Zobrazeno 1 - 10
of 113
pro vyhledávání: '"Robert L. Mutel"'
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 1, p 86 (2024)
We report multiepoch astrometric very long baseline interferometry observations of the chromospherically active binary HR 1099 (V711 Tau, HD 22468) at six epochs over 63 days using the Very Long Baseline Array at 22.2 GHz. We determined hourly radio
Externí odkaz:
https://doaj.org/article/8ac9f654a7ea4fb0aa3a3c09a638f4cb
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:1394-1410
We searched for thermal gyro-synchrotron radio emission from a sample of five radio-loud stars whose X-ray coronae contain a hot ($T_e>10^7$ K) thermal component. We used the JVLA to measure Stokes I and V/I spectral energy distributions (SEDs) over
Autor:
Xinyu Mai, Robert L Mutel
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 517:L108-L110
Er et al. (2021) recently proposed a two-planet solution to account for eclipse timing variations (ETVs) observed from the sdB binary NY Virginis. We tested the proposed planetary system for orbit stability using both numerical simulations and chaoti
Autor:
Xinyu Mai, Robert L Mutel
We report 90 new observations of three post common envelope binaries at primary eclipse spanning between December 2018 to February 2022. We combine recent primary eclipse timing observations with previously published values to search for substellar c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e5ba0981999fbe7a07a13337d905d3d
http://arxiv.org/abs/2110.14869
http://arxiv.org/abs/2110.14869
Autor:
T. W. S. Holoien, Robert L. Mutel, Christopher S. Kochanek, E. E. Falco, T. M. Reynolds, WeiKang Zheng, A. Fiore, Andrea Pastorello, Alexei V. Filippenko, Auni Somero, Benjamin J. Shappee, Naveen A. Reddy, T. G. Brink, Peter Lundqvist, Subo Dong, Katie Auchettl, Chris Ashall, K. Z. Stanek, M. Stritzinger, Dirk Grupe, Tuguldur Sukhbold, Seppo Mattila, S. Benetti, Subhash Bose, Steven Villanueva, David Pooley, J. S. Brown, R. S. Post, Junbo Zhang, J. L. Prieto, Todd A. Thompson, Ping Chen
Publikováno v:
Bose, S, Dong, S, Kochanek, C S, Stritzinger, M D, Ashall, C, Benetti, S, Falco, E, Filippenko, A V, Pastorello, A, Prieto, J L, Somero, A, Sukhbold, T, Zhang, J, Auchettl, K, Brink, T G, Brown, J S, Chen, P, Fiore, A, Grupe, D, Holoien, T W S, Lundqvist, P, Mattila, S, Mutel, R, Pooley, D, Post, R S, Reddy, N, Reynolds, T M, Shappee, B J, Stanek, K Z, Thompson, T A, Villanueva, S & Zheng, W K 2021, ' ASASSN-18am/SN 2018gk : An overluminous type IIb supernova from a massive progenitor ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 3472-3491 . https://doi.org/10.1093/mnras/stab629
Bose, S, Dong, S, Kochanek, C S, Stritzinger, M D, Ashall, C, Benetti, S, Falco, E, Filippenko, A, Pastorello, A, Prieto, J L, Somero, A, Sukhbold, T, Zhang, J, Auchettl, K, Brink, T G, Brown, J S, Chen, P, Fiore, A, Grupe, D, Holoien, T W S, Lundqvist, P, Mattila, S, Mutel, R, Pooley, D, Post, R S, Reddy, N, Reynolds, T M, Shappee, B J, Stanek, K Z, Thompson, T A, Villanueva, S JR & Zheng, W 2021, ' ASASSN-18am/SN 2018gk : an overluminous Type IIb supernova from a massive progenitor ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 3472-3491 . https://doi.org/10.1093/mnras/stab629
Bose, S, Dong, S, Kochanek, C S, Stritzinger, M D, Ashall, C, Benetti, S, Falco, E, Filippenko, A, Pastorello, A, Prieto, J L, Somero, A, Sukhbold, T, Zhang, J, Auchettl, K, Brink, T G, Brown, J S, Chen, P, Fiore, A, Grupe, D, Holoien, T W S, Lundqvist, P, Mattila, S, Mutel, R, Pooley, D, Post, R S, Reddy, N, Reynolds, T M, Shappee, B J, Stanek, K Z, Thompson, T A, Villanueva, S JR & Zheng, W 2021, ' ASASSN-18am/SN 2018gk : an overluminous Type IIb supernova from a massive progenitor ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 3472-3491 . https://doi.org/10.1093/mnras/stab629
ASASSN-18am/SN 2018gk is a newly discovered member of the rare group of luminous, hydrogen-rich supernovae (SNe) with a peak absolute magnitude of MV ≈ −20 mag that is in between normal core-collapse SNe and superluminous SNe. These SNe show no p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f75e874078cb06bc427969f5c3a6422
https://pure.au.dk/portal/da/publications/asassn18amsn-2018gk(7cd63507-3294-4d0e-9b96-8329fdb63c90).html
https://pure.au.dk/portal/da/publications/asassn18amsn-2018gk(7cd63507-3294-4d0e-9b96-8329fdb63c90).html
Autor:
D. A. Ludovici, Robert L. Mutel
Publikováno v:
American Journal of Physics. 85:873-879
We describe a low-cost compact grism spectrometer for use with small astronomical telescopes. The system can be used with existing charge-coupled device (CCD) cameras and filter wheels. The optical design consists of two prisms, a transmission gratin
Publikováno v:
Journal of Geophysical Research: Space Physics. 122:249-257
We present results of intense AKR sources direction finding based on single spacecraft k→ vector source location performed in the frame of Interball-2 mission (POLRAD experiment on board Auroral Probe). With our swept frequency analyzer we are not
Autor:
Jakob Nordin, D. Bersier, Gautham Narayan, Dan Kasen, Zhihao Chen, R. S. Post, B. Cseh, J. Van Cleve, James M. DerKacy, L. Denneau, Lluís Galbany, M. Redick, A. Rest, Krisztián Sárneczky, Subhash Bose, Curtis McCully, Hanna Sai, B. C. Kaiser, E. Baron, C. A. Peterson, J. Vinicius de Miranda Cardoso, Jeffrey L. Coughlin, A. Razza, M. Packard, Steven Williams, G. Beerman, M. Muszynski, Cs. Kalup, B. Elsaesser, O. Hanyecz, G. Csörnyei, Iair Arcavi, J. Moffatt, Isobel Hook, Wenxiong Li, A. Villar, J. Kampmeier, Robert L. Mutel, César Rojas-Bravo, K. A. Larson, Liming Rui, R. Gangopadhyay, B. Csák, S. Margheim, Peter A. Milne, Cosimo Inserra, Subo Dong, Thomas W.-S. Holoien, Jennifer E. Andrews, J. Burke, Han Lin, Jun Mo, Jessie L. Dotson, Kaicheng Zhang, John C Wheeler, J. Palmerio, J. S. Brown, R. M. Larsen, Kate Maguire, H. Flewelling, Katie Auchettl, Danfeng Xiang, K. C. Chambers, Ori D. Fox, Attila Bódi, S. Holmbo, András Pál, C. McGinn, Edward J. Shaya, John L. Tonry, Xulin Zhao, Xiaojia Zhang, E. A. Magnier, M. Hanley, Yen-Chen Pan, Bernadett Ignácz, B. Stalder, R. Szabó, K. M. McCalmont-Everton, G. Zsidi, Joshua S. Reding, J. A. Muñoz, Geert Barentsen, Daichi Hiramatsu, K. Steward, Brad E. Tucker, J. Brimacombe, K. W. Smith, A. Zenteno, R. J. Foley, J. V. Shields, I. Rajmon, Jozsef Vinko, Xiaofeng Wang, Charles D. Kilpatrick, Steven Villanueva, A. Wheaton, B. Spencer, Ann Marie Cody, Peter J. Brown, T. Weschler, L. Migliorini, Xue Li, Claudia P. Gutiérrez, Fang Huang, Saurabh Jha, R. Bjella, C. Labonde, Benjamin J. Shappee, Mark Willman, D. Tallon, V. Nystrom, Tianmeng Zhang, Griffin Hosseinzadeh, S. Flynn, Long Wang, David A. Coulter, David J. Sand, Georgios Dimitriadis, D. O. Jones, J. J. Hermes, Thomas Barclay, Christopher Bilinski, H. Weiland, Réka Könyves-Tóth, Régis Cartier, Steve B. Howell, Peter M. Garnavich, Kim Griest, J. L. Prieto, S. E. Ross, Mark E. Huber, Zs. Bognár, Róbert Szakáts, R. Kloetzel, Krzysztof Z. Stanek, Christopher S. Kochanek, Stefano Valenti, Christina Hedges, G. Castillo, Todd A. Thompson, Ping Chen, C. Z. Waters, L. Kohnert, Adam G. Riess, Nathan Smith, T. B. Lowe, Anthony L. Piro, L. H. Reedy, Levente Kriskovics, Linyi Li, Maria R. Drout, Dale Andrew Howell, A. N. Heinze, A. Ordasi, Stephen J. Smartt, Patrick J. Vallely, A. S. B. Schultz, Joanna Bulger, Michael Gully-Santiago, Jujia Zhang, Ádám Sódor, D. Osborne
Publikováno v:
Astrophys.J.
Astrophys.J., 2019, 870 (1), pp.12. ⟨10.3847/1538-4357/aaec74⟩
Li, W, Wang, X, Vinko, J, Mo, J, Hosseinzadeh, G, Sand, D J, Zhang, J, Lin, H, Zhang, T, Wang, L, Zhang, J, Chen, Z, Xiang, D, Rui, L, Huang, F, Li, X, Zhang, X, Li, L, Baron, E, Derkacy, J M, Zhao, X, Sai, H, Zhang, K, Wang, L, Howell, D A, McCully, C, Arcavi, I, Valenti, S, Hiramatsu, D, Burke, J, Rest, A, Garnavich, P, Tucker, B E, Narayan, G, Shaya, E, Margheim, S, Zenteno, A, Villar, A, Dimitriadis, G, Foley, R J, Pan, Y-C, Coulter, D A, Fox, O D, Jha, S W, Jones, D O, Kasen, D N, Kilpatrick, C D, Piro, A L, Riess, A G, Holmbo, S, PTSS TNTS, LCO, KEGS, UCSC, ASAS-SN, Pan-STARRS, Swift, ePESSTO, ATLAS, K2 Mission Team & Kepler Spacecraft Team 2019, ' Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations ', Astrophysical Journal, vol. 870, no. 1, 12 . https://doi.org/10.3847/1538-4357/aaec74
The Astrophysical Journal
Astrophys.J., 2019, 870 (1), pp.12. ⟨10.3847/1538-4357/aaec74⟩
Li, W, Wang, X, Vinko, J, Mo, J, Hosseinzadeh, G, Sand, D J, Zhang, J, Lin, H, Zhang, T, Wang, L, Zhang, J, Chen, Z, Xiang, D, Rui, L, Huang, F, Li, X, Zhang, X, Li, L, Baron, E, Derkacy, J M, Zhao, X, Sai, H, Zhang, K, Wang, L, Howell, D A, McCully, C, Arcavi, I, Valenti, S, Hiramatsu, D, Burke, J, Rest, A, Garnavich, P, Tucker, B E, Narayan, G, Shaya, E, Margheim, S, Zenteno, A, Villar, A, Dimitriadis, G, Foley, R J, Pan, Y-C, Coulter, D A, Fox, O D, Jha, S W, Jones, D O, Kasen, D N, Kilpatrick, C D, Piro, A L, Riess, A G, Holmbo, S, PTSS TNTS, LCO, KEGS, UCSC, ASAS-SN, Pan-STARRS, Swift, ePESSTO, ATLAS, K2 Mission Team & Kepler Spacecraft Team 2019, ' Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations ', Astrophysical Journal, vol. 870, no. 1, 12 . https://doi.org/10.3847/1538-4357/aaec74
The Astrophysical Journal
Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting constraints o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55e9e5cf46dafad065d3e32cbff5c492
https://hal.archives-ouvertes.fr/hal-01990737
https://hal.archives-ouvertes.fr/hal-01990737
Autor:
Thomas W.-S. Holoien, F. Delplancke-Ströbele, Benjamin J. Shappee, G. W. Christie, Andrew Gould, R. S. Post, Robert L. Mutel, Tim Natusch, Todd A. Thompson, Ping Chen, Subo Dong, J. L. Prieto, Antoine Mérand, Christopher S. Kochanek, Krzysztof Z. Stanek
Publikováno v:
The Astrophysical Journal
We employ VLTI GRAVITY to resolve, for the first time, the two images generated by a gravitational microlens. The measurements of the image separation \theta_{-,+}=3.78 +/- 0.05 mas, and hence the Einstein radius \theta_E =1.87 +/- 0.03 mas, are prec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5cca903c47931c4af233ac122b46cf1
https://hdl.handle.net/21.11116/0000-0005-D15E-6
https://hdl.handle.net/21.11116/0000-0005-D15E-6
Autor:
Robert L. Mutel, Hongjing Yang, Shude Mao, Shun-Sheng Li, Shaoming Hu, Tim Natusch, Fengwu Sun, G. W. Christie, Subo Dong, Tyler Roth, Alexander Kurtenkov, Dax L. Feliz, Antoine Mérand, Weicheng Zang, Jonathan Green, Tharindu Jayasinghe, Yossi Shvartzvald, T. Vanmunster, F. Delplancke-Ströbele, B. Scott Gaudi, Wei Zhu, Robert Koff, Joseph Brimacombe, Andrew Gould, M. Minev, Sean Carey, K. B. Alton, Sebastiano Calchi Novati, Ping Chen
Publikováno v:
The Astrophysical Journal. 897:180
We report the lens mass and distance measurements of the nearby microlensing event TCP J05074264+2447555. We measure the microlens parallax vector ${\pi}_{\rm E}$ using Spitzer and ground-based light curves with constraints on the direction of lens-s