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A Farrell, K. Mori, K. Pfrang, K. Ragan, L. Fortson, M. Capasso, MDM) C. B. Adams, M. Errando, M. J. Lang, M. Kertzman, M. Nievas-Rosillo, M. Pohl, M. Santander, N. Park, O. Hervet, P. Kaaret, P. Moriarty, P. T. Reynolds, R. A. Ong, R. Mukherjee, R. R. Prado, S. O'Brien, S. Patel, S. Schlenstedt, T. B. Humensky, T. Hassan, T. J Williamson (VERITAS collaboration), W. Benbow, W. Jin, Y. M. Tokayer","submitted_at":"2021-10-03T19:16:31Z","abstract_excerpt":"HESS J0632+057 belongs to a rare subclass of binary systems which emits gamma-rays above 100 GeV. It stands out for its distinctive high-energy light curve, which features a sharp ``primary'' peak and broader ``secondary'' peak. We present the results of contemporaneous observations by NuSTAR and VERITAS during the secondary peak between Dec. 2019 and Feb. 2020, when the orbital phase ($\\phi$) is between 0.55 and 0.75. NuSTAR detected X-ray spectral evolution, while VERITAS detected TeV emission. 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Brill, A. Falcone, A. Furniss, A. Gent, A. N. Otte, A. Weinstein, B. Hona, C. E McGrath, C. Giuri, C. J. Hailey (NuSTAR Collaboration, D. A. Williams, D. Hanna, D. Kieda, D. Ribeiro, E. Pueschel, E. Roache, G. H. Sembroski, G. Maier, G. M Foote, H. An, J. H. Buckley, J. Holder, J. Kim, J. L. Ryan, J. P. Halpern, J. Quinn, K. A Farrell, K. Mori, K. Pfrang, K. Ragan, L. Fortson, M. Capasso, MDM) C. B. Adams, M. Errando, M. J. Lang, M. Kertzman, M. Nievas-Rosillo, M. Pohl, M. Santander, N. Park, O. Hervet, P. Kaaret, P. Moriarty, P. T. Reynolds, R. A. Ong, R. Mukherjee, R. R. Prado, S. O'Brien, S. Patel, S. Schlenstedt, T. B. Humensky, T. Hassan, T. J Williamson (VERITAS collaboration), W. Benbow, W. Jin, Y. M. Tokayer","submitted_at":"2021-10-03T19:16:31Z","abstract_excerpt":"HESS J0632+057 belongs to a rare subclass of binary systems which emits gamma-rays above 100 GeV. 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