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pro vyhledávání: '"Flynn S"'
Autor:
Dimitriadis, G., Foley, R. J., Rest, A., Kasen, D., Piro, A. L., Polin, A., Jones, D. O., Villar, A., Narayan, G., Coulter, D. A., Kilpatrick, C. D., Pan, Y. -C., Rojas-Bravo, C., Fox, O. D., Jha, S. W., Nugent, P. E., Riess, A. G., Scolnic, D., Drout, M. R., Barentsen, G., Dotson, J., Gully-Santiago, M., Hedges, C., Cody, A. M., Barclay, T., Howell, S., Garnavich, P., Tucker, B. E., Shaya, E., Mushotzky, R., Olling, R. P., Margheim, S., Zenteno, A., Coughlin, J., Van Cleve, J. E., Cardoso, J. Vinicius de Miranda, Larson, K. A., McCalmont-Everton, K. M., Peterson, C. A., Ross, S. E., Reedy, L. H., Osborne, D., McGinn, C., Kohnert, L., Migliorini, L., Wheaton, A., Spencer, B., Labonde, C., Castillo, G., Beerman, G., Steward, K., Hanley, M., Larsen, R., Gangopadhyay, R., Kloetzel, R., Weschler, T., Nystrom, V., Moffatt, J., Redick, M., Griest, K., Packard, M., Muszynski, M., Kampmeier, J., Bjella, R., Flynn, S., Elsaesser, B., Chambers, K. C., Flewelling, H. A., Huber, M. E., Magnier, E. A., Waters, C. Z., Schultz, A. S. B., Bulger, J., Lowe, T. B., Willman, M., Smartt, S. J., Smith, K. W., Points, S., Strampelli, G. M., Brimacombe, J., Chen, P., Munoz, J. A., Mutel, R. L., Shields, J., Vallely, P. J., Villanueva Jr, S., Li, W., Wang, X., Zhang, J., Lin, H., Mo, J., Zhao, X., Sai, H., Zhang, X., Zhang, K., Zhang, T., Wang, L., Baron, E., DerKacy, J. M., Li, L., Chen, Z., Xiang, D., Rui, L., Huang, F., Li, X., Hosseinzadeh, G., Howell, D. A., Arcavi, I., Hiramatsu, D., Burke, J., Valenti, S., Tonry, J. L., Denneau, L., Heinze, A. N., Weiland, H., Stalder, B., Vinko, J., Sarneczky, K., Pa, A., Bodi, A., Bognar, Zs., Csak, B., Cseh, B., Csornyei, G., Hanyecz, O., Ignacz, B., Kalup, Cs., Konyves-Toth, R., Kriskovics, L., Ordasi, A., Rajmon, I., Sodor, A., Szabo, R., Szakats, R., Zsidi, G., Williams, S. C., Nordin, J., Cartier, R., Frohmaier, C., Galbany, L., Gutierrez, C. P., Hook, I., Inserra, C., Smith, M., Sand, D. J., Andrews, J. E., Smith, N., Bilinski, C.
We present an exquisite, 30-min cadence Kepler (K2) light curve of the Type Ia supernova (SN Ia) 2018oh (ASASSN-18bt), starting weeks before explosion, covering the moment of explosion and the subsequent rise, and continuing past peak brightness. The
Externí odkaz:
http://arxiv.org/abs/1811.10061
Autor:
Li, W., Wang, X., Vinkó, J., Mo, J., Hosseinzadeh, G., Sand, D. J., Zhang, J., Lin, H., Zhang, T., Wang, L., 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., 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., Rojas-Bravo, C., Shappee, B. J., Holoien, T. W. -S., Stanek, K. Z., Drout, M. R., Auchettl, K., Kochanek, C. S., Brown, J. S., Bose, S., Bersier, D., Brimacombe, J., Chen, P., Dong, S., Holmbo, S., Muñoz, J. A., Mutel, R. L., Post, R. S., Prieto, J. L., Shields, J., Tallon, D., Thompson, T. A., Vallely, P. J., Villanueva Jr., S., Smartt, S. J., Smith, K. W., Chambers, K. C., Flewelling, H. A., Huber, M. E., Magnier, E. A., Waters, C. Z., Schultz, A. S. B., Bulger, J., Lowe, T. B., Willman, M., Sárneczky, K., Pál, A., Wheeler, J. C., Bódi, A., Bognár, Zs., Csák, B., Cseh, B., Csörnyei, G., Hanyecz, O., Ignácz, B., Kalup, Cs., Könyves-Tóth, R., Kriskovics, L., Ordasi, A., Rajmon, I., Sódor, A., Szabó, R., Szakáts, R., Zsidi, G., Milne, P., Andrews, J. E., Smith, N., Bilinski, C., Brown, P. J., Nordin, J., Williams, S. C., Galbany, L., Palmerio, J., Hook, I. M., Inserra, C., Maguire, K., Cartier, Régis, Razza, A., Gutiérrez, C. P., Hermes, J. J., Reding, J. S., Kaiser, B. C., Tonry, J. L., Heinze, A. N., Denneau, L., Weiland, H., Stalder, B., Barentsen, G., Dotson, J., Barclay, T., Gully-Santiago, M., Hedges, C., Cody, A. M., Howell, S., Coughlin, J., Van Cleve, J. E., Cardoso, J. Vinícius de Miranda, Larson, K. A., McCalmont-Everton, K. M., Peterson, C. A., Ross, S. E., Reedy, L. H., Osborne, D., McGinn, C., Kohnert, L., Migliorini, L., Wheaton, A., Spencer, B., Labonde, C., Castillo, G., Beerman, G., Steward, K., Hanley, M., Larsen, R., Gangopadhyay, R., Kloetzel, R., Weschler, T., Nystrom, V., Moffatt, J., Redick, M., Griest, K., Packard, M., Muszynski, M., Kampmeier, J., Bjella, R., Flynn, S., Elsaesser, B.
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:
http://arxiv.org/abs/1811.10056
Autor:
Shappee, B. J., Holoien, T. W. -s., Drout, M. R., Auchettl, K., Stritzinger, M. D., Kochanek, C. S., Stanek, K. Z., Shaya, E., Narayan, G., Brown, J. S., Bose, S., Bersier, D., Brimacombe, J., Chen, Ping, Dong, Subo, Holmbo, S., Katz, B., Munnoz, J. A., Mutel, R. L., Post, R. S., Prieto, J. L., Shields, J., Tallon, D., Thompson, T. A., Vallely, P. J., Villanueva Jr., S., Denneau, L., Flewelling, H., Heinze, A. N., Smith, K. W., Stalder, B., Tonry, J. L., Weiland, H., Barclay, T., Barentsen, G., Cody, A. M., Dotson, J., Foerster, F., Garnavich, P., Gully-santiago, M., Hedges, C., Howell, S., Kasen, D., Margheim, S., Mushotzky, R., Rest, A., Tucker, B. E., Villar, A., Zenteno, A., Beerman, G., Bjella, R., Castillo, G., Coughlin, J., Elsaesser, B., Flynn, S., Gangopadhyay, R., Griest, K., Hanley, M., Kampmeier, J., Kloetzel, R., Kohnert, L., Labonde, C., Larsen, R., Larson, K. A., Mccalmont-everton, K. M., Mcginn, C., Migliorini, L., Moffatt, J., Muszynski, M., Nystrom, V., Osborne, D., Packard, M., Peterson, C. A., Redick, M., Reedy, L. H., Ross, S. E., Spencer, B., Steward, K., Van Cleve, J. E., Cardoso, J. Vinicius De Miranda, Weschler, T., Wheaton, A., Bulger, J., Lowe, T. B., Magnier, E. A., Schultz, A. S. B., Waters, C. Z., Willman, M., Baron, Eddie, Chen, Zhihao, Derkacy, James M., Huang, Fang, Li, Linyi, Li, Wenxiong, Li, Xue, Rui, Liming, Sai, Hanna, Wang, Lifan, Wang, Lingzhi, Wang, Xiaofeng, Xiang, Danfeng, Zhang, Jicheng, Zhang, Jujia, Zhang, Kaicheng, Zhang, Tianmeng, Zhang, Xinghan, Zhao, Xulin, Brown, P. J., Hermes, J. J., Nordin, J., Points, S., Strampelli, G. M.
On 2018 Feb. 4.41, the All-Sky Automated Survey for SuperNovae (ASAS-SN) discovered ASASSN-18bt in the K2 Campaign 16 field. With a redshift of z=0.01098 and a peak apparent magnitude of B_{max}=14.31, ASASSN-18bt is the nearest and brightest SNe Ia
Externí odkaz:
http://arxiv.org/abs/1807.11526
Autor:
Kopsalis, I., Allport, P., Benhammadi, S., Bosley, R., Dopke, J., Fasselt, L., Flynn, S., Freeman, P., Gonella, L., Guerrini, N., Issever, C., Nikolopoulos, K., Phillips, P., Price, T., Sedgwick, I., Villani, E.G., Warren, M., Watson, N.K., Weber, H., Wilson, F., Winter, A., Worm, S., Zhang, Z.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 September 2022 1038
Autor:
Hayden, N. K.1 (AUTHOR), Flynn, S.1 (AUTHOR), Blumenfeld, F.2 (AUTHOR), Hastings, R. P.1,3 (AUTHOR), Gray, K. M.1,3 (AUTHOR), Cullen, S.1 (AUTHOR), Cullen, M. A.1 (AUTHOR), Langdon, P. E.1,4,5 (AUTHOR) Peter.Langdon@warwick.ac.uk
Publikováno v:
Pilot & Feasibility Studies. 11/27/2023, Vol. 9 Issue 1, p1-11. 11p.
Autor:
Sutherland, D.1 daniel.sutherland@warwick.ac.uk, Flynn, S.1, Kurzeja, O.1, Griffin, J.1, Hastings, R.1,2
Publikováno v:
Journal of Intellectual Disability Research. Oct2023, Vol. 67 Issue 10, p1003-1028. 26p. 1 Diagram, 6 Charts.
Autor:
Allport, P., Benhammadi, S., Bosley, R., Dopke, J., Flynn, S., Freeman, P., Gonella, L., Guerrini, N., Kopsalis, I., Nikolopoulos, K., Phillips, P., Price, T., Scott, A., Sedgwick, I., Villani, E.G., Warren, M., Watson, N., Wilson, F., Winter, A., Worm, S., Zhang, Z.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 October 2020 978
Autor:
Allport, P.P., Bosley, R., Dopke, J., Flynn, S., Gonella, L., Kopsalis, I., Nikolopoulos, K., Phillips, P.W., Price, T., Scott, A., Sedgwick, I., Villani, E.G., Warren, M., Watson, N., Wilson, F., Winter, A., Worm, S., Zhang, Z.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 April 2020 958
Autor:
Austermann, J. E., Dunlop, J. S., Perera, T. A., Scott, K. S., Wilson, G. W., Aretxaga, I., Hughes, D. H., Almaini, O., Chapin, E. L., Chapman, S. C., Cirasuolo, M., Clements, D. L., Coppin, K. E. K., Dunne, L., Dye, S., Eales, S. A., Egami, E., Farrah, D., Ferrusca, D., Flynn, S., Haig, D., Halpern, M., Ibar, E., Ivison, R. J., van Kampen, E., Kang, Y., Kim, S., Lacey, C., Lowenthal, J. D., Mauskopf, P. D., McLure, R. J., Mortier, A. M. J., Negrello, M., Oliver, S., Peacock, J. A., Pope, A., Rawlings, S., Rieke, G., Roseboom, I., Rowan-Robinson, M., Scott, D., Serjeant, S., Smail, I., Swinbank, A. M., Stevens, J. A., Velazquez, M., Wagg, J., Yun, M. S.
We present the first results from the largest deep extragalactic millimetre-wavelength survey undertaken to date. These results are derived from maps covering over 0.7 deg^2, made at 1.1mm, using the AzTEC continuum camera mounted on the James Clerk
Externí odkaz:
http://arxiv.org/abs/0907.1093