Rebuttal From Dr White et al

White, Douglas B.; Lo, Bernard; Peek, Monica E.

doi:10.1016/j.chest.2022.03.032

Cited by 3 publications

(4 citation statements)

References 3 publications

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“…This is consistent with the underprediction of f σ 8 between 0 < z < 0.75 we discussed in the pre vious section. A lo wer v alue of S 8 would also be consistent with the most recent measurements by large-scale structure experiments (DES Collaboration 2021 ;Garc ía-Garc ía et al 2021 ;Heymans et al 2021 ;Krolewski, Ferraro & White 2021 ;White et al 2021 ), the origin of which could lie on a lo wer v alue of m (Hang et al 2021 ).…”

Section: Cosmolo Gical Parameter Ssupporting

confidence: 87%

“…This result is lower than, but statically compatible with, the Planck 2018 (Planck Collaboration VI 2020 ) cosmology. We also find S 8 = 0.788 ± 0.029, an intermediate value, statistically compatible with both the Planck 2018 cosmology (Planck Collaboration VI 2020 ) and the recent local measurements from weak lensing and galaxy clustering (DES Collaboration 2021 ; Garc ía-Garc ía et al 2021 ; Heymans et al 2021 ;Krolewski et al 2021 ;White et al 2021 ).…”

Section: O N C L U S I O N Ssupporting

confidence: 86%

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Model-independent constraints on Ωm and H(z) from the link between geometry and growth

Ruiz-Zapatero

García-García

Alonso

et al. 2022

Monthly Notices of the Royal Astronomical Society

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We constrain the expansion history of the Universe and the cosmological matter density fraction in a model-independent way by exclusively making use of the relationship between background and perturbations under a minimal set of assumptions. We do so by employing a Gaussian process to model the expansion history of the Universe from present time to the recombination era. The expansion history and the cosmological matter density are then constrained using recent measurements from cosmic chronometers, Type-Ia supernovae, baryon acoustic oscillations, and redshift-space distortion data. Our results show that the evolution in the reconstructed expansion history is compatible with the Planck 2018 prediction at all redshifts. The current data considered in this study can constrain a Gaussian process on H(z) to an average $9.4 \%$ precision across redshift. We find Ωm = 0.224 ± 0.066, lower but statistically compatible with the Planck 2018 cosmology. Finally, the combination of future DESI measurements with the CMB measurement considered in this work holds the promise of $8 \%$ average constraints on a model-independent expansion history as well as a five-fold tighter Ωm constraint using the methodology developed in this work.

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Section: Cosmolo Gical Parameter Ssupporting

confidence: 87%

Section: O N C L U S I O N Ssupporting

confidence: 86%

Model-independent constraints on Ωm and H(z) from the link between geometry and growth

Ruiz-Zapatero

García-García

Alonso

et al. 2022

Monthly Notices of the Royal Astronomical Society

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“…In the case of our patient, GS syndrome developed as a complication of peritonsillar abscess, which is uncommon, being that GS more commonly occurs with retropharyngeal abscesses. 6 Her main complaint was progressive neck pain with limited mobility and associated with left facial swelling, with no sore throat, fever or palpable cervical lymph nodes.…”

Section: Denouementmentioning

confidence: 99%

Cervical Pain in a Seventeen-year-old Girl

Baptista de Lima,

Barros,

Mota Pinheiro

et al. 2024

Pediatric Infectious Disease Journal

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“…This formulation was developed by the U.S. military, made up of cholesterol and liposomes containing saturated phospholipids and monophosphoryl lipid A (MPLA) (82). There are improved versions of army liposome formulation (ALF), i.e., ALF adsorbed to aluminum hydroxide (ALFA), ALF containing the QS21 saponin (ALFQ), and ALFQ adsorbed to aluminum hydroxide (ALFQA) (83,84). It has been found that the vaccine candidate circumsporozite protein of Plasmodium falciparum adjuvanted with ALFA imparted adequate humoral and cellular immune responses (85).…”

Section: Army Liposome Formulationmentioning

confidence: 99%

New-age vaccine adjuvants, their development, and future perspective

Verma

Mahajan²,

Singh³

et al. 2023

Front. Immunol.

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In the present scenario, immunization is of utmost importance as it keeps us safe and protects us from infectious agents. Despite the great success in the field of vaccinology, there is a need to not only develop safe and ideal vaccines to fight deadly infections but also improve the quality of existing vaccines in terms of partial or inconsistent protection. Generally, subunit vaccines are known to be safe in nature, but they are mostly found to be incapable of generating the optimum immune response. Hence, there is a great possibility of improving the potential of a vaccine in formulation with novel adjuvants, which can effectively impart superior immunity. The vaccine(s) in formulation with novel adjuvants may also be helpful in fighting pathogens of high antigenic diversity. However, due to the limitations of safety and toxicity, very few human-compatible adjuvants have been approved. In this review, we mainly focus on the need for new and improved vaccines; the definition of and the need for adjuvants; the characteristics and mechanisms of human-compatible adjuvants; the current status of vaccine adjuvants, mucosal vaccine adjuvants, and adjuvants in clinical development; and future directions.

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Rebuttal From Dr White et al

Cited by 3 publications

References 3 publications

Model-independent constraints on Ωm and H(z) from the link between geometry and growth

Model-independent constraints on Ωm and H(z) from the link between geometry and growth

Cervical Pain in a Seventeen-year-old Girl

New-age vaccine adjuvants, their development, and future perspective

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