Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Papovich, Casey J."'
Autor:
Fang, Jerome J., Faber, S. M., Koo, David C., Rodriguez-Puebla, Aldo, Guo, Yicheng, Barro, Guillermo, Behroozi, Peter, Brammer, Gabriel, Chen, Zhu, Dekel, Avishai, Ferguson, Henry C., Gawiser, Eric, Giavalisco, Mauro, Kartaltepe, Jeyhan, Kocevski, Dale D., Koekemoer, Anton M., McGrath, Elizabeth J., McIntosh, Daniel, Newman, Jeffrey A., Pacifici, Camilla, Pandya, Viraj, Perez-Gonzalez, Pablo G., Primack, Joel R., Salmon, Brett, Trump, Jonathan R., Weiner, Benjamin, Willner, S. P., Acquaviva, Viviana, Dahlen, Tomas, Finkelstein, Steven L., Finlator, Kristian, Fontana, Adriano, Galametz, Audrey, Grogin, Norman A., Gruetzbauch, Ruth, Johnson, Seth, Mobasher, Bahram, Papovich, Casey J., Pforr, Janine, Salvato, Mara, Santini, P., van der Wel, Arjen, Wiklind, Tommy, Wuyts, Stijn
This is the first in a series of papers examining the demographics of star-forming galaxies at $0.2
Externí odkaz:
http://arxiv.org/abs/1710.05489
Autor:
Tran, Kim-Vy H., Nanayakkara, Themiya, Yuan, Tiantian, Kacprzak, Glenn G., Glazebrook, Karl, Kewley, Lisa J., Momcheva, Ivelina, Papovich, Casey J., Quadri, Ryan, Rudnick, Greg, Saintonge, Amélie, Spitler, Lee R., Straatman, Caroline, Tomczak, Adam
We spectroscopically survey the galaxy cluster XMM-LSS J02182-05102 (hereafter IRC 0218) using LRIS (optical) and MOSFIRE (near-infrared) on Keck I as part of the ZFIRE survey. IRC 0218 has a narrow redshift range of $1.612
Externí odkaz:
http://arxiv.org/abs/1508.03057
Autor:
Mobasher, Bahram, Dahlen, Tomas, Ferguson, Henry C., Acquaviva, Viviana, Barro, Guillermo, Finkelstein, Steven L., Fontana, Adriano, Gruetzbauch, Ruth, Johnson, Seth, Lu, Yu, Papovich, Casey J., Pforr, Janine, Salvato, Mara, Somerville, Rachel S., Wiklind, Tommy, Wuyts, Stijn, Ashby, Matthew L. N., Bell, Eric, Conselice, Christopher J., Dickinson, Mark E., Faber, Sandra M., Fazio, Giovanni, Finlator, Kristian, Galametz, Audrey, Gawiser, Eric, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Guo, Yicheng, Hathi, Nimish, Kocevski, Dale, Koekemoer, Anton M., Koo, David C., Newman, Jeffrey A., Reddy, Naveen, Santini, Paola, Wechsler, Risa H.
In this paper we perform a comprehensive study of the main sources of random and systematic errors in stellar mass measurement for galaxies using their Spectral Energy Distributions (SEDs). We use mock galaxy catalogs with simulated multi-waveband ph
Externí odkaz:
http://arxiv.org/abs/1505.01501
Autor:
Wong, Kenneth C., Tran, Kim-Vy H., Suyu, Sherry H., Momcheva, Ivelina G., Brammer, Gabriel B., Brodwin, Mark, Gonzalez, Anthony H., Halkola, Aleksi, Kacprzak, Glenn G., Koekemoer, Anton M., Papovich, Casey J., Rudnick, Gregory H.
We identify a strong lensing galaxy in the cluster IRC 0218 (also known as XMM-LSS J02182$-$05102) that is spectroscopically confirmed to be at $z=1.62$, making it the highest-redshift strong lens galaxy known. The lens is one of the two brightest cl
Externí odkaz:
http://arxiv.org/abs/1405.3661
Autor:
Koekemoer, Anton M., Faber, S. M., Ferguson, Henry C., Grogin, Norman A., Kocevski, Dale D., Koo, David C., Lai, Kamson, Lotz, Jennifer M., Lucas, Ray A., McGrath, Elizabeth J., Ogaz, Sara, Rajan, Abhijith, Riess, Adam G., Rodney, Steve A., Strolger, Louis, Casertano, Stefano, Castellano, Marco, Dahlen, Tomas, Dickinson, Mark, Dolch, Timothy, Fontana, Adriano, Giavalisco, Mauro, Grazian, Andrea, Guo, Yicheng, Hathi, Nimish P., Huang, Kuang-Han, van der Wel, Arjen, Yan, Hao-Jing, Acquaviva, Viviana, Almaini, David M. Alexander Omar, Ashby, Matthew L. N., Barden, Marco, Bell, Eric F., Bournaud, Frédéric, Brown, Thomas M., Caputi, Karina I., Cassata, Paolo, Challis, Peter, Chary, Ranga-Ram, Cheung, Edmond, Cirasuolo, Michele, Conselice, Christopher J., Cooray, Asantha Roshan, Croton, Darren J., Daddi, Emanuele, Davé, Romeel, de Mello, Duilia F., de Ravel, Loic, Dekel, Avishai, Donley, Jennifer L., Dunlop, James S., Dutton, Aaron A., Elbaz, David, Fazio, Giovanni G., Filippenko, Alex V., Finkelstein, Steven L., Frazer, Chris, Gardner, Jonathan P., Garnavich, Peter M., Gawiser, Eric, Gruetzbauch, Ruth, Hartley, Will G., Häussler, Boris, Herrington, Jessica, Hopkins, Philip F., Huang, Jia-Sheng, Jha, Saurabh, Johnson, Andrew, Kartaltepe, Jeyhan S., Khostovan, Ali Ahmad, Kirshner, Robert P., Lani, Caterina, Lee, Kyoung-Soo, Li, Weidong, Madau, Piero, McCarthy, Patrick J., McIntosh, Daniel H., McLure, Ross J., McPartland, Conor, Mobasher, Bahram, Moreira, Heidi, Mortlock, Alice, Moustakas, Leonidas A., Mozena, Mark, Nandra, Kirpal, Newman, Jeffrey A., Nielsen, Jennifer L., Niemi, Sami, Noeske, Kai G., Papovich, Casey J., Pentericci, Laura, Pope, Alexandra, Primack, Joel R., Ravindranath, Swara, Reddy, Naveen A., Renzini, Alvio, Rix, Hans-Walter, Robaina, Aday R., Rosario, David J., Rosati, Piero, Salimbeni, Sara, Scarlata, Claudia, Siana, Brian, Simard, Luc, Smidt, Joseph, Snyder, Diana, Somerville, Rachel S., Spinrad, Hyron, Straughn, Amber N., Telford, Olivia, Teplitz, Harry I., Trump, Jonathan R., Vargas, Carlos, Villforth, Carolin, Wagner, Cory R., Wandro, Pat, Wechsler, Risa H., Weiner, Benjamin J., Wiklind, Tommy, Wild, Vivienne, Wilson, Grant, Wuyts, Stijn, Yun, Min S.
This paper describes the Hubble Space Telescope imaging data products and data reduction procedures for the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS). This survey is designed to document the evolution of galaxies and black ho
Externí odkaz:
http://arxiv.org/abs/1105.3754
Autor:
Grogin, Norman A., Kocevski, Dale D., Faber, S. M., Ferguson, Henry C., Koekemoer, Anton M., Riess, Adam G., Acquaviva, Viviana, Alexander, David M., Almaini, Omar, Ashby, Matthew L. N., Barden, Marco, Bell, Eric F., Bournaud, Frédéric, Brown, Thomas M., Caputi, Karina I., Casertano, Stefano, Cassata, Paolo, Castellano, Marco, Challis, Peter, Chary, Ranga-Ram, Cheung, Edmond, Cirasuolo, Michele, Conselice, Christopher J., Cooray, Asantha Roshan, Croton, Darren J., Daddi, Emanuele, Dahlen, Tomas, Davé, Romeel, de Mello, Duília F., Dekel, Avishai, Dickinson, Mark, Dolch, Timothy, Donley, Jennifer L., Dunlop, James S., Dutton, Aaron A., Elbaz, David, Fazio, Giovanni G., Filippenko, Alexei V., Finkelstein, Steven L., Fontana, Adriano, Gardner, Jonathan P., Garnavich, Peter M., Gawiser, Eric, Giavalisco, Mauro, Grazian, Andrea, Guo, Yicheng, Hathi, Nimish P., Häussler, Boris, Hopkins, Philip F., Huang, Jia-Sheng, Huang, Kuang-Han, Jha, Saurabh W., Kartaltepe, Jeyhan S., Kirshner, Robert P., Koo, David C., Lai, Kamson, Lee, Kyoung-Soo, Li, Weidong, Lotz, Jennifer M., Lucas, Ray A., Madau, Piero, McCarthy, Patrick J., McGrath, Elizabeth J., McIntosh, Daniel H., McLure, Ross J., Mobasher, Bahram, Moustakas, Leonidas A., Mozena, Mark, Nandra, Kirpal, Newman, Jeffrey A., Niemi, Sami-Matias, Noeske, Kai G., Papovich, Casey J., Pentericci, Laura, Pope, Alexandra, Primack, Joel R., Rajan, Abhijith, Ravindranath, Swara, Reddy, Naveen A., Renzini, Alvio, Rix, Hans-Walter, Robaina, Aday R., Rodney, Steven A., Rosario, David J., Rosati, Piero, Salimbeni, Sara, Scarlata, Claudia, Siana, Brian, Simard, Luc, Smidt, Joseph, Somerville, Rachel S., Spinrad, Hyron, Straughn, Amber N., Strolger, Louis-Gregory, Telford, Olivia, Teplitz, Harry I., Trump, Jonathan R., van der Wel, Arjen, Villforth, Carolin, Wechsler, Risa H., Weiner, Benjamin J., Wiklind, Tommy, Wild, Vivienne, Wilson, Grant, Wuyts, Stijn, Yan, Hao-Jing, Yun, Min S.
The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) is designed to document the first third of galactic evolution, over the approximate redshift (z) range 8--1.5. It will image >250,000 distant galaxies using three separate c
Externí odkaz:
http://arxiv.org/abs/1105.3753
Autor:
Tran, Kim-Vy H., Papovich, Casey J., Saintonge, Amelie, Brodwin, Mark, Dunlop, James S., Farrah, Duncan, Finkelstein, Keely D., Finkelstein, Steven L., Lotz, Jennifer, McLure, Ross J., Momcheva, Ivelina, Willmer, Christopher N. A.
We measure the rest-frame colors (dust-corrected), infrared luminosities, star formation rates, and stellar masses of 92 galaxies in a Spitzer-selected cluster at z=1.62. By fitting spectral energy distributions (SEDs) to 10-band photometry (0.4 micr
Externí odkaz:
http://arxiv.org/abs/1005.5126
Autor:
Brand, Kate, Moustakas, John, Armus, Lee, Assef, Roberto J., Brown, Michael J. I., Cool, Richard R., Desai, Vandana, Dey, Arjun, Floc'h, Emeric Le, Jannuzi, Buell T., Kochanek, Christopher S., Melbourne, Jason, Papovich, Casey J., Soifer, B. T.
Publikováno v:
Astrophys.J.693:340-346,2009
Observations with the Spitzer Space Telescope have revealed a population of red-sequence galaxies with a significant excess in their 24-micron emission compared to what is expected from an old stellar population. We identify 900 red galaxies with 0.1
Externí odkaz:
http://arxiv.org/abs/0811.1398
Autor:
Younger, Joshua D., Huang, Jia-Sheng, Fazio, Giovanni G., Cox, Thomas J., Lai, Kamson, Hopkins, Philip F., Hernquist, Lars, Papovich, Casey J., Simard, Luc, Lin, Lihwai, Cheng, Yi-Wen, Yan, Haojin, Keres, Dusan, Shapley, Alice E.
We present the rest-frame ultraviolet through near infrared spectral energy distribution for an interacting Lyman break galaxy at a redshift z=4.42, the highest redshift merging system known with clearly resolved tidal features. The two objects in th
Externí odkaz:
http://arxiv.org/abs/0708.0835
Autor:
Stevans, Matthew, Finkelstein, Steven, Wold, Isak, Kawinwanichakij, Lalitwadee, Papovich, Casey J., Sherman, Sydney, Gebhardt, Karl, Jogee, Shardha, Ciardullo, Robin, Gronwall, Caryl, Gawiser, Eric J., Acquaviva, Viviana, Casey, Caitlin, Florez, Jonathan
We present the most-detailed probe yet into the impact of active galactic nuclei feedback on star formation by measuring the shape of the bright end of the galaxy UV luminosity function at z~4.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::509127b1b7bcb55d3a7c5db82ecf73c6