Zobrazeno 1 - 10
of 400
pro vyhledávání: '"Lucas, Phillip"'
Autor:
Minniti, Dante, Saito, Roberto K., Gonzalez, Oscar A., Alonso-García, Javier, Rejkuba, Marina, Barbá, Rodolfo, Irwin, Mike, Kammers, Roberto, Lucas, Phillip W., Majaess, Daniel, Valenti, Elena
Publikováno v:
A&A 616, A26 (2018)
The windows of low extinction in the Milky Way (MW) plane are rare but important because they enable us to place structural constraints on the opposite side of the Galaxy, which has hitherto been done rarely. We use the near-infrared (near-IR) images
Externí odkaz:
http://arxiv.org/abs/1804.07785
Autor:
Endl, Michael, Caldwell, Douglas A., Barclay, Thomas, Huber, Daniel, Isaacson, Howard, Buchhave, Lars A., Brugamyer, Erik, Robertson, Paul, Cochran, William D., MacQueen, Phillip J., Havel, Mathieu, Lucas, Phillip, Howell, Steve B., Fischer, Debra, Quintana, Elisa, Ciardi, David R.
Hot Jupiter systems provide unique observational constraints for migration models in multiple systems and binaries. We report on the discovery of the Kepler-424 (KOI-214) two-planet system, which consists of a transiting hot Jupiter (Kepler-424b) in
Externí odkaz:
http://arxiv.org/abs/1409.8156
Autor:
Ivanov, Valentin D., Minniti, Dante, Hempel, Maren, Kurtev, Radostin, Toledo, Ignacio, Saito, Roberto K., Alonso-Garcia, Javier, Beamin, Juan Carlos, Borissova, Jura, Catelan, Marcio, Chene, Andre-Nicolas, Emerson, Jim, Gonzalez, Oscar A., Lucas, Phillip W., Martin, Eduardo L., Rejkuba, Marina, Gromadzki, Mariusz
[abridged] The severe crowding in the direction of the inner Milky Way suggests that the census of stars within a few tens of parsecs in that direction may not be complete. We search for new nearby objects companions of known high proper motion (HPM)
Externí odkaz:
http://arxiv.org/abs/1309.4301
Autor:
Endl, Michael, MacQueen, Phillip J., Cochran, William D., Brugamyer, Erik, Buchhave, Lars A., Rowe, Jason, Lucas, Phillip, Issacson, Howard, Bryson, Steve, Howell, Steve B., Fortney, Jonathan J., Hansen, Terese, Borucki, William J., Caldwell, Douglas, Christiansen, Jessie L., Ciardi, David R., Demory, Brice-Olivier, Everett, Mark, Ford, Eric B., Haas, Michael R., Holman, Matthew J., Horch, Elliot, Jenkins, Jon M., Koch, David J., Lissauer, Jack J., Machalek, Pavel, Still, Martin, Welsh, William F., Sanderfer, Dwight T., Seader, Shawn E., Smith, Jeffrey C., Thompson, Susan E., Twicken, Joseph D.
We report the discovery of Kepler-15b, a new transiting exoplanet detected by NASA's Kepler mission. The transit signal with a period of 4.94 days was detected in the quarter 1 (Q1) Kepler photometry. For the first time, we have used the High-Resolut
Externí odkaz:
http://arxiv.org/abs/1107.2596
Autor:
Lucas, Phillip Charles
Publikováno v:
Nova Religio: The Journal of Alternative and Emergent Religions, 2007 Aug . 11(1), 31-60.
Externí odkaz:
https://www.jstor.org/stable/10.1525/nr.2007.11.1.31
Autor:
Lucas, Phillip Charles
Publikováno v:
Nova Religio: The Journal of Alternative and Emergent Religions, 2007 May . 10(4), 8-16.
Externí odkaz:
https://www.jstor.org/stable/10.1525/nr.2007.10.4.8
Autor:
Lucas, Phillip Charles
Publikováno v:
Nova Religio: The Journal of Alternative and Emergent Religions, 2004 Nov . 8(2), 28-47.
Externí odkaz:
https://www.jstor.org/stable/10.1525/nr.2004.8.2.28
Autor:
Bozeman, John, Lucas, Phillip
Publikováno v:
Nova Religio: The Journal of Alternative and Emergent Religions, 1999 Apr . 2(2), 303-306.
Externí odkaz:
https://www.jstor.org/stable/10.1525/nr.1999.2.2.303
Autor:
Lucas, Phillip C.
Publikováno v:
Nova Religio: The Journal of Alternative and Emergent Religions, 1997 Oct . 1(1), 6-11.
Externí odkaz:
https://www.jstor.org/stable/10.1525/nr.1997.1.1.6
Autor:
Crevier, Lucas Phillip
[THE PROBLEM] For a model’s development and the associated time and monetary commitment to be warranted, its function and output must be accepted by policy makers and other stakeholders. It is challenging to develop computational models that are at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bbfe7240a32cb046afea2d4206cb4b8b