Prospects of Detecting HI using Redshifted 21-cm Radiation at z∼3-Reference-Cited by-同舟云学术

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Prospects of Detecting HI using Redshifted 21-cm Radiation at z∼3

Published:2017-03 Issue:1 Volume:38 Page:
ISSN:0250-6335
Container-title:Journal of Astrophysics and Astronomy
language:en
Short-container-title:J Astrophys Astron

Author:

Gehlot Bharat Kumar,Bagla J. S.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s12036-017-9436-y.pdf

Reference57 articles.

1. Ali, S. S. Bharadwaj, S. 2014, JApA, 35, 157.

2. Ali, S. S., Bharadwaj, S. Chengalur, J. N. 2008, MNRAS, 385, 2166.

3. Bagla, J. S., Nath, B. Padmanabhan, T. 1997, MNRAS, 289, 671.

4. Bagla, J. S., Khandai, N. Datta, K. K. 2010, MNRAS, 407, 567.

5. Bargur, G. S., Prasad, P., Subrahmanya, C. R., Manoharan, P. K., Nandagopal, D. Dhivya, S. 2011, ASInC, 3, 165.

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Constraining warm dark matter power spectrum using the cross-correlation of HI 21 cm signal and the Lyman-α forest;Journal of Cosmology and Astroparticle Physics;2019-12-19

2. An analytical method to simulate the H i 21-cm visibility signal for intensity mapping experiments;Monthly Notices of the Royal Astronomical Society;2017-09-11

3. The Ooty Wide Field Array;Journal of Astrophysics and Astronomy;2017-03

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