1. Riess A. G., Filippenko A. V., Challis P., Clocchiatti A., Diercks A., Garnavich P. M. [et al.] (Supernova Search Team). Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant. The Astronomical Journal, 1998, vol. 116, pp. 1009-1038. https://doi.org/10.1086/300499
2. Perlmutter S., Aldering G., Goldhaber G., Knop R. A., Nugent P., Castro P. G. [et al.] (Supernova Cosmology Project). Measurements of Ω and Λ from 42 High-Redshift. Supernovae. The Astronomical Journal, 1998, vol. 517, pp. 565-586. https://doi.org/10.1086/307221
3. Eisenstein D. J., Zehavi I., Hogg D. W., Scoccimarro R., Blanton M. R., Nichol R. C., Scranton R. [et al.] (SDSS). Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies. The Astronomical Journal, 2005, vol. 633, pp. 560-574. https://doi.org/10.1086/466512
4. Sahni V., Starobinski A. The Case for a Positive Cosmological Lambda Term. International Journal of Modern Physics D, 2000, vol. 9, no. 4, pp. 373-444. https://doi.org/10.1142/S0218271800000542
5. Padmanabhan T. Cosmological constant - the weight of the vacuum. Physics Reports, 2003, vol. 380, no. 5-6, pp. 235- 320. https://doi.org/10.1016/S0370-1573(03)00120-0
6. Matos T., Guzman F. S. On the spacetime of a galaxy. Classical and Quantum Gravity, 2001, vol. 18, no. 23, pp. 5055- 5064. https://doi.org/10.1088/0264-9381/18/23/303
7. Peebles P. J. E., Ratra B. The cosmological constant and dark energy. Reviews of Modern Physics, 2003, vol. 75, pp. 559-606. https://doi.org/10.1103/revmodphys.75.559
8. Copeland E. J., Sami M., Tsujikawa S. Dynamics of dark energy. International Journal of Modern Physics D, 2006, vol. 15, no. 11, pp. 1753-1936. https://doi.org/10.1142/s021827180600942x
9. Belinchón J. A., Harko T., Mak M. K. Exact Scalar-Tensor Cosmological Solutions via Noether Symmetry. Astrophysics and Space Science, 2016, vol. 361, no. 2, p. 52. https://doi.org/10.1007/s10509-015-2642-7
10. Scherrer R. J., Sen A. A. Thawing quintessence with a nearly flat potential. Physical Review D, 2008, vol. 77, 083515. https://doi.org/10.1103/PhysRevD.77.083515
11. Starobinsky A. A. How to determine an effective potential for a variable cosmological term. Journal of Experimental and Theoretical Physics Letters, 1998, vol. 68, pp. 757-763. https://doi.org/10.1134/1.567941
12. Freund P., Nambu Y. Scalar Fields Coupled to the Trace of the Energy-Momentum Tensor. Physical Review, 1968, vol. 174, pp. 1741-1747. https://doi.org/10.1103/physrev.174.1741
13. Dudko I. G., Vyblyi Yu. P. Scalar field with the source in the form of the stress-energy tensor trace as a dark energy model. Gravitation and Cosmology, 2016, vol. 22, pp. 368-373. https://doi.org/10.1134/s020228931604006x
14. Sharov G. S., Vasilev V. O. How predictions of cosmological models depend on Hubble parameter data sets. Mathematical Modelling and Geometry, 2018, vol. 6, no, 1, pp. 1-20. https://doi.org/10.26456/mmg/2018-611
15. Scolnic D. M., Jones D. O., Rest A., Pan Y. C., Chornock R., Foley R. J., Huber M. E. [et al.] The Complete Lightcurve Sample of Spectroscopically Confirmed SNe la from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample. The Astronomical Journal, 2018, vol. 859, no. 2, p. 101. https://doi.org/10.3847/1538-4357/aab9bb