Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Thomas B Lowe"'
Autor:
WeiKang Zheng, Benjamin E Stahl, Thomas de Jaeger, Alexei V Filippenko, Shan-Qin Wang, Wen-Pei Gan, Thomas G Brink, Ivan Altunin, Raphael Baer-Way, Andrew Bigley, Kyle Blanchard, Peter K Blanchard, James Bradley, Samantha K Cargill, Chadwick Casper, Teagan Chapman, Vidhi Chander, Sanyum Channa, Byung Yun Choi, Nick Choksi, Matthew Chu, Kelsey I Clubb, Daniel P Cohen, Paul A Dalba, Asia deGraw, Maxime de Kouchkovsky, Michael Ellison, Edward Falcon, Ori D Fox, Kiera Fuller, Mohan Ganeshalingam, Nachiket Girish, Carolina Gould, Goni Halevi, Andrew Halle, Kevin T Hayakawa, Romain Hardy, Julia Hestenes, Andrew M Hoffman, Michael Hyland, Benjamin T Jeffers, Connor Jennings, Michael T Kandrashoff, Anthony Khodanian, Minkyu Kim, Haejung Kim, Michelle E Kislak, Daniel Krishnan, Sahana Kumar, Snehaa Ganesh Kumar, Joel Leja, Erin J Leonard, Gary Z Li, Weidong Li, Ji-Shun Lian, Evelyn Liu, Thomas B Lowe, Philip Lu, Emily Ma, Michelle N Mason, Michael May, Kyle McAllister, Emma McGinness, Shaunak Modak, Jeffrey Molloy, Yukei S Murakami, Omnarayani Nayak, Derek Perera, Kenia Pina, Druv Punjabi, Andrew Rikhter, Timothy W Ross, Jackson Sipple, Costas Soler, Samantha Stegman, Haynes Stephens, James Sunseri, Kevin Tang, Stephen Taylor, Patrick Thrasher, Schuyler D Van Dyk, Xiang-Gao Wang, Jeremy Wayland, Andrew Wilkins, Abel Yagubyan, Heechan Yuk, Sameen Yunus, Keto D Zhang
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 512, iss 3
We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c5ae515f803371e98f5e9dcf8e878042
https://resolver.caltech.edu/CaltechAUTHORS:20220525-91785000
https://resolver.caltech.edu/CaltechAUTHORS:20220525-91785000
Autor:
C. Agliozzo, Claudia P. Gutiérrez, Seppo Mattila, David Young, Eugene A. Magnier, Anders Jerkstrand, Lluís Galbany, Cosimo Inserra, C. Gonzalez, Nidia Morrell, Carlos Contreras, Stefano Valenti, Kate Maguire, T.-W. Chen, Mark E. Huber, Erkki Kankare, Thomas B. Lowe, Mark M. Phillips, Stephen Smartt, K. C. Chambers, S. Castellon, Jesper Sollerman, Morgan Fraser, Eric Hsiao, Santiago González-Gaitán, Thomas Krühler, Joseph P. Anderson, Luc Dessart, H. Flewelling, Griffin Hosseinzadeh, Maximilian Stritzinger, Mark Sullivan
Publikováno v:
Nature Astronomy
Nature Astronomy, Nature Publishing Group, 2018, 2 (7), pp.574-579. ⟨10.1038/s41550-018-0458-4⟩
Anderson, J P, Dessart, L, Gutiérrez, C P, Krühler, T, Galbany, L, Jerkstrand, A, Smartt, S J, Contreras, C, Morrell, N, Phillips, M M, Stritzinger, M D, Hsiao, E Y, González-Gaitán, S, Agliozzo, C, Castellón, S, Chambers, K C, Flewelling, H, Gonzalez, C, Hosseinzadeh, G, Huber, M, Fraser, M, Inserra, C, Kankare, E, Mattila, S, Magnier, E, Maguire, K, Lowe, T B, Sollerman, J, Sullivan, M, Young, D R & Valenti, S 2018, ' The lowest-metallicity type II supernova from the highest-mass red supergiant progenitor ', Nature Astronomy, vol. 2, pp. 574-579 . https://doi.org/10.1038/s41550-018-0458-4
Nature Astronomy, 2018, 2 (7), pp.574-579. ⟨10.1038/s41550-018-0458-4⟩
Anderson, J P, Dessart, L, Gutiérrez, C P, Krühler, T, Galbany, L, Jerkstrand, A, Smartt, S J, Contreras, C, Morrell, N, Phillips, M M, Stritzinger, M D, Hsiao, E Y, González-Gaitán, S, Agliozzo, C, Castellón, S, Chambers, K C, Chen, T-W, Flewelling, H, Gonzalez, C, Hosseinzadeh, G, Huber, M, Fraser, M, Inserra, C, Kankare, E, Mattila, S, Magnier, E, Maguire, K, Lowe, T B, Sollerman, J, Sullivan, M, Young, D R & Valenti, S 2018, ' The lowest-metallicity type II supernova from the highest-mass red supergiant progenitor ', Nature Astronomy, vol. 2, pp. 574-579 . https://doi.org/10.1038/s41550-018-0458-4
Nature Astronomy, Nature Publishing Group, 2018, 2 (7), pp.574-579. ⟨10.1038/s41550-018-0458-4⟩
Anderson, J P, Dessart, L, Gutiérrez, C P, Krühler, T, Galbany, L, Jerkstrand, A, Smartt, S J, Contreras, C, Morrell, N, Phillips, M M, Stritzinger, M D, Hsiao, E Y, González-Gaitán, S, Agliozzo, C, Castellón, S, Chambers, K C, Flewelling, H, Gonzalez, C, Hosseinzadeh, G, Huber, M, Fraser, M, Inserra, C, Kankare, E, Mattila, S, Magnier, E, Maguire, K, Lowe, T B, Sollerman, J, Sullivan, M, Young, D R & Valenti, S 2018, ' The lowest-metallicity type II supernova from the highest-mass red supergiant progenitor ', Nature Astronomy, vol. 2, pp. 574-579 . https://doi.org/10.1038/s41550-018-0458-4
Nature Astronomy, 2018, 2 (7), pp.574-579. ⟨10.1038/s41550-018-0458-4⟩
Anderson, J P, Dessart, L, Gutiérrez, C P, Krühler, T, Galbany, L, Jerkstrand, A, Smartt, S J, Contreras, C, Morrell, N, Phillips, M M, Stritzinger, M D, Hsiao, E Y, González-Gaitán, S, Agliozzo, C, Castellón, S, Chambers, K C, Chen, T-W, Flewelling, H, Gonzalez, C, Hosseinzadeh, G, Huber, M, Fraser, M, Inserra, C, Kankare, E, Mattila, S, Magnier, E, Maguire, K, Lowe, T B, Sollerman, J, Sullivan, M, Young, D R & Valenti, S 2018, ' The lowest-metallicity type II supernova from the highest-mass red supergiant progenitor ', Nature Astronomy, vol. 2, pp. 574-579 . https://doi.org/10.1038/s41550-018-0458-4
Red supergiants have been confirmed as the progenitor stars of the majority of hydrogen-rich type II supernovae. However, while such stars are observed with masses >25M$_\odot$, detections of >18M$_\odot$ progenitors remain elusive. Red supergiants a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70361d93b4bdb413859de996efae3f34
https://orca.cardiff.ac.uk/id/eprint/117991/1/1805.04434.pdf
https://orca.cardiff.ac.uk/id/eprint/117991/1/1805.04434.pdf
Autor:
Aleksandar Cikota, Giorgos Leloudas, Mattia Bulla, Cosimo Inserra, Ting-Wan Chen, Jason Spyromilio, Ferdinando Patat, Zach Cano, Stefan Cikota, Michael W Coughlin, Erkki Kankare, Thomas B Lowe, Justyn R Maund, Armin Rest, Stephen J Smartt, Ken W Smith, Richard J Wainscoat, David R Young
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 486:L9-L9
Autor:
Christian Schwab, John Asher Johnson, Andrew W. Howard, Jason T. Wright, Debra A. Fischer, Geoffrey W. Marcy, Peter K. G. Williams, Howard Isaacson, Gregory W. Henry, Kathryn M. G. Peek, Sabine Reffert, Thomas B. Lowe, Matthew J. Giguere
Publikováno v:
Publications of the Astronomical Society of the Pacific. 121:613-620
We present radial velocity measurements of two stars observed as part of the Lick Subgiants Planet Search and the Keck N2K survey. Variations in the radial velocities of both stars reveal the presence of Jupiter-mass exoplanets in highly eccentric or
Autor:
D. McGonagle, Thomas B. Lowe, Per Bergman, Henry E. Matthews, William M. Irvine, A. Nummelin, T. C. Owen
Publikováno v:
Origins of Life and Evolution of the Biosphere. 33:609-619
Comets have been suggested as a possibly significant source of organic molecules to the early Earth. Hydrogen cyanide (HCN) is important in models of prebiotic chemistry, but may be difficult to form in the early terrestrial environment, while hydrog
Autor:
Kathryn M. G. Peek, Sabine Reffert, Michael C. Liu, Thomas B. Lowe, Geoffrey W. Marcy, John Asher Johnson, Gregory W. Henry, Brendan P. Bowler, Debra A. Fischer, Kelsey I. Clubb, Christian Schwab
We present an analysis of ~5 years of Lick Observatory radial velocity measurements targeting a uniform sample of 31 intermediate-mass subgiants (1.5 < M*/Msun < 2.0) with the goal of measuring the occurrence rate of Jovian planets around (evolved) A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::de4a662dc8fad59123e94a13c1f3de16
https://resolver.caltech.edu/CaltechAUTHORS:20130107-094105764
https://resolver.caltech.edu/CaltechAUTHORS:20130107-094105764
Autor:
Mohan Ganeshalingam, Ryan Chornock, Martin P. Mobberley, Thomas B. Lowe, Niels Joubert, Nathan Smith, D. Winslow, Christopher V. Griffith, Thea N. Steele, Weidong Li, Alexei V. Filippenko, N. Lee, Jeffrey M. Silverman
We present visual-wavelength photometry and spectroscopy of supernova SN2008S. Based on the low peak luminosity for a SN of M_R = -13.9 mag, photometric and spectral evolution unlike that of low-luminosity SNe, a late-time decline rate slower than 56
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b76a1079bc919803d8314c262638fe0
Autor:
William M, Irvine, Per, Bergman, Thomas B, Lowe, Henry, Matthews, Douglas, McGonagle, Albert, Nummelin, Toby, Owen
Publikováno v:
Origins of life and evolution of the biosphere : the journal of the International Society for the Study of the Origin of Life. 33(6)
Comets have been suggested as a possibly significant source of organic molecules to the early Earth. Hydrogen cyanide (HCN) is important in models of prebiotic chemistry, but may be difficult to form in the early terrestrial environment, while hydrog
Autor:
Eric B. Ford, Kelsey I. Clubb, Sabine Reffert, Gregory W. Henry, Debra A. Fischer, John Asher Johnson, Christian Schwab, Brendan P. Bowler, Andrew W. Howard, Geoffrey W. Marcy, Thomas B. Lowe, John M. Brewer, Matthew J. Payne
Publikováno v:
The Astronomical Journal. 141:16
We report radial velocity measurements of the G-type subgiants 24 Sextanis (=HD90043) and HD200964. Both are massive, evolved stars that exhibit periodic variations due to the presence of a pair of Jovian planets. Photometric monitoring with the T12
Autor:
Qinan Wang, Armin Rest, Yossef Zenati, Ryan Ridden-Harper, Georgios Dimitriadis, Gautham Narayan, V. Ashley Villar, Mark R. Magee, Ryan J. Foley, Edward J. Shaya, Peter Garnavich, Lifan Wang, Lei Hu, Attila Bódi, Patrick Armstrong, Katie Auchettl, Thomas Barclay, Geert Barentsen, Zsófia Bognár, Joseph Brimacombe, Joanna Bulger, Jamison Burke, Peter Challis, Kenneth Chambers, David A. Coulter, Géza Csörnyei, Borbála Cseh, Maxime Deckers, Jessie L. Dotson, Lluís Galbany, Santiago González-Gaitán, Mariusz Gromadzki, Michael Gully-Santiago, Ottó Hanyecz, Christina Hedges, Daichi Hiramatsu, Griffin Hosseinzadeh, D. Andrew Howell, Steve B. Howell, Mark E. Huber, Saurabh W. Jha, David O. Jones, Réka Könyves-Tóth, Csilla Kalup, Charles D. Kilpatrick, Levente Kriskovics, Wenxiong Li, Thomas B Lowe, Steven Margheim, Curtis McCully, Ayan Mitra, Jose A. Muñoz, Matt Nicholl, Jakob Nordin, András Pál, Yen-Chen Pan, Anthony L. Piro, Sofia Rest, João Rino-Silvestre, César Rojas-Bravo, Krisztián Sárneczky, Matthew R. Siebert, Stephen J. Smartt, Ken Smith, Ádám Sódor, Maximilian D. Stritzinger, Róbert Szabó, Róbert Szakáts, Brad E. Tucker, József Vinkó, Xiaofeng Wang, J. Craig Wheeler, David R. Young, Alfredo Zenteno, KaiCheng Zhang, Gabriella Zsidi
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Wang, Q, Rest, A, Zenati, Y, Ridden-Harper, R, Dimitriadis, G, Narayan, G, Villar, V A, Magee, M R, Foley, R J, Shaya, E J, Garnavich, P, Wang, L, Hu, L, Bodi, A, Armstrong, P, Auchettl, K, Barclay, T, Barentsen, G, Bognar, Z, Brimacombe, J, Bulger, J, Burke, J, Challis, P, Chambers, K, Coulter, D A, Csornyei, G, Cseh, B, Deckers, M, Dotson, J L, Galbany, L, Gonzalez-Gaitan, S, Gromadzki, M, Gully-Santiago, M, Hanyecz, O, Hedges, C, Hiramatsu, D, Hosseinzadeh, G, Howell, D A, Howell, S B, Huber, M E, Jha, S W, Jones, D O, Konyves-Toth, R, Kalup, C, Kilpatrick, C D, Kriskovics, L, Li, W, Lowe, T B, Margheim, S, McCully, C, Mitra, A, Munoz, J A, Nicholl, M, Nordin, J, Pal, A, Pan, Y-C, Piro, A L, Rest, S, Rino-Silvestre, J, Rojas-Bravo, C, Sarneczky, K, Siebert, M R, Smartt, S J, Smith, K, Sodor, A, Stritzinger, M D, Szabo, R, Szakats, R, Tucker, B E, Vinko, J, Wang, X, Wheeler, J C, Young, D R, Zenteno, A, Zhang, K & Zsidi, G 2021, ' SN 2018agk : A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2) ', Astrophysical Journal, vol. 923, no. 2, 167 . https://doi.org/10.3847/1538-4357/ac2c84
instname
Wang, Q, Rest, A, Zenati, Y, Ridden-Harper, R, Dimitriadis, G, Narayan, G, Villar, V A, Magee, M R, Foley, R J, Shaya, E J, Garnavich, P, Wang, L, Hu, L, Bodi, A, Armstrong, P, Auchettl, K, Barclay, T, Barentsen, G, Bognar, Z, Brimacombe, J, Bulger, J, Burke, J, Challis, P, Chambers, K, Coulter, D A, Csornyei, G, Cseh, B, Deckers, M, Dotson, J L, Galbany, L, Gonzalez-Gaitan, S, Gromadzki, M, Gully-Santiago, M, Hanyecz, O, Hedges, C, Hiramatsu, D, Hosseinzadeh, G, Howell, D A, Howell, S B, Huber, M E, Jha, S W, Jones, D O, Konyves-Toth, R, Kalup, C, Kilpatrick, C D, Kriskovics, L, Li, W, Lowe, T B, Margheim, S, McCully, C, Mitra, A, Munoz, J A, Nicholl, M, Nordin, J, Pal, A, Pan, Y-C, Piro, A L, Rest, S, Rino-Silvestre, J, Rojas-Bravo, C, Sarneczky, K, Siebert, M R, Smartt, S J, Smith, K, Sodor, A, Stritzinger, M D, Szabo, R, Szakats, R, Tucker, B E, Vinko, J, Wang, X, Wheeler, J C, Young, D R, Zenteno, A, Zhang, K & Zsidi, G 2021, ' SN 2018agk : A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2) ', Astrophysical Journal, vol. 923, no. 2, 167 . https://doi.org/10.3847/1538-4357/ac2c84
Wang, Qinan, et al.
We present the 30 minutes cadence Kepler/K2 light curve of the Type Ia supernova (SN Ia) SN 2018agk, covering approximately one week before explosion, the full rise phase, and the decline until 40 days after peak. We addition
We present the 30 minutes cadence Kepler/K2 light curve of the Type Ia supernova (SN Ia) SN 2018agk, covering approximately one week before explosion, the full rise phase, and the decline until 40 days after peak. We addition