Zobrazeno 1 - 10
of 104
pro vyhledávání: '"Stanford, S. Adam"'
Autor:
Alberts, Stacey, Pope, Alexandra, Brodwin, Mark, Chung, Sun Mi, Cybulski, Ryan, Dey, Arjun, Eisenhardt, Peter R. M., Galametz, Audrey, Gonzalez, Anthony H., Jannuzi, Buell T., Stanford, S. Adam, Snyder, Gregory F., Stern, Daniel, Zeimann, Gregory R.
We present a detailed, multi-wavelength study of star formation (SF) and active galactic nucleus (AGN) activity in 11 near-infrared (IR) selected, spectroscopically confirmed massive (greater than or similar to 10(14)M(circle dot)) galaxy clusters at
Externí odkaz:
http://hdl.handle.net/10150/621395
http://arizona.openrepository.com/arizona/handle/10150/621395
http://arizona.openrepository.com/arizona/handle/10150/621395
Autor:
Decker, Bandon, Brodwin, Mark, Saha, Ripon, Connor, Thomas, Eisenhardt, Peter R. M., Gonzalez, Anthony H., Moravec, Emily, Muhibullah, Mustafa, Stanford, S. Adam, Stern, Daniel, Thongkham, Khunanon, Wylezalek, Dominika, Dicker, Simon R., Mason, Brian, Mroczkowski, Tony, Romero, Charles E., Ruppin, Florian
We present stellar mass fractions and composite luminosity functions (LFs) for a sample of \Ncl\ clusters from the Massive and Distant Clusters of WISE Survey (MaDCoWS) at a redshift range of $0.951 \leq z \leq 1.43$. Using SED fitting of optical and
Externí odkaz:
http://arxiv.org/abs/2112.12239
Autor:
Marocco, Federico, Eisenhardt, Peter R. M., Fowler, John W., Kirkpatrick, J. Davy, Meisner, Aaron M., Schlafly, Edward F., Stanford, S. Adam, Garcia, Nelson, Caselden, Dan, Cushing, Michael C., Cutri, Roc M., Faherty, Jacqueline K., Gelino, Christopher R., Gonzalez, Anthony H., Jarrett, Thomas H., Koontz, Renata, Mainzer, Amanda, Marchese, Elijah J., Mobasher, Bahram, Schlegel, David J., Stern, Daniel, Teplitz, Harry I., Wright, Edward L.
The CatWISE2020 Catalog consists of 1,890,715,640 sources over the entire sky selected from WISE and NEOWISE survey data at 3.4 and 4.6 $\mu$m (W1 and W2) collected from 2010 Jan. 7 to 2018 Dec. 13. This dataset adds two years to that used for the Ca
Externí odkaz:
http://arxiv.org/abs/2012.13084
Autor:
Eisenhardt, Peter R. M., Marocco, Federico, Fowler, John W., Meisner, Aaron M., Kirkpatrick, J. Davy, Garcia, Nelson, Jarrett, Thomas H., Koontz, Renata, Marchese, Elijah J., Stanford, S. Adam, Caselden, Dan, Cushing, Michael C., Cutri, Roc M., Faherty, Jacqueline K., Gelino, Christopher R., Gonzalez, Anthony H., Mainzer, Amanda, Mobasher, Bahram, Schlegel, David J., Stern, Daniel, Teplitz, Harry I., Wright, Edward L.
CatWISE is a program to catalog sources selected from combined ${\it WISE}$ and ${\it NEOWISE}$ all-sky survey data at 3.4 and 4.6 $\mu$m (W1 and W2). The CatWISE Preliminary Catalog consists of 900,849,014 sources measured in data collected from 201
Externí odkaz:
http://arxiv.org/abs/1908.08902
Autor:
Masters, Daniel C., Stern, Daniel K., Cohen, Judith G., Capak, Peter L., Stanford, S. Adam, Hernitschek, Nina, Galametz, Audrey, Davidzon, Iary, Rhodes, Jason D., Sanders, Dave, Mobasher, Bahram, Castander, Francisco, Pruett, Kerianne, Fotopoulou, Sotiria
The Complete Calibration of the Color-Redshift Relation (C3R2) survey is a multi-institution, multi-instrument survey that aims to map the empirical relation of galaxy color to redshift to i~24.5 (AB), thereby providing a firm foundation for weak len
Externí odkaz:
http://arxiv.org/abs/1904.06394
Autor:
Gonzalez, Anthony H., Gettings, Daniel P., Brodwin, Mark, Eisenhardt, Peter R. M., Stanford, S. Adam, Wylezalek, Dominika, Decker, Bandon, Marrone, Daniel P., Moravec, Emily, O'Donnell, Christine, Stalder, Brian, Stern, Daniel, Abdulla, Zubair, Brown, Gillen, Carlstrom, John, Chambers, Kenneth C., Hayden, Brian, Lin, Yen-Ting, Magnier, Eugene, Masci, Frank, Mantz, Adam B., McDonald, Michael, Mo, Wenli, Perlmutter, Saul, Wright, Edward L., Zeimann, Gregory R.
We present the Massive and Distant Clusters of WISE Survey (MaDCoWS), a search for galaxy clusters at 0.7
Externí odkaz:
http://arxiv.org/abs/1809.06820
Autor:
Rubin, David, Hayden, Brian, Huang, Xiaosheng, Aldering, Greg, Amanullah, Rahman, Barbary, Kyle, Boone, Kyle, Brodwin, Mark, Deustua, Susana E., Dixon, Sam, Eisenhardt, Peter, Fruchter, Andrew S., Gonzalez, Anthony H., Goobar, Ariel, Gupta, Ravi R., Hook, Isobel, Jee, M. James, Kim, Alex G., Kowalski, Marek, Lidman, Chris E., Linder, Eric, Luther, Kyle, Nordin, Jakob, Pain, Reynald, Perlmutter, Saul, Raha, Zachary, Rigault, Mickael, Ruiz-Lapuente, Pilar, Saunders, Clare M., Sofiatti, Caroline, Spadafora, Anthony L., Stanford, S. Adam, Stern, Daniel, Suzuki, Nao, Williams, Steven C.
We present the discovery and measurements of a gravitationally lensed supernova (SN) behind the galaxy cluster MOO J1014+0038. Based on multi-band Hubble Space Telescope and Very Large Telescope (VLT) photometry of the supernova, and VLT spectroscopy
Externí odkaz:
http://arxiv.org/abs/1707.04606
Autor:
Alberts, Stacey, Pope, Alexandra, Brodwin, Mark, Chung, Sun Mi, Cybulski, Ryan, Dey, Arjun, Eisenhardt, Peter, Galametz, Audrey, Gonzalez, Anthony, Jannuzi, Buell, Stanford, S. Adam, Snyder, Gregory, Stern, Daniel, Zeimann, Gregory
We present a detailed, multi-wavelength study of star formation (SF) and AGN activity in 11 near-infrared (IR) selected, spectroscopically confirmed, massive ($\gtrsim10^{14}\,\rm{M_{\odot}}$) galaxy clusters at $1
Externí odkaz:
http://arxiv.org/abs/1604.03564
Autor:
Tsai, Chao-Wei, Eisenhardt, Peter, Wu, Jingwen, Stern, Daniel, Assef, Roberto, Blain, Andrew, Bridge, Carrie, Benford, Dominic, Cutri, Roc, Griffith, Roger, Jarrett, Thomas, Lonsdale, Carol, Masci, Frank, Moustakas, Leonidas, Petty, Sara, Sayers, Jack, Stanford, S. Adam, Wright, Edward, Yan, Lin, Leisawitz, David, Liu, Fengchuan, Mainzer, Amy, McLean, Ian, Padgett, Deborah, Skrutskie, Michael, Gelino, Christopher, Beichman, Charles, Juneau, Stéphanie
We present 20 WISE-selected galaxies with bolometric luminosities L_bol > 10^14 L_sun, including five with infrared luminosities L_IR = L(rest 8-1000 micron) > 10^14 L_sun. These "extremely luminous infrared galaxies," or ELIRGs, were discovered usin
Externí odkaz:
http://arxiv.org/abs/1410.1751
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