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1.E. Dagotto, Science 309, 257 (2005).
2.H. Takagi and H. Y. Hwang, Science 327, 1601 (2010).
3.J. Manhart and D. G. Schlom, Science 327, 1607 (2010).
4.P. Zubko, S. Gariglio, M. Gabay, P. Ghosez, and J.-M. Triscone, Annu. Rev. Condens. Matter Phys. 2(1), 141 (2011).
5.H. Y. Hwang, Y. Iwasa, M. Kawasaki, B. Keimer, N. Nagaosa, and Y. Tokura, Nat. Mater. 11, 103 (2012).
6.J. M. Rondinelli and N. A. Spaldin, Adv. Mater. 23, 3363 (2011).
7.O. E. Peil, M. Ferrero, and A. Georges, Phys. Rev. B 90, 045128 (2014).
8.D. G. Schlom, L.-Q. Chen, C.-B. Eom, K. M. Rabe, S. K. Streiffer, and J.-M. Triscone, Annu. Rev. Mater. Res. 37(1), 589 (2007).
9.J. He, A. Borisevich, S. V. Kalinin, S. J. Pennycook, and S. T. Pantelides, Phys. Rev. Lett. 105, 227203 (2010).
10.M. Gibert, P. Zubko, R. Scherwitzl, J. Íñiguez, and J.-M. Triscone, Nat. Mater. 11(3), 195 (2012).
11.E. J. Moon, P. V. Balachandran, B. J. Kirby, D. J. Keavney, R. J. Sichel-Tissot, C. M. Schlepütz, E. Karapetrova, X. M. Cheng, J. M. Rondinelli, and S. J. May, Nano Lett. 14, 2509 (2014).
12.J. M. Rondinelli, S. J. May, and J. W. Freeland, MRS Bull. 37(03), 261 (2012).
13.F. He, B. O. Wells, and S. M. Shapiro, Phys. Rev. Lett. 94(17), 176101 (2005).
14.T. T. Fister, H. Zhou, Z. Luo, S. S. A. Seo, S. O. Hruszkewycz, D. L. Proffit, J. A. Eastman, P. H. Fuoss, P. M. Baldo, H. N. Lee, and D. D. Fong, APL Mater. 2(2), 021102 (2014).
15.M. Imada, A. Fujimori, and Y. Tokura, Rev. Mod. Phys. 70, 1039 (1998).
16.M. L. Medarde, J. Phys.: Condens. Matter 9(8), 1679 (1997).
17.G. Catalan, Phase Transitions 81(7-8), 729 (2008).
18.P. C. Canfield, J. D. Thompson, S. W. Cheong, and L. W. Rupp, Phys. Rev. B 47(18), 12357 (1993).
19.J. B. Torrance, P. Lacorre, A. I. Nazzal, E. J. Ansaldo, and C. Niedermayer, Phys. Rev. B 45(14), 8209 (1992).
20.A. S. Disa, D. P. Kumah, J. H. Ngai, E. D. Specht, D. A. Arena, F. J. Walker, and C. H. Ahn, APL Mater. 1, 032110 (2013).
21.J. Liu, M. Kargarian, M. Kareev, B. Gray, P. J. Ryan, A. Cruz, N. Tahir, Y.-D. Chuang, J. Guo, J. M. Rondinelli, J. W. Freeland, G. A. Fiete, and J. Chakhalian, Nat. Commun. 4, 2714 (2013).
22.R. Scherwitzl, P. Zubko, I. G. Lezama, S. Ono, A. F. Morpurgo, G. Catalan, and J.-M. Triscone, Adv. Mater. 22(48), 5517 (2010).
23.S. Catalano, M. Gibert, V. Bisogni, O. E. Peil, F. He, R. Sutarto, M. Viret, P. Zubko, R. Scherwitzl, A. Georges, G. A. Sawatzky, T. Schmitt, and J.-M. Triscone, APL Mater. 2, 116110 (2014).
24.P.-H. Xiang, N. Zhong, C.-G. Duan, X. D. Tang, Z. G. Hu, P. X. Yang, Z. Q. Zhu, and J. H. Chu, J. Appl. Phys. 114, 243713 (2013).
25.J. Son, B. Jalan, A. P. Kajdos, L. Balents, S. J. Allen, and S. Stemmer, Appl. Phys. Lett. 99(19), 192107 (2011).
26.X. K. Lian, F. Chen, X. L. Tan, P. F. Chen, L. F. Wang, G. Y. Gao, S. W. Jin, and W. B. Wu, Appl. Phys. Lett. 103, 172110 (2013).
27.M. Hepting, M. Minola, A. Frano, G. Cristiani, G. Logvenov, E. Schierle, M. Wu, M. Bluschke, E. Weschke, H. U. Habermeier, E. Benckiser, M. Le Tacon, and B. Keimer, Phys. Rev. Lett. 113(22), 227206 (2014).
28.See supplementary material at for a more detailed description.[Supplementary Material]
29.G. Catalan, R. M. Bowman, and J. M. Gregg, Phys. Rev. B 62(12), 7892 (2000).
30.D. G. Hawthorn, F. He, L. Venema, H. Davis, A. J. Achkar, J. Zhang, R. Sutarto, H. Wadati, A. Radi, T. Wilson, G. Wright, K. M. Shen, J. Geck, H. Zhang, V. Novák, and G. A. Sawatzky, Rev. Sci. Instrum. 82, 073104 (2011).
31.A. Frano, E. Schierle, M. W. Haverkort, Y. Lu, M. Wu, S. Blanco-Canosa, U. Nwankwo, A. V. Boris, P. Wochner, G. Cristiani, H. U. Habermeier, G. Logvenov, V. Hinkov, E. Benckiser, V. Weschke, and B. Keimer, Phys. Rev. Lett. 111(10), 106804 (2013).
32.J. L. Garcia-Muñoz, J. Rodriguez-Carvajal, and P. Lacorre, Europhys. Lett. 20(3), 241 (1992).
33.V. Scagnoli, U. Staub, A. M. Mulders, M. Janousch, G. I. Meijer, G. Hammerl, J. M. Tonnerre, and N. Stojic, Phys. Rev. B 73(10), 100409 (2006).
34.A. D. Caviglia, M. Först, R. Scherwitzl, V. Khanna, H. Bromberger, R. Mankowsky, R. Singla, Y.-D. Chuang, W. S. Lee, O. Krupin, W. F. Schlotter, J. J. Turner, G. L. Dakovski, M. P. Minitti, J. Robinson, V. Scagnoli, S. B. Wilkins, S. A. Cavill, M. Gibert, S. Gariglio, P. Zubko, J.-M. Triscone, J. P. Hill, S. S. Dhesi, and A. Cavalleri, Phys. Rev. B 88, 220401(R) (2013).
35.W. Marti, P. Fischer, F. Altorfer, H. J. Scheel, and M. Tadin, J. Phys.: Condens. Matter 6, 127 (1994).
36.C. J. Howard, B. J. Kennedy, and B. C. Chakoumakos, J. Phys.: Condens. Matter 12, 349 (2000).
37.F. He, B. O. Wells, Z. G. Ban, S. P. Alpay, S. Grenier, S. M. Shapiro, W. Si, A. Clark, and X. X. Xi, Phys. Rev. B 70(23), 235405 (2004).
38.I. V. Nikulin, M. A. Novojilov, A. R. Kaul, A. F. Maiorova, and S. N. Mudretsova, Mater. Res. Bull. 39(6), 803 (2004).
39.J.-S. Zhou, J. B. Goodenough, and B. Dabrowski, Phys. Rev. Lett. 95, 127204 (2005).

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Bulk NdNiO and thin films grown along the (001) axis display a 1st order metal to insulator transition (MIT) together with a Néel transition at T = 200 K. Here, we show that for NdNiO films deposited on (111) NdGaO, the MIT occurs at T = 335 K and the Néel transition at T = 230 K. By comparing transport and magnetic properties of layers grown on substrates with different symmetries and lattice parameters, we demonstrate a particularly large tuning when the epitaxy is realized on (111) surfaces. We attribute this effect to the specific lattice matching conditions imposed along this direction when using orthorhombic substrates.


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