Zobrazeno 1 - 10
of 118
pro vyhledávání: '"Ulmer, Melville P."'
Autor:
Durret, Florence, Marquez, Isabel, Acebron, Ana, Adami, Christophe, Cabrera-Lavers, Antonio, Capelato, Hugo, Martinet, Nicolas, Sarron, Florian, Ulmer, Melville P.
Publikováno v:
A&A 588, A69 (2016)
Clusters of galaxies are at the intersection of cosmic filaments and are still accreting galaxies and groups along these preferential directions, but, because of their relatively low contrast on the sky, they are difficult to detect (unless a large a
Externí odkaz:
http://arxiv.org/abs/1601.07694
Autor:
Morawe, Christian, Mimura, Hidekazu, Khounsary, Ali M., Ulmer, Melville P., Capoot, Connor J., Assoufid, Lahsen, Quispe, Daniel, Buchholz, Donald B., Chung, Yip-Wah, Cao, Jian
Publikováno v:
Proceedings of SPIE; October 2024, Vol. 13150 Issue: 1 p131500D-131500D-7, 1183508p
Autor:
Durret, Florence, Adami, Christophe, Bertin, Emmanuel, Hao, Jiangang, Marquez, Isabel, Martinet, Nicolas, Maurogordato, Sophie, Sauvaget, Tabatha, Scepi, Nicolas, Takey, Ali, Ulmer, Melville P.
Based on a recent photometric redshift galaxy catalogue, we have searched for galaxy clusters in the Stripe~82 region of the Sloan Digital Sky Survey by applying the Adami & MAzure Cluster FInder (AMACFI). Extensive tests were made to fine-tune the A
Externí odkaz:
http://arxiv.org/abs/1504.00452
Autor:
Maksym, W. Peter, Ulmer, Melville, Roth, Kathy, Irwin, Jimmy, Dupke, Renato, Ho, Luis, Keel, William, Adami, Christophe
A likely tidal disruption of a star by the intermediate-mass black hole (IMBH) of a dwarf galaxy was recently identified in association with Abell 1795. Without deep spectroscopy for this very faint object, however, the possibility of a more massive
Externí odkaz:
http://arxiv.org/abs/1407.6737
Autor:
Pilachowski, Caty, Badenes, Carles, Bailey, Stephen, Barth, Aaron, Beaton, Rachel, Bell, Eric, Bernstein, Rebecca, Bian, Fuyan, Blanton, Michael, Blum, Robert, Bolton, Adam, Bond, Howard, Brodwin, Mark, Bullock, James, Carlin, Jeff, Chary, Ranga-Ram, Cinabro, David, Cooper, Michael, Cota, Jorge L. C., Davis, Marc, Dawson, Kyle, Dey, Arjun, Donahue, Megan, Drake, Jeremy, Ellingson, Erica, Faccioli, Lorenzo, Fan, Xiaohui, Ferguson, Harry, Gawiser, Eric, Geha, Marla, Giavalisco, Mauro, Gonzalez, Anthony, Griest, Kim, Grossan, Bruce, Guhathakurta, Raja, Harding, Paul, Heap, Sara R., Ho, Shirley, Howell, Steve, Jannuzi, Buell, Kalirai, Jason, Keeney, Brian, Kewley, Lisa, Kong, Xu, Lampton, Michael, Lin, Wei-Peng, de la Macorra, Axel, Macri, Lucas, Majewski, Steve, Martini, Paul, Massey, Phil, McSwain, Virginia, Miller, Adam A., Minniti, Dante, Modjaz, Maryam, Morrison, Heather, Moustakas, John, Myers, Adam, Najita, Joan, Newman, Jeffrey, Norman, Dara, Olsen, Knut, Pierce, Michael, Pope, Alexandra, Prescott, Moire, Reddy, Naveen, Reil, Kevin, Rest, Armin, Rhode, Katherine, Rockosi, Connie, Rudnick, Greg, Saha, Abhijit, Salzer, John, Sanders, David, Schlegel, David, Sesar, Branimir, Shields, Joseph, Silverman, Jeffrey, Simon, Josh, Stanford, Adam, Stern, Daniel, Storrie-Lombardi, Lisa, Suntzeff, Nicholas, Surace, Jason, Szalay, Alex, Ulmer, Melville, Weiner, Ben, Willman, Beth, Windhorst, Rogier, Wood-Vasey, Michael
This document summarizes the results of a community-based discussion of the potential science impact of the Mayall+BigBOSS highly multiplexed multi-object spectroscopic capability. The KPNO Mayall 4m telescope equipped with the DOE- and international
Externí odkaz:
http://arxiv.org/abs/1211.0285
Detailed temperature and abundance radial profile maps have revealed a significant lack of homogeneity within the Perseus Galaxy cluster. Previous surveys of Perseus with the Suzaku telescope, which has a worse angular resolution and less light colle
Externí odkaz:
http://arxiv.org/abs/1210.1253
Cluster faint low surface brightness galaxies (fLSBs) are difficult to observe. Consequently, their origin, physical properties and number density are not well known. After a first search for fLSBs in the highly substructured Coma cluster, we present
Externí odkaz:
http://arxiv.org/abs/1101.4136
Theory suggests that a star making a close passage by a supermassive black hole at the center of a galaxy can under most circumstances be expected to emit a giant flare of radiation as it is disrupted and a portion of the resulting stream of shock-he
Externí odkaz:
http://arxiv.org/abs/1008.4140
Autor:
Gavazzi, Raphael, Adami, Christophe, Durret, Florence, Cuillandre, Jean-Charles, Ilbert, Olivier, Mazure, Alain, Pello, Roser, Ulmer, Melville P.
Due to observational constraints, dark matter determinations in nearby clusters based on weak lensing are still extremely rare, in spite of their importance for the determination of cluster properties independent of other methods. We present a weak l
Externí odkaz:
http://arxiv.org/abs/0904.0220
We report results from an X-ray study of the Abell 2111 galaxy cluster using the Advanced Satellite for Astrophysics and Cosmology ASCA and the ROSAT Position Sensitive Proportional Counter (PSPC). By correcting for the energy-dependent point-spread
Externí odkaz:
http://arxiv.org/abs/astro-ph/9903194