Built on

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2018

Ingredients for 21cm intensity mapping

Villaescusa-Navarro, Francisco, Genel, Shy, Castorina, Emanuele et al.

Understand

[Abridged] We study the abundance and clustering properties of HI at redshifts $z\leqslant5$ using TNG100, a large state-of-the-art magneto-hydrodynamic simulation of a 75 Mpc/h box size.

We show that most of the HI lies within dark matter halos and quantify the average HI mass hosted by halos of mass M at redshift z.
We find that only halos with circular velocities larger than $\simeq$ 30 km/s contain HI.
While the density profiles of HI exhibit a large halo-to-halo scatter, the mean profiles are universal across mass and redshift.

Built on

Delhaize, J., Meyer, M. J., Staveley-Smith, L., & Boyle, B. J. 2013, MNRAS, 433, 1398, [arXiv:1305.1968]
Original
1968
Earlier work this paper cites.
Zel’dovich, Y. B. 1970, A&A, 5, 84
1970
Earlier work this paper cites.
Rahmati, A., Schaye, J., Pawlik, A. H., & Rai c ˇ \check{{\rm c}} evi c ` \grave{{\rm c}} , M. 2013b, MNRAS, 431, 2261, [arXiv:1301.1978]
Original
1978
Earlier work this paper cites.
Davis, M., Efstathiou, G., Frenk, C. S., & White, S. D. M. 1985, ApJ, 292, 371
1985
Earlier work this paper cites.
Kaiser, N. 1987, MNRAS, 227, 1
1987
Earlier work this paper cites.
Bryan, G. L., & Norman, M. L. 1998, ApJ, 495, 80, [arXiv:astro-ph/9710107]
1998
Earlier work this paper cites.
Allende Prieto, C., Lambert, D. L., & Asplund, M. 2001, ApJ, 556, L63, [arXiv:astro-ph/0106360]
2001
Earlier work this paper cites.
Bharadwaj, S., Nath, B. B., & Sethi, S. K. 2001, Journal of Astrophysics and Astronomy, 22, 21, [arXiv:astro-ph/0003200]
2001
Earlier work this paper cites.
Bharadwaj, S., & Sethi, S. K. 2001, Journal of Astrophysics and Astronomy, 22, 293, [arXiv:astro-ph/0203269]
2001
Earlier work this paper cites.
Sheth, R. K., Mo, H. J., & Tormen, G. 2001, MNRAS, 323, 1, [arXiv:astro-ph/9907024]
2001
Earlier work this paper cites.
Springel, V., White, S. D. M., Tormen, G., & Kauffmann, G. 2001, MNRAS, 328, 726, [arXiv:arXiv:astro-ph/0012055]
2001
Earlier work this paper cites.
Cooray, A., & Sheth, R. 2002, Phys. Rep., 372, 1, [arXiv:astro-ph/0206508]
2002
Earlier work this paper cites.
Monaco, P., Theuns, T., & Taffoni, G. 2002, MNRAS, 331, 587, [arXiv:astro-ph/0109323]
2002
Earlier work this paper cites.
Sheth, R. K., & Tormen, G. 2002, MNRAS, 329, 61, [arXiv:arXiv:astro-ph/0105113]
2002
Earlier work this paper cites.
Springel, V., & Hernquist, L. 2003, MNRAS, 339, 289, [arXiv:astro-ph/0206393]
2003
Earlier work this paper cites.
Battye, R. A., Davies, R. D., & Weller, J. 2004, Mon.Not.Roy.Astron.Soc., 355, 1339, [arXiv:astro-ph/0401340]
2004
Earlier work this paper cites.
Maller, A. H., & Bullock, J. S. 2004, MNRAS, 355, 694, [arXiv:astro-ph/0406632]
2004
Earlier work this paper cites.
——. 2004, MNRAS, 350, 1385, [arXiv:astro-ph/0402237]
2004
Earlier work this paper cites.
Gao, L., Springel, V., & White, S. D. M. 2005, MNRAS, 363, L66, [arXiv:astro-ph/0506510]
2005
Earlier work this paper cites.
Miralda-Escudé, J. 2005, ApJ, 620, L91, [arXiv:astro-ph/0410315]
2005
Earlier work this paper cites.
Péroux, C., Dessauges-Zavadsky, M., D’Odorico, S., Sun Kim, T., & McMahon, R. G. 2005, MNRAS, 363, 479, [arXiv:astro-ph/0507353]
2005
Earlier work this paper cites.
McQuinn, M., Zahn, O., Zaldarriaga, M., Hernquist, L., & Furlanetto, S. R. 2006, ApJ, 653, 815, [arXiv:astro-ph/0512263]
2006
Earlier work this paper cites.
Rao, S. M., Turnshek, D. A., & Nestor, D. B. 2006, ApJ, 636, 610, [arXiv:astro-ph/0509469]
2006
Earlier work this paper cites.
Schaye, J. 2006, ApJ, 643, 59, [arXiv:astro-ph/0409137]
2006
Earlier work this paper cites.
Wechsler, R. H., Zentner, A. R., Bullock, J. S., Kravtsov, A. V., & Allgood, B. 2006, ApJ, 652, 71, [arXiv:astro-ph/0512416]
2006
Earlier work this paper cites.
Zwaan, M. A., & Prochaska, J. X. 2006, ApJ, 643, 675, [arXiv:astro-ph/0601655]
Original
2006
Earlier work this paper cites.
Gao, L., & White, S. D. M. 2007, MNRAS, 377, L5, [arXiv:astro-ph/0611921]
2007
Earlier work this paper cites.
Lah, P. et al. 2007, MNRAS, 376, 1357, [arXiv:astro-ph/0701668]
2007
Earlier work this paper cites.
Chang, T.-C., Pen, U.-L., Peterson, J. B., & McDonald, P. 2008, Physical Review Letters, 100, 091303, [arXiv:0709.3672]
Original
2008
Earlier work this paper cites.
Krumholz, M. R., McKee, C. F., & Tumlinson, J. 2008, ApJ, 689, 865, [arXiv:0805.2947]
Original
2008
Earlier work this paper cites.
Loeb, A., & Wyithe, J. S. B. 2008, Physical Review Letters, 100, 161301, [arXiv:0801.1677]
Original
2008
Earlier work this paper cites.
Okamoto, T., Gao, L., & Theuns, T. 2008, MNRAS, 390, 920, [arXiv:0806.0378]
Original
2008
Earlier work this paper cites.
Faucher-Giguère, C., Lidz, A., Zaldarriaga, M., & Hernquist, L. 2009, ApJ, 703, 1416, [arXiv:0901.4554]
Original
2009
Earlier work this paper cites.
——. 2009, ApJ, 693, 216, [arXiv:0811.0004]
Original
2009
Earlier work this paper cites.
Obreschkow, D., Klöckner, H.-R., Heywood, I., Levrier, F., & Rawlings, S. 2009, ApJ, 703, 1890, [arXiv:0908.0983]
Original
2009
Earlier work this paper cites.