Variation of the nebular dust attenuation curve with the properties of local star-forming galaxies von Rezaee, Saeed, Reddy, Naveen, Shivaei, Irene, Fetherolf, Tara, Emami, Najmeh, Khostovan, A A

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Evolution of the H β + [O iii] and [O ii] luminosity functions and the [O ii] star formation history of the Universe up to z ∼ 5 from HiZELS von Khostovan, A. A., Sobral, D., Mobasher, B., Best, P. N., Smail, I., Stott, J. P., Hemmati, S., Nayyeri, H.

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CANDELS MULTI-WAVELENGTH CATALOGS: SOURCE IDENTIFICATION AND PHOTOMETRY IN THE CANDELS COSMOS SURVEY FIELD von Nayyeri, H., Hemmati, S., Mobasher, B., Ferguson, H. C., Cooray, A., Barro, G., Faber, S. M., Dickinson, M., Koekemoer, A. M., Peth, M., Salvato, M., Ashby, M. L. N., Darvish, B., Donley, J., Durbin, M., Finkelstein, S., Fontana, A., Grogin, N. A., Gruetzbauch, R., Huang, K., Khostovan, A. A., Kocevski, D., Kodra, D., Lee, B., Newman, J., Pacifici, C., Pforr, J., Stefanon, M., Wiklind, T., Willner, S. P., Wuyts, S., Castellano, M., Conselice, C., Dolch, T., Dunlop, J. S., Galametz, A., Hathi, N. P., Lucas, R. A., Yan, H.

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Evolution of H α equivalent widths from z ∼ 0.4 - 2.2: implications for star formation and legacy surveys with Roman and Euclid von Khostovan, A A, Malhotra, S, Rhoads, J E, Sobral, D, Harish, S, Tilvi, V, Coughlin, A, Rezaee, S

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The clustering of typical Ly α emitters from z ∼ 2.5–6: host halo masses depend on Ly α and UV luminosities von Khostovan, A A, Sobral, D, Mobasher, B, Matthee, J, Cochrane, R K, Chartab, N, Jafariyazani, M, Paulino-Afonso, A, Santos, S, Calhau, J

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The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ∼ 2 to z ∼ 6 von Santos, S, Sobral, D, Butterworth, J, Paulino-Afonso, A, Ribeiro, B, da Cunha, E, Calhau, J, Khostovan, A A, Matthee, J, Arrabal Haro, P

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A Large, Deep 3 Deg2 Survey of Hα, [OIII], and [OII] Emitters from LAGER: Constraining Luminosity Functions von Khostovan, A A, Malhotra, S, Rhoads, J E, Jiang, C., Wang, J., Wold, I, Zheng, Z.-Y., Barrientos, L. F., Coughlin, A., Harish, S., Hu, W., Infante, L., Perez, L. A., Pharo, J, Valdes, F., Walker, A. R., Yang, H

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Correlations between H α equivalent width and galaxy properties at z = 0.47: Physical or selection-driven? von Khostovan, A A, Malhotra, S, Rhoads, J E, Harish, S, Jiang, C, Wang, J, Wold, I, Zheng, Z-Y, Barrientos, L F, Coughlin, A, Hu, W, Infante, L, Perez, L A, Pharo, J, Valdes, F, Walker, A R

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The clustering of H β + [O iii] and [O ii] emitters since z ∼ 5: dependencies with line luminosity and stellar mass von Khostovan, A A, Sobral, D, Mobasher, B, Best, P N, Smail, I, Matthee, J, Darvish, B, Nayyeri, H, Hemmati, S, Stott, J P

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Slicing COSMOS with SC4K: the evolution of typical Ly α emitters and the Ly α escape fraction from z ∼ 2 to 6 von Sobral, David, Santos, Sérgio, Matthee, Jorryt, Paulino-Afonso, Ana, Ribeiro, Bruno, Calhau, João, Khostovan, Ali A

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The Interstellar Medium in [O iii]-selected Star-forming Galaxies at z ∼ 3.2 von Suzuki, Tomoko L., Kodama, Tadayuki, Onodera, Masato, Shimakawa, Rhythm, Hayashi, Masao, Tadaki, Ken-ichi, Koyama, Yusei, Tanaka, Ichi, Sobral, David, Smail, Ian, Best, Philip N., Khostovan, Ali A., Minowa, Yosuke, Yamamoto, Moegi

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Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses von Amblard, Alexandre, Cooray, Asantha, Serra, Paolo, Altieri, B, Arumugam, V, Aussel, H, Blain, A, Bock, J, Boselli, A, Buat, V, Castro-Rodríguez, N, Cava, A, Chanial, P, Chapin, E, Clements, D L, Conley, A, Conversi, L, Dowell, C D, Dwek, E, Eales, S, Elbaz, D, Farrah, D, Franceschini, A, Gear, W, Glenn, J, Griffin, M, Halpern, M, Hatziminaoglou, E, Ibar, E, Isaak, K, Ivison, R J, Khostovan, A A, Lagache, G, Levenson, L, Lu, N, Madden, S, Maffei, B, Mainetti, G, Marchetti, L, Marsden, G, Mitchell-Wynne, K, Nguyen, H T, O'Halloran, B, Oliver, S J, Omont, A, Page, M J, Panuzzo, P, Papageorgiou, A, Pearson, C P, Pérez-Fournon, I, Pohlen, M, Rangwala, N, Roseboom, I G, Rowan-Robinson, M, Portal, M Sánchez, Schulz, B, Scott, Douglas, Seymour, N, Shupe, D L, Smith, A J, Stevens, J A, Symeonidis, M, Trichas, M, Tugwell, K, Vaccari, M, Valiante, E, Valtchanov, I, Vieira, J D, Vigroux, L, Wang, L, Ward, R, Wright, G, Xu, C K, Zemcov, M

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The nature of Hβ+[O iii] and [O ii] emitters to z ∼ 5 with HiZELS: stellar mass functions and the evolution of EWs von Khostovan, A A, Sobral, D, Mobasher, B, Smail, I, Darvish, B, Nayyeri, H, Hemmati, S, Stott, J P

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HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements von Cooray, A., Amblard, A., Wang, L., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chanial, P., Clements, D. L., Conley, A., Conversi, L., Dowell, C. D., Dwek, E., Eales, S., Elbaz, D., Farrah, D., Fox, M., Franceschini, A., Gear, W., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Khostovan, A. A., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Marsden, G., Mitchell-Wynne, K., Mortier, A. M. J., Nguyen, H. T., O'Halloran, B., Oliver, S. J., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Perez Fournon, I., Pohlen, M., Rawlings, J. I., Raymond, G., Rigopoulou, D., Rizzo, D., Roseboom, I. G., Rowan-Robinson, M., Schulz, B., Scott, D., Serra, P., Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vieira, J. D., Vigroux, L., Ward, R., Wright, G., Xu, C. K., Zemcov, M.

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MIGHTEE-H i: H i galaxy properties in the large-scale structure environment at z ∼ 0.37 from a stacking experiment von Sinigaglia, Francesco, Rodighiero, Giulia, Elson, Ed, Bianchetti, Alessandro, Vaccari, Mattia, Maddox, Natasha, Ponomareva, Anastasia A, Frank, Bradley S, Jarvis, Matt J, Catinella, Barbara, Cortese, Luca, Roychowdhury, Sambit, Baes, Maarten, Collier, Jordan D, Ilbert, Olivier, Khostovan, Ali A, Kurapati, Sushma, Pan, Hengxing, Prandoni, Isabella, Rajohnson, Sambatriniaina H A, Salvato, Mara, Sekhar, Srikrishna, Sharma, Gauri

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SPITZER -IRAC IDENTIFICATION OF HERSCHEL -ATLAS SPIRE SOURCES von Kim, Sam, Wardlow, Julie L, Cooray, Asantha, Fleuren, S, Sutherland, W, KHOSTOVAN, A A, Auld, R, Baes, M, Bussmann, R S, BUTTIGLIONE, S

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Spitzer Imaging of Herschel-atlas Gravitationally Lensed Submillimeter Sources von Hopwood, R, Wardlow, J, Cooray, A, Khostovan, A. A, Kim, S, Negrello, M, da Cunha, E, Burgarella, D, Aretxaga, I, Auld, R, Baes, M, Barton, E, Bertoldi, F, Bonfield, D. G, Blundell, R, Buttiglione, S, Cava, A, Clements, D. L, Cooke, J, Dannerbauer, H, Dariush, A, de Zotti, G, Dunlop, J, Dunne, L, Dye, S, Eales, S, Fritz, J, Frayer, D, Gurwell, M. A, Hughes, D. H, Ibar, E, Ivison, R. J, Jarvis, M. J, Lagache, G, Leeuw, L, Maddox, S, Michałowski, M. J, Omont, A, Pascale, E, Pohlen, M, Rigby, E, Rodighiero, G, Scott, D, Serjeant, S, Smail, I, Smith, D. J. B, Temi, P, Thompson, M. A, Valtchanov, I, van der Werf, P, Verma, A, Vieira, J. D

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Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10 11 solar masses von Amblard, Alexandre, Cooray, Asantha, Serra, Paolo, Altieri, B., Arumugam, V., Aussel, H., Blain, A., Bock, J., Boselli, A., Buat, V., Castro-Rodríguez, N., Cava, A., Chanial, P., Chapin, E., L. Clements, D., Conley, A., Conversi, L., D. Dowell, C., Dwek, E., Eales, S., Elbaz, D., Farrah, D., Franceschini, A., Gear, W., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., J. Ivison, R., A. Khostovan, A., Lagache, Guilaine, Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Marsden, G., Mitchell-Wynne, K., T. Nguyen, H., O'Halloran, B., J. Oliver, S., Omont, A., J. Page, M., Panuzzo, P., Papageorgiou, A., P. Pearson, C., Pérez-Fournon, I., Pohlen, M., Rangwala, N., G. Roseboom, I., Rowan-Robinson, M., Sánchez Portal, M., Schulz, B., Scott, Douglas, Seymour, N., L. Shupe, D., J. Smith, A., A. Stevens, J., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valiante, E., Valtchanov, I., D. Vieira, J., Vigroux, L., Wang, L., Ward, R., Wright, Gavin, K. Xu, C., Zemcov, M.

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[O iii] emission line as a tracer of star-forming galaxies at high redshifts: comparison between Hα and [O iii] emitters at z=2.23 in HiZELS von Suzuki, T. L., Kodama, T., Sobral, D., Khostovan, A. A., Hayashi, M., Shimakawa, R., Koyama, Y., Tadaki, K.-i., Tanaka, I., Minowa, Y., Yamamoto, M., Smail, I., Best, P. N.

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The nature of H[Beta]+[O III] and [O II] emitters to z ~ 5 with HiZELS: stellar mass functions and the evolution of EWs von Khostovan, A A, Sobral, D, Mobasher, B, Smail, I, Darvish, B, Nayyeri, H, Hemmati, S, Stott, J P

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