Zobrazeno 1 - 10
of 56
pro vyhledávání: '"Mancone, Conor"'
Autor:
Wagner, Cory R., Brodwin, Mark, Snyder, Gregory F., Gonzalez, Anthony H., Stanford, S. A., Alberts, Stacey, Pope, Alexandra, Stern, Daniel, Zeimann, Gregory R., Chary, Ranga-Ram, Dey, Arjun, Eisenhardt, Peter R. M., Mancone, Conor L., Moustakas, John
We measure the star formation rates (SFRs) of massive ($M_{\star}>10^{10.1}M_{\odot}$) early-type galaxies (ETGs) in a sample of 11 high-redshift ($1.0 < z < 1.5$) galaxy clusters drawn from the IRAC Shallow Cluster Survey (ISCS). We identify ETGs vi
Externí odkaz:
http://arxiv.org/abs/1412.6717
We present PyGFit, a program designed to measure PSF-matched photometry from images with disparate pixel scales and PSF sizes. While PyGFit has a number of uses, its primary purpose is to extract robust spectral energy distributions (SEDs) from crowd
Externí odkaz:
http://arxiv.org/abs/1310.6046
Autor:
Alberts, Stacey, Pope, Alexandra, Brodwin, Mark, Atlee, David W., Lin, Yen-Ting, Dey, Arjun, Eisenhardt, Peter R. M., Gettings, Daniel P., Gonzalez, Anthony H., Jannuzi, Buell T., Mancone, Conor L., Moustakas, John, Snyder, Gregory F., Stanford, S. Adam, Stern, Daniel, Weiner, Benjamin J., Zeimann, Gregory R.
We compare the star formation (SF) activity in cluster galaxies to the field from z=0.3-1.5 using $Herschel$ SPIRE 250$\mu$m imaging. We utilize 274 clusters from the IRAC Shallow Cluster Survey (ISCS) selected as rest-frame near-infrared overdensiti
Externí odkaz:
http://arxiv.org/abs/1310.6040
Autor:
Zeimann, Gregory, Stanford, S. A., Brodwin, Mark, Gonzalez, Anthony H., Mancone, Conor, Snyder, Gregory F., Stern, Daniel, Eisenhardt, Peter, Dey, Arjun, Moustakas, John
We present Hubble Space Telescope near-IR spectroscopy for 18 galaxy clusters at 1.0 < $z$ < 1.5 in the IRAC Shallow Cluster Survey. We use Wide Field Camera 3 grism data to spectroscopically identify H$\alpha$ emitters in both the cores of galaxy cl
Externí odkaz:
http://arxiv.org/abs/1310.6037
Autor:
Mancone, Conor, Baker, Troy, Gonzalez, Anthony H., Ashby, Matthew L. N., Stanford, Spencer A., Brodwin, Mark, Eisenhardt, Peter R. M., Snyder, Greg, Stern, Daniel, Wright, Edward L.
We measure the faint end slope of the galaxy luminosity function (LF) for cluster galaxies at 1
Externí odkaz:
http://arxiv.org/abs/1211.1664
Autor:
Zeimann, Gregory R., Stanford, S. A., Brodwin, Mark, Gonzalez, Anthony H., Snyder, Gregory F., Stern, Daniel, Eisenhardt, Peter, Mancone, Conor, Dey, Arjun
We report the discovery of an IR-selected galaxy cluster in the IRAC Distant Cluster Survey (IDCS). New data from the Hubble Space Telescope spectroscopically confirm IDCS J1433.2+3306 at z = 1.89 with robust spectroscopic redshifts for seven members
Externí odkaz:
http://arxiv.org/abs/1207.4793
Autor:
Snyder, Gregory F., Brodwin, Mark, Mancone, Conor M., Zeimann, Gregory R., Stanford, S. A., Gonzalez, Anthony H., Stern, Daniel, Eisenhardt, Peter R. M., Brown, Michael J. I., Dey, Arjun, Jannuzi, Buell, Perlmutter, Saul
Publikováno v:
Astrophys.J. 756 (2012) 114
We present results for the assembly and star formation histories of massive (~L*) red sequence galaxies in 11 spectroscopically confirmed, infrared-selected galaxy clusters at 1.0 < z < 1.5, the precursors to present-day massive clusters with M ~ 10^
Externí odkaz:
http://arxiv.org/abs/1207.4790
Autor:
Gettings, Daniel P., Gonzalez, Anthony H., Stanford, S. Adam, Eisenhardt, Peter R. M., Brodwin, Mark, Mancone, Conor, Stern, Daniel, Zeimann, Gregory R., Masci, Frank J., Papovich, Casey, Tanaka, Ichi, Wright, Edward L.
We present spectroscopic confirmation of a z=0.99 galaxy cluster discovered using data from the Wide-field Infrared Survey Explorer (WISE). This is the first z~1 cluster candidate from the Massive Distant Clusters of WISE Survey (MaDCoWS) to be confi
Externí odkaz:
http://arxiv.org/abs/1205.7092
Autor:
Gonzalez, Anthony H., Stanford, S. A., Brodwin, Mark, Fedeli, Cosimo, Dey, Arjun, Eisenhardt, Peter R. M., Mancone, Conor, Stern, Daniel, Zeimann, Greg
The galaxy cluster IDCS J1426.5+3508 at z = 1.75 is the most massive galaxy cluster yet discovered at z > 1.4 and the first cluster at this epoch for which the Sunyaev-Zel'Dovich effect has been observed. In this paper we report on the discovery with
Externí odkaz:
http://arxiv.org/abs/1205.3788
Autor:
Mancone, Conor, Gonzalez, Anthony
We present EzGal, a flexible python program designed to easily generate observable parameters (magnitudes, colors, mass-to-light ratios) for any stellar population synthesis (SPS) model. As has been demonstrated by various authors, the choice of inpu
Externí odkaz:
http://arxiv.org/abs/1205.0009