Designing High-Affinity Peptides for Organic Molecules by Explicit Solvent Molecular Dynamics

2015 ◽  
Vol 119 (41) ◽  
pp. 12963-12969 ◽  
Author(s):  
Ivan Gladich ◽  
Alex Rodriguez ◽  
Rolando P. Hong Enriquez ◽  
Filomena Guida ◽  
Federico Berti ◽  
...  
2013 ◽  
Vol 104 (2) ◽  
pp. 556a
Author(s):  
Rolando P. Hong Enriquez ◽  
Silvia Pavan ◽  
Fabio Benedetti ◽  
Alessandro Tossi ◽  
Adriano Savoini ◽  
...  

2012 ◽  
Vol 8 (3) ◽  
pp. 1121-1128 ◽  
Author(s):  
Rolando P. Hong Enriquez ◽  
Silvia Pavan ◽  
Fabio Benedetti ◽  
Alessandro Tossi ◽  
Adriano Savoini ◽  
...  

1989 ◽  
Vol 50 (C2) ◽  
pp. C2-33-C2-35 ◽  
Author(s):  
D. FENYÖ ◽  
B. U.R. SUNDQVIST ◽  
B. KARLSSON ◽  
R. E. JOHNSON

Molecules ◽  
2021 ◽  
Vol 26 (3) ◽  
pp. 721
Author(s):  
Srinivasaraghavan Kannan ◽  
Pietro G. A. Aronica ◽  
Thanh Binh Nguyen ◽  
Jianguo Li ◽  
Chandra S. Verma

S100B(ββ) proteins are a family of multifunctional proteins that are present in several tissues and regulate a wide variety of cellular processes. Their altered expression levels have been associated with several human diseases, such as cancer, inflammatory disorders and neurodegenerative conditions, and hence are of interest as a therapeutic target and a biomarker. Small molecule inhibitors of S100B(ββ) have achieved limited success. Guided by the wealth of available experimental structures of S100B(ββ) in complex with diverse peptides from various protein interacting partners, we combine comparative structural analysis and molecular dynamics simulations to design a series of peptides and their analogues (stapled) as S100B(ββ) binders. The stapled peptides were subject to in silico mutagenesis experiments, resulting in optimized analogues that are predicted to bind to S100B(ββ) with high affinity, and were also modified with imaging agents to serve as diagnostic tools. These stapled peptides can serve as theranostics, which can be used to not only diagnose the levels of S100B(ββ) but also to disrupt the interactions of S100B(ββ) with partner proteins which drive disease progression, thus serving as novel therapeutics.


2014 ◽  
Vol 82 (7) ◽  
pp. 1319-1331 ◽  
Author(s):  
Garrett B. Goh ◽  
Benjamin S. Hulbert ◽  
Huiqing Zhou ◽  
Charles L. Brooks

2016 ◽  
Vol 18 (18) ◽  
pp. 13052-13065 ◽  
Author(s):  
Emanuel K. Peter ◽  
Joan-Emma Shea ◽  
Igor V. Pivkin

In this paper, we present a coarse replica exchange molecular dynamics (REMD) approach, based on kinetic Monte Carlo (kMC).


Author(s):  
Panpan Wang ◽  
Xiaonan Gao ◽  
Ke Zhang ◽  
Qinglan Pei ◽  
Xiaobo Xu ◽  
...  

Based on the binding mode and electrostatics, the features of high affinity PAMs were the reduced hydrophobicity with low electronegativity of R1, increased hydrophobicity with low electronegativity of R2 and with high electronegativity of linker.


2019 ◽  
Vol 629 ◽  
pp. A28 ◽  
Author(s):  
Natalia Inostroza ◽  
Diego Mardones ◽  
Jose Cernicharo ◽  
Hans Zinnecker ◽  
Jixing Ge ◽  
...  

We present a detailed simulation of a dust grain covered by a decamer of (CH3OH)10-ice-mantle, bombarded by an OH− closed-shell molecule with kinetic energies from 10–22 eV. The chemical pathways are studied through Born-Oppenheimer (ab initio) molecular dynamics. The simulations show that methanol ice-mantles can be a key generator of complex organic molecules (COMs). We report the formation of COMs such as methylene glycol (CH2(OH)2) and the OCH2OH radical, which have not been detected yet in the interstellar medium (ISM). We discuss the chemical formation of new species through the reaction of CH3OH with the hydroxyl projectile. The dependence of the outcome on the kinetic energy of the projectile and the implications for the observation and detection of these molecules might explain why the methoxy radical (CH3  ⋅ ) has been observed in a wider range of astrophysical environments than the hydroxymethyl (CH2OH ⋅) isomer. Because of the projectile kinetic energies required for these reactions to occur, we suggest that these processes are likely relevant in the production of COMs in photodissociation and shock regions produced by high-velocity jets and outflows from young stellar objects.


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