Built on

J. Asorey, M. Crocce, E. Gaztanaga, and A. Lewis, Recovering 3D clustering information with angular correlations
Original
1902
Earlier work this paper cites.
P. J. E. Peebles, Statistical Analysis of Catalogs of Extragalactic Objects. I. Theory
1973
Earlier work this paper cites.
N. Kaiser, Clustering in real space and in redshift space
1987
Earlier work this paper cites.
J. R. Bond, S. Cole, G. Efstathiou, and N. Kaiser, Excursion set mass functions for hierarchical Gaussian fluctuations
1991
Earlier work this paper cites.
F. Bernardeau, The nonlinear evolution of rare events
1994
Earlier work this paper cites.
L. Knox, Determination of inflationary observables by cosmic microwave background anisotropy experiments
1995
Earlier work this paper cites.
M. Tegmark and G. Efstathiou, A method for subtracting foregrounds from multifrequency CMB sky maps
1996
Earlier work this paper cites.
J. R. Bond, A. H. Jaffe, and L. Knox, Estimating the Power Spectrum of the Cosmic Microwave Background
1998
Earlier work this paper cites.
R. K. Sheth and G. Lemson, Biasing and the distribution of dark matter haloes
1999
Earlier work this paper cites.
S. M. Rao and D. A. Turnshek, Discovery of DampedLy α \alpha Systems at Redshifts Less than 1.65 and Results on Their Incidence and Cosmological Mass Density
2000
Earlier work this paper cites.
I. Szapudi, S. Prunet, and S. Colombi, Fast Analysis of Inhomogenous Megapixel Cosmic Microwave Background Maps
2001
Earlier work this paper cites.
M. Tegmark and A. de Oliveira-Costa, How to measure CMB power spectra without losing information
2001
Earlier work this paper cites.
I. Szapudi, S. Prunet, D. Pogosyan, A. S. Szalay, and J. R. Bond, Fast Cosmic Microwave Background Analyses via Correlation Functions
2001
Earlier work this paper cites.
V. Springel, N. Yoshida, and S. D. M. White, GADGET: a code for collisionless and gasdynamical cosmological simulations
2001
Earlier work this paper cites.
R. K. Sheth and G. Tormen, An excursion set model of hierarchical clustering: ellipsoidal collapse and the moving barrier
2002
Earlier work this paper cites.
E. Hivon, K. M. Górski, C. B. Netterfield, B. P. Crill, S. Prunet, and F. Hansen, MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets
2002
Earlier work this paper cites.
R. E. Smith, J. A. Peacock, and A. Jenkins, Stable clustering, the halo model and non-linear cosmological power spectra
2003
Earlier work this paper cites.
G. Chon, A. Challinor, S. Prunet, E. Hivon, and I. Szapudi, Fast estimation of polarization power spectra using correlation functions
2004
Earlier work this paper cites.
G. Efstathiou, Myths and truths concerning estimation of power spectra: the case for a hybrid estimator
2004
Earlier work this paper cites.
M. A. Zwaan, M. J. Meyer, L. Staveley-Smith, and R. L. Webster, The HIPASS catalogue: Ω H I \Omega_{HI} and environmental effects on the HI mass function of galaxies
2005
Earlier work this paper cites.
V. Springel, The cosmological simulation code GADGET-2
2005
Earlier work this paper cites.
K. M. Górski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke, and M. Bartelmann, Healpix: A framework for high-resolution discretization and fast analysis of data distributed on the sphere
2005
Earlier work this paper cites.
S. M. Rao, D. A. Turnshek, and D. B. Nestor, Damped Ly α \alpha Systems at z < 1.65 z<1.65 : The Expanded Sloan Digital Sky Survey Hubble Space Telescope Sample
2006
Earlier work this paper cites.
J. S. B. Wyithe, A. Loeb, and P. M. Geil, Baryonic acoustic oscillations in 21-cm emission: a probe of dark energy out to high redshifts
Original
2007
Earlier work this paper cites.
P. Lah, J. N. Chengalur, F. H. Briggs, M. Colless, R. De Propris, M. B. Pracy, W. J. G. De Blok, S. S. Fujita, M. Ajiki, Y. Shioya, T. Nagao, T. Murayama, Y. Taniguchi, M. Yagi, and S. Okamura, The H I content of star-forming galaxies at z= 0.24
2007
Earlier work this paper cites.
D. S. Reed, R. Bower, C. S. Frenk, A. Jenkins, and T. Theuns, The halo mass function from the dark ages through the present day
2007
Earlier work this paper cites.
N. Padmanabhan, D. J. Schlegel, U. Seljak, A. Makarov, N. A. Bahcall, M. R. Blanton, J. Brinkmann, D. J. Eisenstein, D. P. Finkbeiner, J. E. Gunn, D. W. Hogg, Ž. Ivezić, G. R. Knapp, J. Loveday, R. H. Lupton, R. C. Nichol, D. P. Schneider, M. A. Strauss, M. Tegmark, and D. G. York, The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging data
2007
Earlier work this paper cites.
A. Cabre, P. Fosalba, E. Gaztañaga, and M. Manera, Error analysis in cross-correlation of sky maps: application to the Integrated Sachs-Wolfe detection
2007
Earlier work this paper cites.
A. Loeb and J. S. B. Wyithe, Possibility of Precise Measurement of the Cosmological Power Spectrum with a Dedicated Survey of 21cm Emission after Reionization
Original
2008
Earlier work this paper cites.

Similar

Then

W. A. Watson, I. T. Iliev, A. D’Aloisio, A. Knebe, P. R. Shapiro, and G. Yepes, The halo mass function through the cosmic ages
Original
2013
Later among the works it cites.
E. Di Dio, F. Montanari, J. Lesgourgues, and R. Durrer, The CLASSgal code for relativistic cosmological large scale structure
Original
2013
Later among the works it cites.
E. Papastergis, R. Giovanelli, M. P. Haynes, A. Rodríguez-Puebla, and M. G. Jones, The Clustering of ALFALFA Galaxies: Dependence on H I Mass, Relationship with Optical Samples, and Clues of Host Halo Properties
Original
2013
Later among the works it cites.
P. S. Behroozi, R. H. Wechsler, and H.-Y. Wu, The ROCKSTAR Phase-space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
Original
2013
Later among the works it cites.

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2015

Simulating the Large-Scale Structure of HI Intensity Maps

Seehars, Sebastian, Paranjape, Aseem, Witzemann, Amadeus et al.

Understand

Intensity mapping of neutral hydrogen (HI) is a promising observational probe of cosmology and large-scale structure.

We present wide field simulations of HI intensity maps based on N-body simulations of a $2.6\, {\rm Gpc / h}$ box with $2048^3$ particles (particle mass $1.6 \times 10^{11}\, {\rm M_\odot / h}$).
Using a conditional mass function to populate the simulated dark matter density field with halos below the mass resolution of the simulation ($10^{8}\, {\rm M_\odot / h} < M_{\rm halo} < 10^{13}\, {\rm M_\odot / h}$), we assign HI to those halos according to a phenomenological halo to HI mass relation.
The simulations span a redshift range of 0.35 < z < 0.9 in redshift bins of width $\Delta z \approx 0.05$ and cover a quarter of the sky at an angular resolution of about 7'.

Built on

J. Asorey, M. Crocce, E. Gaztanaga, and A. Lewis, Recovering 3D clustering information with angular correlations
Original
1902
Earlier work this paper cites.
P. J. E. Peebles, Statistical Analysis of Catalogs of Extragalactic Objects. I. Theory
1973
Earlier work this paper cites.
N. Kaiser, Clustering in real space and in redshift space
1987
Earlier work this paper cites.
J. R. Bond, S. Cole, G. Efstathiou, and N. Kaiser, Excursion set mass functions for hierarchical Gaussian fluctuations
1991
Earlier work this paper cites.
F. Bernardeau, The nonlinear evolution of rare events
1994
Earlier work this paper cites.
L. Knox, Determination of inflationary observables by cosmic microwave background anisotropy experiments
1995
Earlier work this paper cites.
M. Tegmark and G. Efstathiou, A method for subtracting foregrounds from multifrequency CMB sky maps
1996
Earlier work this paper cites.
J. R. Bond, A. H. Jaffe, and L. Knox, Estimating the Power Spectrum of the Cosmic Microwave Background
1998
Earlier work this paper cites.
R. K. Sheth and G. Lemson, Biasing and the distribution of dark matter haloes
1999
Earlier work this paper cites.
S. M. Rao and D. A. Turnshek, Discovery of DampedLy α \alpha Systems at Redshifts Less than 1.65 and Results on Their Incidence and Cosmological Mass Density
2000
Earlier work this paper cites.
I. Szapudi, S. Prunet, and S. Colombi, Fast Analysis of Inhomogenous Megapixel Cosmic Microwave Background Maps
2001
Earlier work this paper cites.
M. Tegmark and A. de Oliveira-Costa, How to measure CMB power spectra without losing information
2001
Earlier work this paper cites.
I. Szapudi, S. Prunet, D. Pogosyan, A. S. Szalay, and J. R. Bond, Fast Cosmic Microwave Background Analyses via Correlation Functions
2001
Earlier work this paper cites.
V. Springel, N. Yoshida, and S. D. M. White, GADGET: a code for collisionless and gasdynamical cosmological simulations
2001
Earlier work this paper cites.
R. K. Sheth and G. Tormen, An excursion set model of hierarchical clustering: ellipsoidal collapse and the moving barrier
2002
Earlier work this paper cites.
E. Hivon, K. M. Górski, C. B. Netterfield, B. P. Crill, S. Prunet, and F. Hansen, MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets
2002
Earlier work this paper cites.
R. E. Smith, J. A. Peacock, and A. Jenkins, Stable clustering, the halo model and non-linear cosmological power spectra
2003
Earlier work this paper cites.
G. Chon, A. Challinor, S. Prunet, E. Hivon, and I. Szapudi, Fast estimation of polarization power spectra using correlation functions
2004
Earlier work this paper cites.
G. Efstathiou, Myths and truths concerning estimation of power spectra: the case for a hybrid estimator
2004
Earlier work this paper cites.
M. A. Zwaan, M. J. Meyer, L. Staveley-Smith, and R. L. Webster, The HIPASS catalogue: Ω H I \Omega_{HI} and environmental effects on the HI mass function of galaxies
2005
Earlier work this paper cites.
V. Springel, The cosmological simulation code GADGET-2
2005
Earlier work this paper cites.
K. M. Górski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke, and M. Bartelmann, Healpix: A framework for high-resolution discretization and fast analysis of data distributed on the sphere
2005
Earlier work this paper cites.
S. M. Rao, D. A. Turnshek, and D. B. Nestor, Damped Ly α \alpha Systems at z < 1.65 z<1.65 : The Expanded Sloan Digital Sky Survey Hubble Space Telescope Sample
2006
Earlier work this paper cites.
J. S. B. Wyithe, A. Loeb, and P. M. Geil, Baryonic acoustic oscillations in 21-cm emission: a probe of dark energy out to high redshifts
Original
2007
Earlier work this paper cites.
P. Lah, J. N. Chengalur, F. H. Briggs, M. Colless, R. De Propris, M. B. Pracy, W. J. G. De Blok, S. S. Fujita, M. Ajiki, Y. Shioya, T. Nagao, T. Murayama, Y. Taniguchi, M. Yagi, and S. Okamura, The H I content of star-forming galaxies at z= 0.24
2007
Earlier work this paper cites.
D. S. Reed, R. Bower, C. S. Frenk, A. Jenkins, and T. Theuns, The halo mass function from the dark ages through the present day
2007
Earlier work this paper cites.
N. Padmanabhan, D. J. Schlegel, U. Seljak, A. Makarov, N. A. Bahcall, M. R. Blanton, J. Brinkmann, D. J. Eisenstein, D. P. Finkbeiner, J. E. Gunn, D. W. Hogg, Ž. Ivezić, G. R. Knapp, J. Loveday, R. H. Lupton, R. C. Nichol, D. P. Schneider, M. A. Strauss, M. Tegmark, and D. G. York, The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging data
2007
Earlier work this paper cites.
A. Cabre, P. Fosalba, E. Gaztañaga, and M. Manera, Error analysis in cross-correlation of sky maps: application to the Integrated Sachs-Wolfe detection
2007
Earlier work this paper cites.
A. Loeb and J. S. B. Wyithe, Possibility of Precise Measurement of the Cosmological Power Spectrum with a Dedicated Survey of 21cm Emission after Reionization
Original
2008
Earlier work this paper cites.

Similar

Then

W. A. Watson, I. T. Iliev, A. D’Aloisio, A. Knebe, P. R. Shapiro, and G. Yepes, The halo mass function through the cosmic ages
Original
2013
Later among the works it cites.
E. Di Dio, F. Montanari, J. Lesgourgues, and R. Durrer, The CLASSgal code for relativistic cosmological large scale structure
Original
2013
Later among the works it cites.
E. Papastergis, R. Giovanelli, M. P. Haynes, A. Rodríguez-Puebla, and M. G. Jones, The Clustering of ALFALFA Galaxies: Dependence on H I Mass, Relationship with Optical Samples, and Clues of Host Halo Properties
Original
2013
Later among the works it cites.
P. S. Behroozi, R. H. Wechsler, and H.-Y. Wu, The ROCKSTAR Phase-space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
Original
2013
Later among the works it cites.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Original

2010

Cited alongside, same era.

M. Crocce, P. Fosalba, F. J. Castander, and E. Gaztañaga, Simulating the Universe with MICE: the abundance of massive clusters

Original

2010

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V. Desjacques and R. K. Sheth, Redshift space correlations and scale-dependent stochastic biasing of density peaks

Original

2010

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Y. Gong, A. Cooray, M. B. Silva, M. G. Santos, and P. Lubin, Probing Reionization with Intensity Mapping of Molecular and Fine-structure Lines

Original

2011

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N. Khandai, S. K. Sethi, T. Di Matteo, R. A. C. Croft, V. Springel, A. Jana, and J. P. Gardner, Detecting neutral hydrogen in emission at redshift z ≃ 1 z\simeq 1

Original

2011

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Thomas, S A and Abdalla, F B and Lahav, O, The angular power spectra of photometric sloan digital sky survey luminous red galaxies

Original

2011

Cited alongside, same era.

C. Bonvin and R. Durrer, What galaxy surveys really measure

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2011

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A. Challinor and A. Lewis, Linear power spectrum of observed source number counts

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Cited alongside, same era.

arXiv:1406.2288

Original

K. Bandura, G. E. Addison, M. Amiri, J. R. Bond, D. Campbell-Wilson, L. Connor, J. F. Cliche, G. Davis, M. Deng, N. Denman, M. Dobbs, M. Fandino, K. Gibbs, A. Gilbert, M. Halpern, D. Hanna, A. D. Hincks, G. Hinshaw, C. Höfer, P. Klages, T. L. Landecker, K. Masui, J. Mena P, L. B. Newburgh, U. L. Pen, J. B. Peterson, A. Recnik, J. R. Shaw, K. Sigurdson, M. Sitwell, G. Smecher, R. Smegal, K. Vanderlinde, and D. Wiebe, Canadian Hydrogen Intensity Mapping Experiment (CHIME) pathfinder · 2014