Search Results - "Tyson, Tony"

Maximizing the scientific return of Roman and Rubin with a joint wide-sky observing strategy by Bianco, Federica B, Blum, Robert, Connolly, Andrew, Graham, Melissa, Guy, Leanne, Ivezic, Zeljko, Ritz, Steve, Strauss, Michael A, Tyson, Tony

“…This work presents the case for a single-band LSST-matched depth Roman Community Survey over the footprint of the Vera C. Rubin Observatory Legacy Survey of…”
Get full text

Science-Driven Optimization of the LSST Observing Strategy by LSST Science Collaboration, Marshall, Phil, Anguita, Timo, Bianco, Federica B, Bellm, Eric C, Brandt, Niel, Clarkson, Will, Connolly, Andy, Gawiser, Eric, Jones, Lynne, Lochner, Michelle, Lund, Michael B, Mahabal, Ashish, Nidever, David, Olsen, Knut, Ridgway, Stephen, Rhodes, Jason, Shemmer, Ohad, Trilling, David, Vivas, Kathy, Walkowicz, Lucianne, Willman, Beth, Yoachim, Peter, Anderson, Scott, Antilogus, Pierre, Angus, Ruth, Arcavi, Iair, Awan, Humna, Biswas, Rahul, Bell, Keaton J, Bennett, David, Britt, Chris, Buzasi, Derek, Casetti-Dinescu, Dana I, Claver, Chuck, Cook, Kem, Davenport, James, Debattista, Victor, Digel, Seth, Doctor, Zoheyr, Firth, R. E, Foley, Ryan, Fong, Wen-fai, Galbany, Lluis, Giampapa, Mark, Gizis, John E, Graham, Melissa L, Grillmair, Carl, Gris, Phillipe, Haiman, Zoltan, Hartigan, Patrick, Hawley, Suzanne, Hlozek, Renee, Jha, Saurabh W, Johns-Krull, C, Kanbur, Shashi, Kalogera, Vassiliki, Kashyap, Vinay, Kasliwal, Vishal, Kessler, Richard, Kim, Alex, Kurczynski, Peter, Liu, Michael C, Malz, Alex, Margutti, Raffaella, Matheson, Tom, McEwen, Jason D, McGehee, Peregrine, Meibom, Soren, Meyers, Josh, Monet, Dave, Neilsen, Eric, Newman, Jeffrey, O'Dowd, Matt, Peiris, Hiranya V, Penny, Matthew T, Peters, Christina, Poleski, Radoslaw, Ponder, Kara, Richards, Gordon, Rho, Jeonghee, Rubin, David, Schmidt, Samuel, Schuhmann, Robert L, Shporer, Avi, Slater, Colin, Smith, Nathan, Soares-Santos, Marcelles, Strader, Jay, Strauss, Michael, Street, Rachel, Stubbs, Christopher, Sullivan, Mark, Szkody, Paula, Trimble, Virginia, Tyson, Tony, de Val-Borro, Miguel, Wagoner, Robert, Wood-Vasey, W. Michael, Zauderer, Bevin Ashley

“…The Large Synoptic Survey Telescope is designed to provide an unprecedented optical imaging dataset that will support investigations of our Solar System,…”
Get full text

Educating the Next Generation of Leading Scientists: Turning Ideas into Action by Wood-Vasey, Michael, Schulte-Ladbeck, Regina, Blair, William, Borne, Kirk, Clampin, Mark, Gatley, Ian, Graf, Paul, Ivezic, Zeljko, Magnier, Eugene, Mather, John, Stubbs, Christopher, Schweitzer, Andrea, Spadafora, Tony, Stahl, Phil, Tyson, Tony

“…The core of scientific research is turning new ideas into reality. From the school science fair to the search for the secrets of dark energy, high-quality…”
Get full text

Exploring Dark Energy with Next-Generation Photometric Redshift Surveys by Zhan, Hu, Albrecht, Andreas, Cooray, Asantha, Habib, Salman, Heavens, Alan, Heitmann, Katrin, Jain, Bhuvnesh, Jee, Myungkook J, Knox, Lloyd, Mandelbaum, Rachel, Newman, Jeff, Schmidt, Samuel, Scranton, Ryan, Strauss, Michael, Tyson, Tony, Verde, Licia, Wittman, David, Wood-Vasey, Michael

“…The coming decade will be an exciting period for dark energy research, during which astronomers will address the question of what drives the accelerated cosmic…”
Get full text

The Case for Deep, Wide-Field Cosmology by Scranton, Ryan, Albrecht, Andreas, Caldwell, Robert, Cooray, Asantha, Dore, Olivier, Habib, Salman, Heavens, Alan, Heitmann, Katrin, Jain, Bhuvnesh, Knox, Lloyd, Newman, Jeffrey A, Serra, Paolo, Song, Yong-Seon, Strauss, Michael, Tyson, Tony, Verde, Licia, Zhan, Hu

“…Much of the science case for the next generation of deep, wide-field optical/infrared surveys has been driven by the further study of dark energy. This is a…”
Get full text

The Normal Cluster Weak Lensing Survey: Mass Profiles and M/L Ratios of Eight Clusters at z=0.2 by Wittman, David, Dell'Antonio, Ian, Tyson, Tony, Bernstein, Gary, Fischer, Philippe, Smith, Deano

“…We present a survey of mass profiles and mass-to-light ratios of eight typical galaxy clusters at a common redshift (z ~ 0.2). We use weak gravitational…”
Get full text