[1] Escudero Sanz I, Heske A, Livas J C. A telescope for LISA-the laser interferometer space antenna[J]. Adv Opt Technol, 7, 395-400(2018).

[2] Sallusti M, Gath P, Weise D et al. LISA system design highlights[J]. Class Quantum Grav, 26, 094015(2009).

[3] Jennrich O. LISA technology and instrumentation[J]. Class Quantum Grav, 26, 153001(2009).

[4] Weise D R, Marenaci P, Weimer P et al. Alternative opto-mechanical architectures for the LISA instrument[J]. J Phys Conf Ser, 154, 012029(2009).

[5] Brugger C, Broll B, Fitzsimons E et al. An experiment to test in-field pointing for Elisa[J]. Proc SPIE, 10563, 105634D(2017).

[6] Witovet G, Human J. Realization and performance validation of the in-field pointing mechanism for the evolved laser interferometer space antenna[C](2015).

[7] Livas J, Sankar S, West G et al. eLISA telescope in-field pointing and scattered light study[J]. J Phys Conf Ser, 840, 012015(2017).

[8] Brzozowski W, Robertson D, Fitzsimons E et al. The LISA optical bench: an overview and engineering challenges[J]. Proc SPIE, 12180, 121800O(2022).

[9] d’Arcio L, Bogenstahl J, Diekmann C et al. An elegant breadboard of the optical bench for eLISA/NGO[J]. Proc SPIE, 10564, 105640I(2017).

[10] Fleddermann R. Interferometry for a space-based gravitational wave observatory: reciprocity of an optical fiber[D](2012).

[11] Fleddermann R, Diekmann C, Steier F et al. Sub-pm Hz−1 non-reciprocal noise in the LISA backlink fiber[J]. Class Quantum Grav, 35, 075007(2018).

[12] Fleddermann R, Steier F, Tröbs M et al. Measurement of the non-reciprocal phase noise of a polarization maintaining single-mode optical fiber[J]. J Phys Conf Ser, 154, 012022(2009).

[13] Steier F, Fleddermann R, Bogenstahl J et al. Construction of the LISA back-side fibre link interferometer prototype[J]. Class Quantum Grav, 26, 175016(2009).

[14] Wang X Y, Bai S J, Zhang Q et al. Research progress of telescopes for space-based gravitational wave missions[J]. Opto-Electron Eng, 50, 230219(2023).

[15] Chwalla M, Danzmann K, Dovale Álvarez M et al. Optical suppression of tilt-to-length coupling in the LISA long-arm interferometer[J]. Phys Rev Appl, 14, 014030(2020).

[16] Chwalla M, Danzmann K, Fernández Barranco G et al. Design and construction of an optical test bed for LISA imaging systems and tilt-to-length coupling[J]. Class Quantum Grav, 33, 245015(2016).

[17] Robins W P. Phase Noise in Signal Sources[M](1982).

[18] Esteban Delgado J J. Laser ranging and data communcation for the laser interferometer space antenna[D](2012).

[19] Barke S. Inter-spacecraft frequency distribution for future gravitational wave observatories[D](2015).

[20] Wissel L, Wittchen A, Schwarze T S et al. Relative-intensity-noise coupling in heterodyne interferometers[J]. Phys Rev Appl, 17, 024025(2022).

[21] Livas J C, Arsenovic P, Crow J A et al. Telescopes for space-based gravitational wave missions[J]. Opt Eng, 52, 091811(2013).

[22] Livas J, Sankar S. Optical telescope design study results[J]. J Phys Conf Ser, 610, 012029(2015).

[23] Livas J C, Sankar S R. Optical telescope system-level design considerations for a space-based gravitational wave mission[J]. Proc SPIE, 9904, 99041K(2016).

[24] Sankar S R, Livas J C. Optical telescope design for a space-based gravitational-wave mission[J]. Proc SPIE, 9143, 914314(2014).

[25] Spector A, Mueller G. Back-reflection from a Cassegrain telescope for space-based interferometric gravitational-wave detectors[J]. Class Quantum Grav, 29, 205005(2012).