michael B. Pracy, Jayaram N. Chengalur {\it et al.}2009, \mnras, 399, 14471929 \bibitem[Lah et al. 2009]{lah.09} Philip Lah, Michael B. Pracy, Jayaram N. Chengalur et al. 2009, \mnras, 399, 1447 1928 1930 % ( astro-ph/0907.1416) 1929 1931 1930 1932 % Livre Astrophysical Formulae de Lang 1931 \bibitem[Lang 1999]{astroformul} Lang, K.R. {\it Astrophysical Formulae}, Springer, 3rd Edition 19991933 \bibitem[Lang 1999]{astroformul} Lang, K.R. 1999, Astrophysical Formulae (Springer, 3rd Edition) 1932 1934 1933 1935 % WMAP CMB 7 years power spectrum 2011 1934 1936 % \bibitem[Hinshaw et al. (2008)]{hinshaw.08} Hinshaw, G., Weiland, J.L., Hill, R.S. {\it et al.} 2008, arXiv:0803.0732) 1935 \bibitem[Larson et al. 2011]{larson.11} Larson, D. , {\it et al.} (WMAP) 2011,\apjs, 192, 161937 \bibitem[Larson et al. 2011]{larson.11} Larson, D. et al. 2011, (WMAP) \apjs, 192, 16 1936 1938 1937 1939 %% Description MWA 1938 \bibitem[Lonsdale et al. 2009]{lonsdale.09} Lonsdale C.J., Cappallo R.J., Morales M.F. {\it et al.},2009,1939 IEEE Proceeding, 97, 1497 -1506(arXiv:0903.1828)1940 \bibitem[Lonsdale et al. 2009]{lonsdale.09} Lonsdale C.J., Cappallo R.J., Morales M.F. et al. 2009, 1941 IEEE Proceeding, 97, 1497 (arXiv:0903.1828) 1940 1942 1941 1943 % Planck Fischer matrix, computed for EUCLID … … 1943 1945 1944 1946 % Temperature du 21 cm 1945 \bibitem[Madau et al. 1997]{madau.97} Madau, P., Meiksin, A. and Rees, M.J., 1997, \apj 475, 4291947 \bibitem[Madau et al. 1997]{madau.97} Madau, P., Meiksin, A. and Rees, M.J., 1997, \apj, 475, 429 1946 1948 1947 1949 % Foret Ly alpha - 1 1948 \bibitem[McDonald et al. 2006]{baolya} McDonald P., Seljak, U. and Burles, S. {\it et al.}2006, \apjs, 163, 801950 \bibitem[McDonald et al. 2006]{baolya} McDonald P., Seljak, U. and Burles, S. et al. 2006, \apjs, 163, 80 1949 1951 1950 1952 % Foret Ly alpha - 2 , BAO from Ly-a … … 1952 1954 1953 1955 % Boomerang 2000, Acoustic pics 1954 \bibitem[Mauskopf et al. 2000]{mauskopf.00} Mauskopf, P. D., Ade, P. A. R., de Bernardis, P. {\it et al.} 2000, \apjl, 536, 591956 \bibitem[Mauskopf et al. 2000]{mauskopf.00} Mauskopf, P. D., Ade, P. A. R., de Bernardis, P. {\it et al.} 2000, \apjl, 536, 59 1955 1957 1956 1958 %% PNoise and cosmological parameters with reionization 1957 1959 \bibitem[McQuinn et al. 2006]{mcquinn.06} McQuinn M., Zahn O., Zaldarriaga M., Hernquist L., Furlanetto S.R. 1958 2006, \apj, 653, 815 -8341960 2006, \apj, 653, 815 1959 1961 1960 1962 % Papier sur la mesure de sensibilite P(k)_reionisation 1961 \bibitem[Morales \& Hewitt 2004]{morales.04} Morales M. \& Hewitt J., 2004, \apj, 615, 7 -181963 \bibitem[Morales \& Hewitt 2004]{morales.04} Morales M. \& Hewitt J., 2004, \apj, 615, 7 1962 1964 1963 1965 % Papier sur le traitement des observations radio / mode mixing 1964 \bibitem[Morales et al. (2006)]{morales.06} Morales, M., Bowman, J.D., Hewitt, J.N., 2006, \apj, 648, 767 -7731966 \bibitem[Morales et al. (2006)]{morales.06} Morales, M., Bowman, J.D., Hewitt, J.N., 2006, \apj, 648, 767 1965 1967 1966 1968 %% Foreground removal using smooth frequency dependence … … 1968 1970 1969 1971 % Global Sky Model Paper 1970 \bibitem[Oliveira-Costa et al. 2008]{gsm.08} de Oliveira-Costa, A., Tegmark, M., Gaensler, B.~M. {\it et al.}2008,1971 \mnras, 388, 247 -2601972 \bibitem[Oliveira-Costa et al. 2008]{gsm.08} de Oliveira-Costa, A., Tegmark, M., Gaensler, B.~M. et al. 2008, 1973 \mnras, 388, 247 1972 1974 1973 1975 %% Description+ resultats PAPER - arXiv:0904.2334 1974 \bibitem[Parsons et al. 2010]{parsons.10} Parsons A.R.,Backer D.C.,Bradley R.F. {\it et al.} 2010, 1975 \aj, 2010, 139, 1468-1480 1976 \bibitem[Parsons et al. 2010]{parsons.10} Parsons A.R.,Backer D.C.,Bradley R.F. et al. 2010, \aj, 139, 1468 1976 1977 1977 1978 % Livre Cosmo de Peebles 1978 \bibitem[Peebles 1993]{cosmo.peebles} Peebles, P.J.E., {\it Principles of Physical Cosmology},1979 Princeton University Press, 1993 1979 \bibitem[Peebles 1993]{cosmo.peebles} Peebles, P.J.E., 1993, Principles of Physical Cosmology, 1980 (Princeton University Press) 1980 1981 1981 1982 % Original CRT HSHS paper (Moriond Cosmo 2006 Proceedings) … … 1983 1984 1984 1985 % Synchrotron index =-2.8 in the freq range 1.4-7.5 GHz 1985 \bibitem[Platania et al. 1998]{platania.98} Platania P., Bensadoun M., Bersanelli M. {\it al.} 1998, \apj, 505, 473-4831986 \bibitem[Platania et al. 1998]{platania.98} Platania P., Bensadoun M., Bersanelli M. et al. 1998, \apj, 505, 473 1986 1987 1987 1988 % SDSS BAO 2007 1988 \bibitem[Percival et al. 2007]{percival.07} Percival, W.J., Nichol, R.C., Eisenstein, D.J. {\it et al.}, 2007, \apj,657, 6451989 \bibitem[Percival et al. 2007]{percival.07} Percival, W.J., Nichol, R.C., Eisenstein, D.J. et al. 2007, \apj, 657, 645 1989 1990 1990 1991 % SDSS BAO 2010 - arXiv:0907.1660 1991 \bibitem[Percival et al. 2010]{percival.10} Percival, W.J., Reid, B.A., Eisenstein, D.J. {\it et al.}, 2010, \mnras, 401, 2148-21681992 \bibitem[Percival et al. 2010]{percival.10} Percival, W.J., Reid, B.A., Eisenstein, D.J. et al. 2010, \mnras, 401, 2148 1992 1993 1993 1994 % Livre Cosmo de Jim Rich 1994 \bibitem[Rich 2001]{cosmo.rich} James Rich, {\it Fundamentals of Cosmology}, Springer, 20011995 \bibitem[Rich 2001]{cosmo.rich} James Rich, 2001, Fundamentals of Cosmology (Springer) 1995 1996 1996 1997 % Radio spectral index between 100-200 MHz 1997 \bibitem[Rogers \& Bowman 2008]{rogers.08} Rogers, A.E.E. \& Bowman, J. D. 2008, \aj 136, 641 -6481998 \bibitem[Rogers \& Bowman 2008]{rogers.08} Rogers, A.E.E. \& Bowman, J. D. 2008, \aj 136, 641 1998 1999 1999 2000 %% LOFAR description 2000 \bibitem[Rottering et al. 2006]{rottgering.06} Rottgering H.J.A., Braun, r., Barthel, P.D. {\it et al.}2006, arXiv:astro-ph/06105962001 \bibitem[Rottering et al. 2006]{rottgering.06} Rottgering H.J.A., Braun, r., Barthel, P.D. et al. 2006, arXiv:astro-ph/0610596 2001 2002 %%%% 2002 2003 … … 2005 2006 2006 2007 % Reionisation: Can the reionization epoch be detected as a global signature in the cosmic background? 2007 \bibitem[Shaver et al. 1999]{shaver.99} Shaver P.A., Windhorst R. A., Madau P., de Bruyn A.G. \aap, 345, 380 -3902008 \bibitem[Shaver et al. 1999]{shaver.99} Shaver P.A., Windhorst R. A., Madau P., de Bruyn A.G. \aap, 345, 380 2008 2009 2009 2010 % Frank H. Briggs, Matthew Colless, Roberto De Propris, Shaun Ferris, Brian P. Schmidt, Bradley E. Tucker 2010 2011 2011 2012 % Papier 21cm-BAO Fermilab ( arXiv:0910.5007) 2012 \bibitem[Seo et al 2010]{seo.10} Seo, H.J. Dodelson, S., Marriner, J. {\it et al.} 2010, \apj, 721, 164-1732013 \bibitem[Seo et al 2010]{seo.10} Seo, H.J. Dodelson, S., Marriner, J. et al. 2010, \apj, 721, 164 2013 2014 2014 2015 % Mesure P(k) par SDSS 2015 \bibitem[Tegmark et al. 2004]{tegmark.04} Tegmark M., Blanton M.R, Strauss M.A. {\it et al.} 2004, \apj, 606, 702-7402016 2017 % FFT telescope 2018 \bibitem[Tegmark \& Zaldarriaga 2009]{tegmark.09} Tegmark, M. \& Zaldarriaga, M., 2009, \prd, 79, 8, p. 083530 % arXiv:0802.17102016 \bibitem[Tegmark et al. 2004]{tegmark.04} Tegmark M., Blanton M.R, Strauss M.A. et al. 2004, \apj, 606, 702 2017 2018 % FFT telescope % arXiv:0802.1710 2019 \bibitem[Tegmark \& Zaldarriaga 2009]{tegmark.09} Tegmark, M. \& Zaldarriaga, M., 2009, \prd, 79, 8, 083530 2019 2020 2020 2021 % Thomson-Morane livre interferometry 2021 \bibitem[Thompson, Moran \& Swenson (2001)]{radastron} Thompson, A.R., Moran, J.M., Swenson, G.W, {\itInterferometry and2022 Synthesis in Radio Astronomy }, John Wiley \& sons, 2nd Edition 20012022 \bibitem[Thompson, Moran \& Swenson (2001)]{radastron} Thompson, A.R., Moran, J.M., Swenson, 2001, G.W, Interferometry and 2023 Synthesis in Radio Astronomy (John Wiley \& sons, 2nd Edition) 2023 2024 2024 2025 % Lyman-alpha, HI fraction 2025 2026 \bibitem[Wolf et al. 2005]{wolf.05} Wolfe, A. M., Gawiser, E. \& Prochaska, J.X. 2005 \araa, 43, 861 2026 2027 2027 % BAO à 21 cm et reionisation 2028 \bibitem[Wyithe et al. 2008]{wyithe.08} Wyithe, S., Loeb, A. \& Geil, P. 2008, \mnras, 383, 1195 % http://fr.arxiv.org/abs/0709.2955,2028 % BAO à 21 cm et reionisation % http://fr.arxiv.org/abs/0709.2955, 2029 \bibitem[Wyithe et al. 2008]{wyithe.08} Wyithe, S., Loeb, A. \& Geil, P. 2008, \mnras, 383, 1195 2029 2030 2030 2031 %% Papier fluctuations 21 cm par Zaldarriaga et al 2031 \bibitem[Zaldarriaga et al. 2004]{zaldarriaga.04} Zaldarriaga, M., Furlanetto, S.R., Hernquist, L., 2004, 2032 \apj, 608, 622-635 2032 \bibitem[Zaldarriaga et al. 2004]{zaldarriaga.04} Zaldarriaga, M., Furlanetto, S.R., Hernquist, L., 2004, \apj, 608, 622 2033 2033 2034 2034 %% Today HI cosmological density
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