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- Werle, A., Giunchi, E., Poggianti, B., Gullieuszik, M., Moretti, A., Zanella, A., Tonnesen, S., Fritz, J., Vulcani, B., Bacchini, C., Akerman, N., Kulier, A., Tomicic, N., Smith, R., Wolter, A.The history of star-forming regions in the tails of six GASP jellyfish galaxies observed with the Hubble Space Telescope
- Paul, Sebouh, Brecelj, T., Arenhövel, H., Achenbach, P., Ashkenazi, A., Beričič, J., Böhm, R., Bosnar, Damir, Cohen, E.O., Debenjak, L., Distler, M.O., Esser, A., Friščić, Ivica, Gilman, R., Izraeli, D., Kolar, T., Korover, I., Lichtenstadt, J., Mardor, I., Merkel, H., Middleton, D.G., Mihovilovič, M., Müller, U., Olivenboim, M., Piasetzky, E., Pochodzalla, J., Ron, G., Schlimme, B.S., Schoth, M., Schulz, F., Sfienti, C., Širca, S., Štajner, S., Strauch, S., Thiel, M., Tyukin, A., Weber, A., Yaron, I.The influence of Fermi motion on the comparison of the polarization transfer to a proton in elastic e→p and quasi-elastic e→A scattering
- Kolanović, Marko, Pajić, DamirThe influence of domain structure on the variation of coercive field and maximum magnetization of Fe_77.5B_22.5 amorphous alloy
- Sabolek, StjepanThe influence of dynamic surface fields on the coercive field and energy loss of amorphous Co_70.3Fe_4.7Si_15B_10 ribbon
- Delvecchio, I., Daddi, E., Sargent, M. T., Jarvis, M. J., Elbaz, D., Jin, S., Liu, D., Whittam, I. H., Algera, H., Carraro, R., D’Eugenio, C., Delhaize, J., Kalita, B. S., Leslie, S., Molnár, D. Cs., Novak, M., Prandoni, I., Smolčić, V., Ao, Y., Aravena, M., Bournaud, F., Collier, J. D., Randriamampandry, S. M., Randriamanakoto, Z., Rodighiero, G., Schober, J., White, S. V., Zamorani, G.The infrared-radio correlation of star-forming galaxies is strongly M⋆-dependent but nearly redshift-invariant since z ∼ 4
- Molnár, Dániel Cs, Sargent, Mark T., Delhaize, Jacinta, Delvecchio, Ivan, Smolčić, Vernesa, Novak, Mladen, Schinnerer, Eva, Zamorani, Giovanni, Bondi, Marco, Herrera-Ruiz, Noelia, Murphy, Eric J., Vardoulaki, Eleni, Karim, Alexander, Leslie, Sarah, Magnelli, Benjamin, Carollo, C. Marcella, Middelberg, EnnoThe infrared–radio correlation of spheroid- and disc-dominated star-forming galaxies to z ∼ 1.5 in the COSMOS field
- Mioković, Željka, Veža, DamirThe line shape of sodium n^2S_1/2 -3^2 P_1/2;3/2 transitions in Na-Cd high pressure discharge
- Tkachenko, A., Pavlovski, Krešimir, Johnston, C., Pedersen, M. G., Michielsen, M., Bowman, D. M., Southworth, J., Tsymbal, V., Aerts, C.The mass discrepancy in intermediate- and high-mass eclipsing binaries: The need for higher convective core masses
- Novak, Maja, Polak, Bruno, Simunić, Juraj, Boban, Zvonimir, Kuzmić, Barbara, Thomae, Andreas W, Tolić, Iva Marija, Pavin, NenadThe mitotic spindle is chiral due to torques within microtubule bundles
- Sabolek, StjepanThe model for the magnetization of current carrying amorphous ferromagnets
- Lanzuisi, G., Pernar, Margareta, Delvecchio, I., Berta, S., Brusa, M., Cappelluti, N., Comastri, A., Gilli, R., Gruppioni, C., Mignoli, M., Pozzi, F., Vietri, G., Vignali, C., Zamorani, G.The most obscured AGN in the COSMOS field
- Bermuth, J., Merle, P, Carasco, C., Baumann, D., Böhm, D., Bosnar, Damir, Ding, M., Distler, M. O., Friedrich, J., Friedrich, J. M., Golak, J., Glockle, W., Hauger, M., Heil, W., Jennewein, P., Jourdan, J., Kamada, H., Klein, A., Kohl, M., Krusche, B., Krygier, K. W., Merkel, H., Muller, U., Neuhausen, R., Nogga, A., Normand, C., Otten, E., Pospischil, T., Potokar, M., Rohe, D., Schmieden, H., Schmiedeskamp, J., Seimetz, M., Sick, I., Sirca, S., Skibinski, R., Testa, G., Walcher, T., Warren, G., Weis, M., Witala, H., Wohrle, H., Zeier, M.The neutron charge form factor and target analyzing powers from 3He(e→,e′n) scattering
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