Zobrazeno 1 - 10
of 93
pro vyhledávání: '"Jones, R Lynne"'
Autor:
Wagg, Tom, Juric, Mario, Yoachim, Peter, Kurlander, Jake, Cornwall, Sam, Moeyens, Joachim, Eggl, Siegfried, Jones, R. Lynne, Birtwhistle, Peter
We simulate and analyse the contribution of the Rubin Observatory Legacy Survey of Space and Time (LSST) to the rate of discovery of Near Earth Object (NEO) candidates, their submission rates to the NEO Confirmation page (NEOCP), and the resulting de
Externí odkaz:
http://arxiv.org/abs/2408.12517
Autor:
Abrams, Natasha S., Hundertmark, Markus P. G., Khakpash, Somayeh, Street, Rachel A., Jones, R. Lynne, Lu, Jessica R., Bachelet, Etienne, Tsapras, Yiannis, Moniez, Marc, Blaineauu, Tristan, Di Stefano, Rosanne, Makler, Martin, Varela, Anibal, Rabus, Markus
The Vera C. Rubin Legacy Survey of Space and Time will discover thousands of microlensing events across the Milky Way Galaxy, allowing for the study of populations of exoplanets, stars, and compact objects. It will reach deeper limiting magnitudes ov
Externí odkaz:
http://arxiv.org/abs/2309.15310
Autor:
Schwamb, Megan E., Jones, R. Lynne, Yoachim, Peter, Volk, Kathryn, Dorsey, Rosemary C., Opitom, Cyrielle, Greenstreet, Sarah, Lister, Tim, Snodgrass, Colin, Bolin, Bryce T., Inno, Laura, Bannister, Michele T., Eggl, Siegfried, Solontoi, Michael, Kelley, Michael S. P., Jurić, Mario, Lin, Hsing Wen, Ragozzine, Darin, Bernardinelli, Pedro H., Chesley, Steven R., Daylan, Tansu, Ďurech, Josef, Fraser, Wesley C., Granvik, Mikael, Knight, Matthew M., Lisse, Carey M., Malhotra, Renu, Oldroyd, William J., Thirouin, Audrey, Ye, Quanzhi
The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and Time (LSST) in early to mid-2025. This multi-band wide-field synoptic survey will transform our view of the solar system, with the discovery and monitoring of over 5 mi
Externí odkaz:
http://arxiv.org/abs/2303.02355
The Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) has the potential to measure parallaxes for thousands of nearby ultracool dwarfs, enabling improved measurements of the brown dwarf luminosity function. We develop a simple model
Externí odkaz:
http://arxiv.org/abs/2209.15053
Autor:
Lindberg, Christina Willecke, Huppenkothen, Daniela, Jones, R. Lynne, Bolin, Bryce T., Juric, Mario, Golkhou, V. Zach, Bellm, Eric C., Drake, Andrew J., Graham, Matthew J., Laher, Russ R., Mahabal, Ashish A., Masci, Frank J., Riddle, Reed, Shin, Kyung Min
In the era of wide-field surveys like the Zwicky Transient Facility and the Rubin Observatory's Legacy Survey of Space and Time, sparse photometric measurements constitute an increasing percentage of asteroid observations, particularly for asteroids
Externí odkaz:
http://arxiv.org/abs/2111.12596
Autor:
Bianco, Federica B., Ivezić, Željko, Jones, R. Lynne, Graham, Melissa L., Marshall, Phil, Saha, Abhijit, Strauss, Michael A., Yoachim, Peter, Ribeiro, Tiago, Anguita, Timo, Bauer, Franz E., Bellm, Eric C., Blum, Robert D., Brandt, William N., Brough, Sarah, Catelan, Màrcio, Clarkson, William I., Connolly, Andrew J., Gawiser, Eric, Gizis, John, Hlozek, Renee, Kaviraj, Sugata, Liu, Charles T., Lochner, Michelle, Mahabal, Ashish A., Mandelbaum, Rachel, McGehee, Peregrine, Neilsen Jr., Eric H., Olsen, Knut A. G., Peiris, Hiranya, Rhodes, Jason, Richards, Gordon T., Ridgway, Stephen, Schwamb, Megan E., Scolnic, Dan, Shemmer, Ohad, Slater, Colin T., Slosar, Anže, Smartt, Stephen J., Strader, Jay, Street, Rachel, Trilling, David E., Verma, Aprajita, Vivas, A. K., Wechsler, Risa H., Willman, Beth
Vera C. Rubin Observatory is a ground-based astronomical facility under construction, a joint project of the National Science Foundation and the U.S. Department of Energy, designed to conduct a multi-purpose 10-year optical survey of the southern hem
Externí odkaz:
http://arxiv.org/abs/2108.01683
Autor:
Moeyens, Joachim, Juric, Mario, Ford, Jes, Bektesevic, Dino, Connolly, Andrew J., Eggl, Siegfried, Ivezić, Željko, Jones, R. Lynne, Kalmbach, J. Bryce, Smotherman, Hayden
We present "Tracklet-less Heliocentric Orbit Recovery" (THOR), an algorithm for linking of observations of Solar System objects across multiple epochs that does not require intra-night tracklets or a predefined cadence of observations within a search
Externí odkaz:
http://arxiv.org/abs/2105.01056
Autor:
Lochner, Michelle, Scolnic, Dan, Almoubayyed, Husni, Anguita, Timo, Awan, Humna, Gawiser, Eric, Gontcho, Satya Gontcho A, Gris, Philippe, Huber, Simon, Jha, Saurabh W., Jones, R. Lynne, Kim, Alex G., Mandelbaum, Rachel, Marshall, Phil, Petrushevska, Tanja, Regnault, Nicolas, Setzer, Christian N., Suyu, Sherry H., Yoachim, Peter, Biswas, Rahul, Blaineau, Tristan, Hook, Isobel, Moniez, Marc, Neilsen, Eric, Peiris, Hiranya, Rothchild, Daniel, Stubbs, Christopher
Publikováno v:
ApJS 259 58, 2022
The generation-defining Vera C. Rubin Observatory will make state-of-the-art measurements of both the static and transient universe through its Legacy Survey for Space and Time (LSST). With such capabilities, it is immensely challenging to optimize t
Externí odkaz:
http://arxiv.org/abs/2104.05676
Autor:
Collaboration, Vera C. Rubin Observatory LSST Solar System Science, Jones, R. Lynne, Bannister, Michelle T., Bolin, Bryce T., Chandler, Colin Orion, Chesley, Steven R., Eggl, Siegfried, Greenstreet, Sarah, Holt, Timothy R., Hsieh, Henry H., Ivezić, Zeljko, Jurić, Mario, Kelley, Michael S. P., Knight, Matthew M., Malhotra, Renu, Oldroyd, William J., Sarid, Gal, Schwamb, Megan E., Snodgrass, Colin, Solontoi, Michael, Trilling, David E.
Vera C. Rubin Observatory will be a key facility for small body science in planetary astronomy over the next decade. It will carry out the Legacy Survey of Space and Time (LSST), observing the sky repeatedly in u, g, r, i, z, and y over the course of
Externí odkaz:
http://arxiv.org/abs/2009.07653
Autor:
Almoubayyed, Husni, Mandelbaum, Rachel, Awan, Humna, Gawiser, Eric, Jones, R. Lynne, Meyers, Joshua, Tyson, J. Anthony, Yoachim, Peter, Collaboration, The LSST Dark Energy Science
The LSST survey will provide unprecedented statistical power for measurements of dark energy. Consequently, controlling systematic uncertainties is becoming more important than ever. The LSST observing strategy will affect the statistical uncertainty
Externí odkaz:
http://arxiv.org/abs/2006.12538