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Sheth R. K., Tormen G., 1999, MNRAS, 308, 119, arXiv:astro-ph/9901122
1999
Earlier work this paper cites.
Lewis A., Challinor A., Lasenby A., 2000, Astrophys. J., 538, 473, arXiv:astro-ph/9911177
2000
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Blake C., Glazebrook K., 2003, ApJ, 594, 665, arXiv:astro-ph/0301632
2003
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Smith R., et al., 2003, MNRAS, 341, 1311, arXiv:astro-ph/0207664
2003
Earlier work this paper cites.
Meyer M. J. et al., 2004, MNRAS, 350, 1195, arXiv:astro-ph/0406384
2004
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Springel V., et al., 2005, Nature, 435, 629, arXiv:astro-ph/0504097
2005
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De Lucia G., Blaizot J., 2007, MNRAS, 375, 2, arXiv:astro-ph/0606519
2007
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Seo H.-J., Eisenstein D. J., 2007, ApJ, 665, 14, arXiv:astro-ph/0701079
2007
Earlier work this paper cites.
Abdalla F. B., Blake C., Rawlings S., 2009, MNRAS, 401, 743, arXiv:0905.4311
Original
2009
Earlier work this paper cites.
Coe D., 2009, arXiv:0906.4123
Original
2009
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Obreschkow D., Klöckner H.-R., Heywood I., Levrier F., Rawlings S., 2009, ApJ, 703, 1890, arXiv:0908.0983
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2011
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Then

Obreschkow D., Ma X., Meyer M., et al., 2013, Astrophys. J, 766, 137, arXiv:1302.3687
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2013
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2013
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2014
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2014
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2014
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2014

Cosmological performance of SKA HI galaxy surveys

Yahya, S., Bull, P., Santos, M. G. et al.

Understand

The Square Kilometre Array (SKA) will conduct the biggest spectroscopic galaxy survey ever, by detecting the 21cm emission line of neutral hydrogen (HI) from around a billion galaxies over 3/4 of the sky, out to a redshift of z~2.

This will allow the redshift-space matter power spectrum, and corresponding dark energy observables, to be measured with unprecedented precision.
In this paper, we present an improved model of the HI galaxy number counts and bias from semi-analytic simulations, and use it to calculate the expected yield of HI galaxies from surveys with a variety of Phase 1 and 2 SKA configurations.
We illustrate the relative performance of the different surveys by forecasting errors on the radial and transverse scales of the baryon acoustic oscillation (BAO) feature, finding that the full "billion galaxy survey" with SKA2 will deliver the largest dark energy figure of merit of any current or future large-scale structure survey.

Built on

Sheth R. K., Tormen G., 1999, MNRAS, 308, 119, arXiv:astro-ph/9901122
1999
Earlier work this paper cites.
Lewis A., Challinor A., Lasenby A., 2000, Astrophys. J., 538, 473, arXiv:astro-ph/9911177
2000
Earlier work this paper cites.
Blake C., Glazebrook K., 2003, ApJ, 594, 665, arXiv:astro-ph/0301632
2003
Earlier work this paper cites.
Smith R., et al., 2003, MNRAS, 341, 1311, arXiv:astro-ph/0207664
2003
Earlier work this paper cites.
Meyer M. J. et al., 2004, MNRAS, 350, 1195, arXiv:astro-ph/0406384
2004
Earlier work this paper cites.
Springel V., et al., 2005, Nature, 435, 629, arXiv:astro-ph/0504097
2005
Earlier work this paper cites.
De Lucia G., Blaizot J., 2007, MNRAS, 375, 2, arXiv:astro-ph/0606519
2007
Earlier work this paper cites.
Seo H.-J., Eisenstein D. J., 2007, ApJ, 665, 14, arXiv:astro-ph/0701079
2007
Earlier work this paper cites.
Abdalla F. B., Blake C., Rawlings S., 2009, MNRAS, 401, 743, arXiv:0905.4311
Original
2009
Earlier work this paper cites.
Coe D., 2009, arXiv:0906.4123
Original
2009
Earlier work this paper cites.

Similar

Obreschkow D., Klöckner H.-R., Heywood I., Levrier F., Rawlings S., 2009, ApJ, 703, 1890, arXiv:0908.0983
Original
2009
Cited alongside, same era.
Bassett B., Hlozek R., 2010, arXiv: 0910.5224
2010
Cited alongside, same era.
Seo H.-J. et al., 2010, ApJ, 720, 1650, arXiv:0910.5005
Original
2010
Cited alongside, same era.
Bassett B. A., Fantaye Y., Hlozek H R., Kotze J., 2011, Int. J. Mod. Phys. D, 20, 2559
2011
Cited alongside, same era.
Mehta K. T., Seo H.-J., Eckel J., et al., 2011, ApJ, 734, 94, arXiv:1104.1178
Original
2011
Cited alongside, same era.

Then

Obreschkow D., Ma X., Meyer M., et al., 2013, Astrophys. J, 766, 137, arXiv:1302.3687
Original
2013
Later among the works it cites.
Planck Collaboration XVI 2013, arXiv:1303.5076
Original
2013
Later among the works it cites.
Bull P., Ferreira P. G., Patel P., Santos M. G., 2014, arXiv:1405.1452
Original
2014
Closest in time.
Popping G., Behroozi P. S., Peeples M. S., 2014, arXiv:1409.1574
Original
2014
Closest in time.
Villaescusa-Navarro F., Viel M., Alonso D., et al., 2014, arXiv:1410.7393
Original
2014
Closest in time.

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

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Anderson L., et al., 2012, MNRAS, 427, 3435, arXiv:1203.6594

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2012

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Font-Ribera A., et al., 2012, JCAP, 11, 59, arXiv:1209.4596

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2012

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Amendola L., et al., 2013, Living Rev. Relativity, 16, 6, arXiv:1206.1225

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2013

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Dawson K. S., et al., 2013, Astronomical Journal, 145, 10, arXiv:1208.0022

Original

2013

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Dewdney P. E., et al.,, 2013, SKA1 system baseline design, https://www.skatelescope.org/wp-content/uploads/2013/05/SKA-TEL-SKO-DD-001-1_BaselineDesign1.pdf

2013

Cited alongside, same era.

Braun R., et al., 2015, in Advancing Astrophysics with the Square Kilometre Array. SISSA, Trieste, Italy

2015

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Bull P., Camera S., Raccanelli A., Blake C., Ferreira P. G., et al., 2015, arXiv:1501.04088

Original

2015

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Camera S., Santos M. G., Maartens R., 2015, MNRAS, 448, 1035, arXiv:1409.8286

Original

2015

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Santos M. G., Bull P., Alonso D., Camera S., Ferreira P. G., et al., 2015, arXiv:1501.03989

Original

2015

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