Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys | Paper Citation Record

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This paper cites Sachs and A.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Sachs and A

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Observation 02292668-f581-49ca-87f5-dd826c0f0861 · outbound

This paper cites How Filaments are Woven into the Cosmic Web.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys How Filaments are Woven into the Cosmic Web

Reference 2

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 4

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This paper cites Maeder, The Astrophysical Journal 834, 194 (2017).

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Maeder, The Astrophysical Journal 834, 194 (2017)

Reference 5

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 6

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 7

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

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This paper cites Beutler, C.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Beutler, C

Reference 9

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This paper cites Alam and et al., Monthly Notices of the Royal Astronomical Society 470, 2617 (2017), https://academic.oup.com/mnras/article- pdf/470/3/2617/18315003/stx721.pdf.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Alam and et al., Monthly Notices of the Royal Astronomical Society 470, 2617 (2017), https://academic.oup.com/mnras/article- pdf/470/3/2617/18315003/stx721.pdf

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This paper cites Howlett, A.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Howlett, A

Reference 11

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 12

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This paper cites McDonald, U.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys McDonald, U

Reference 13

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This paper cites IrVsiVc, M.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys IrVsiVc, M

Reference 14

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This paper cites Slosar, A.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Slosar, A

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This paper cites Garzilli, A.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Garzilli, A

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This paper cites Hamilton, in The evolving universe (Springer, 1998) pp.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Hamilton, in The evolving universe (Springer, 1998) pp

Reference 17

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This paper cites Delubac, J.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Delubac, J

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This paper cites Font-Ribera, J.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Font-Ribera, J

Reference 19

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 20

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This paper cites an unresolved cited work.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 21

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This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 22

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Adame, J

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys The DESI Experiment, a whitepaper for Snowmass 2013

Reference 24

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This paper cites Scaramella, J.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Scaramella, J

Reference 25

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This paper cites Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys

Reference 26

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 27

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This paper cites Abbott, M.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Abbott, M

Reference 28

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Porredon and et al

Reference 29

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This paper cites Pandey and et al.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Pandey and et al

Reference 30

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This paper cites Hikage and et al., Publications of the Astronomical Society of Japan 71, 43 (2019), https://academic.oup.com/pasj/article- pdf/71/2/43/54666032/pasj 71 2 43.pdf.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Hikage and et al., Publications of the Astronomical Society of Japan 71, 43 (2019), https://academic.oup.com/pasj/article- pdf/71/2/43/54666032/pasj 71 2 43.pdf

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This paper cites Karim and et al., Journal of Cosmology and Astropar- ticle Physics 2025 (02), 045.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Karim and et al., Journal of Cosmology and Astropar- ticle Physics 2025 (02), 045

Reference 32

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Nusser, E

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys HI Fluctuations at Large Redshifts: I--Visibility correlation

Reference 35

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Bharadwaj, B

Reference 36

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Fluctuations in 21cm Emission After Reionization

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization

Reference 38

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys The 21cm Power Spectrum After Reionization

Reference 39

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Cosmological constraints from 21cm surveys after reionization

Reference 40

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys HI Fluctuations at Large Redshifts: II - the Signal Expected for GMRT

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys HI Fluctuations at Large Redshifts: III - Simulating the Signal Expected at GMRT

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Subramanian and T

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Kumar, T

Reference 44

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This paper cites Neutral hydrogen at high redshifts as a probe of structure formation - III. Radio maps from N-Body simulations.

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Neutral hydrogen at high redshifts as a probe of structure formation - III. Radio maps from N-Body simulations

Reference 45

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Padmanabhan, T

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Guha Sarkar, S

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Sarkar, S

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Evolution of Neutral Gas at High Redshift -- Implications for the Epoch of Galaxy Formation

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Peroux, R

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys McQuinn, O

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Chavan, T

Reference 54

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Foreman-Mackey, D

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Kazantzidis and L

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Nesseris and J

Reference 57

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys A semi-cosmographic approach to study cosmological evolution in phase space

Reference 58

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Holsclaw, U

Reference 60

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Shafieloo, A

Reference 61

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Mukherjee and A

Reference 65

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys On using visibility correlations to probe the HI distribution from the dark ages to the present epoch I: Formalism and the expected signal

Reference 67

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Di Matteo, R

Reference 70

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Ghosh, S

Reference 71

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 72

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys The Epoch of Reionization Window: I. Mathematical Formalism

Reference 73

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Liu and M

Reference 74

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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys Unresolved cited work

Reference 75

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