These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

122 related articles for article (PubMed ID: 34612385)

  • 21. HXeI and HXeH in Ar, Kr, and Xe matrices: experiment and simulation.
    Zhu C; Niimi K; Taketsugu T; Tsuge M; Nakayama A; Khriachtchev L
    J Chem Phys; 2015 Feb; 142(5):054305. PubMed ID: 25662643
    [TBL] [Abstract][Full Text] [Related]  

  • 22. Quantum Chemistry Meets Spectroscopy for Astrochemistry: Increasing Complexity toward Prebiotic Molecules.
    Barone V; Biczysko M; Puzzarini C
    Acc Chem Res; 2015 May; 48(5):1413-22. PubMed ID: 25894724
    [TBL] [Abstract][Full Text] [Related]  

  • 23. Chemical changes induced during heating of acetonitrile-rich ice pre-irradiated by X-rays and its implication in astrochemistry.
    Carvalho GA; Pilling S
    Spectrochim Acta A Mol Biomol Spectrosc; 2022 Feb; 267(Pt 1):120495. PubMed ID: 34700156
    [TBL] [Abstract][Full Text] [Related]  

  • 24. Matrix effect on vibrational frequencies: experiments and simulations for HCl and HNgCl (Ng = Kr and Xe).
    Kalinowski J; Gerber RB; Räsänen M; Lignell A; Khriachtchev L
    J Chem Phys; 2014 Mar; 140(9):094303. PubMed ID: 24606357
    [TBL] [Abstract][Full Text] [Related]  

  • 25. Theoretical prediction of new noble-gas molecules FNgBNR (Ng = Ar, Kr, and Xe; R = H, CH3, CCH, CHCH2, F, and OH).
    Chen JL; Yang CY; Lin HJ; Hu WP
    Phys Chem Chem Phys; 2013 Jun; 15(24):9701-9. PubMed ID: 23670409
    [TBL] [Abstract][Full Text] [Related]  

  • 26. Environmental effects on noble-gas hydrides: HXeBr, HXeCCH, and HXeH in noble-gas and molecular matrices.
    Tsuge M; Lignell A; Räsänen M; Khriachtchev L
    J Chem Phys; 2013 Nov; 139(20):204303. PubMed ID: 24289350
    [TBL] [Abstract][Full Text] [Related]  

  • 27. Experimental and theoretical studies of the infrared spectra and bonding properties of NgBeCO₃ and a comparison with NgBeO (Ng = He, Ne, Ar, Kr, Xe).
    Zhang Q; Chen M; Zhou M; Andrada DM; Frenking G
    J Phys Chem A; 2015 Mar; 119(11):2543-52. PubMed ID: 25321412
    [TBL] [Abstract][Full Text] [Related]  

  • 28. Reactions of radiation-induced electrons with carbon dioxide in inert cryogenic films: matrix tuning of the excess electron interactions in solids.
    Shiryaeva ES; Baranova IA; Tyurin DA; Feldman VI
    Phys Chem Chem Phys; 2020 Jul; 22(25):14155-14161. PubMed ID: 32609111
    [TBL] [Abstract][Full Text] [Related]  

  • 29. How strong is the interaction between a noble gas atom and a noble metal atom in the insertion compounds MNgF (M=Cu and Ag, and Ng=Ar, Kr, and Xe)?
    Ghanty TK
    J Chem Phys; 2006 Mar; 124(12):124304. PubMed ID: 16599671
    [TBL] [Abstract][Full Text] [Related]  

  • 30. Noble gas-actinide complexes of the CUO molecule with multiple Ar, Kr, and Xe atoms in noble-gas matrices.
    Andrews L; Liang B; Li J; Bursten BE
    J Am Chem Soc; 2003 Mar; 125(10):3126-39. PubMed ID: 12617681
    [TBL] [Abstract][Full Text] [Related]  

  • 31. Extraterrestrial prebiotic molecules: photochemistry vs. radiation chemistry of interstellar ices.
    Arumainayagam CR; Garrod RT; Boyer MC; Hay AK; Bao ST; Campbell JS; Wang J; Nowak CM; Arumainayagam MR; Hodge PJ
    Chem Soc Rev; 2019 Apr; 48(8):2293-2314. PubMed ID: 30815642
    [TBL] [Abstract][Full Text] [Related]  

  • 32. A Very Short Be-Be Distance but No Bond: Synthesis and Bonding Analysis of Ng-Be
    Zhang Q; Li WL; Zhao L; Chen M; Zhou M; Li J; Frenking G
    Chemistry; 2017 Feb; 23(9):2035-2039. PubMed ID: 28009065
    [TBL] [Abstract][Full Text] [Related]  

  • 33. On the noble-gas-induced intersystem crossing for the CUO molecule: experimental and theoretical investigations of CUO(Ng)n (Ng = Ar, Kr, Xe; n = 1, 2, 3, 4) complexes in solid neon.
    Liang B; Andrews L; Li J; Bursten BE
    Inorg Chem; 2004 Feb; 43(3):882-94. PubMed ID: 14753808
    [TBL] [Abstract][Full Text] [Related]  

  • 34. Noble gas-actinide compounds: evidence for the formation of distinct CUO(Ar)(4-n)(Xe)(n) and CUO(Ar)(4-n)(Kr)(n) (n = 1, 2, 3, 4) complexes.
    Liang B; Andrews L; Li J; Bursten BE
    J Am Chem Soc; 2002 Aug; 124(31):9016-7. PubMed ID: 12148982
    [TBL] [Abstract][Full Text] [Related]  

  • 35. A hydrogen-bonded CHF⋯HF complex: IR spectra and unusual photochemistry.
    Sosulin IS; Tyurin DA; Feldman VI
    J Chem Phys; 2021 Mar; 154(10):104310. PubMed ID: 33722008
    [TBL] [Abstract][Full Text] [Related]  

  • 36. Matrix-isolation and ab initio study of HKrCCCl and HXeCCCl.
    Zhu C; Räsänen M; Khriachtchev L
    J Chem Phys; 2015 Dec; 143(24):244319. PubMed ID: 26723683
    [TBL] [Abstract][Full Text] [Related]  

  • 37. Matrix-isolation and Ab initio study of the HKrCl...HCl complex.
    Corani A; Domanskaya A; Khriachtchev L; Räsänen M; Lignell A
    J Phys Chem A; 2009 Oct; 113(40):10687-92. PubMed ID: 19757804
    [TBL] [Abstract][Full Text] [Related]  

  • 38. Radioresistance of Adenine to Cosmic Rays.
    Vignoli Muniz GS; Mejía CF; Martinez R; Auge B; Rothard H; Domaracka A; Boduch P
    Astrobiology; 2017 Apr; 17(4):298-308. PubMed ID: 28418703
    [TBL] [Abstract][Full Text] [Related]  

  • 39. Detecting weak interactions between Au- and gas molecules: a photoelectron spectroscopic and ab initio study.
    Gao Y; Huang W; Woodford J; Wang LS; Zeng XC
    J Am Chem Soc; 2009 Jul; 131(27):9484-5. PubMed ID: 19537810
    [TBL] [Abstract][Full Text] [Related]  

  • 40. Photolysis of CH
    Carvalho GA; Pilling S
    J Phys Chem A; 2020 Oct; 124(41):8574-8584. PubMed ID: 32924515
    [TBL] [Abstract][Full Text] [Related]  

    [Previous]   [Next]    [New Search]
    of 7.