Search Results - Rafelski, Marc
- Showing 1 - 2 results of 2
-
1
Clumpy galaxies in CANDELS. II. Physical properties of UV-bright clumps at 0.5 ≤ z < 3 by Guo, Yicheng, Rafelski, Marc, Bell, Eric F., Conselice, Christopher J., Dekel, Avishai, Faber, S. M., Giavalisco, Mauro, Koekemoer, Anton M., Koo, David C., Lu, Yu, Mandelker, Nir, Primack, Joel R., Ceverino, Daniel, de Mello, Duilia F., Ferguson, Henry C., Hathi, Nimish, Kocevski, Dale, Lucas, Ray A., Pérez-González, Pablo G., Ravindranath, Swara, Soto, Emmaris, Straughn, Amber, Wang, Weichen
Published 2018Get full text
-
2
Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0 by Mantha, Kameswara Bharadwaj, McIntosh, Daniel H., Brennan, Ryan, Ferguson, Henry C., Kodra, Dritan, Newman, Jeffrey A., Rafelski, Marc, Somerville, Rachel S., Conselice, Christopher J., Cook, Joshua S., Hathi, Nimish P., Koo, David C., Lotz, Jennifer M., Simmons, Brooke D., Straughn, Amber N., Snyder, Gregory F., Wuyts, Stijn, Bell, Eric F, Dekel, Avishai, Kartaltepe, Jeyhan, Kocevski, Dale D., Koekemoer, Anton M., Lee, Seong-Kook, Lucas, Ray A., Pacifici, Camilla, Peth, Michael A., Barro, Guillermo, Dahlen, Tomas, Finkelstein, Steven L., Fontana, Adriano, Galametz, Audrey, Grogin, Norman A., Guo, Yicheng, Mobasher, Bahram, Nayyeri, Hooshang, Pérez-González, Pablo G., Pforr, Janine, Santini, Paola, Stefanon, Mauro, Wiklind, Tommy
Published 2018Get full text