Zobrazeno 1 - 10 of 170 pro vyhledávání: '"Tallon, D"'
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Report
Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations
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
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2
Report
Seeing Double: ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve
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
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3
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5
Seeing Double:ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve
Autor: Shappee, BJ, Holoien, TW-S, Drout, MR, Auchettl, K, Stritzinger, MD, Kochanek, CS, Stanek, KZ, Shaya, E, Narayan, G, Brown, JS, Bose, S, Bersier, D, Brimacombe, J, Chen, P, Dong, S, Holmbo, S, Katz, B, Munoz, JA, Mutel, RL, Post, RS, Prieto, JL, Shields, J, Tallon, D, Thompson, TA, Vallely, PJ, Villanueva, S, Denneau, L, Flewelling, H, Heinze, AN, Smith, KW, Stalder, B, Tonry, JL, Weiland, H, Barclay, T, Barentsen, G, Cody, AM, Dotson, J, Foerster, F, Garnavich, P, Gully-Santiago, M, Hedges, C, Howell, S, Kasen, D, Margheim, S, Mushotzky, R, Rest, A, Tucker, BE, 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, KA, McCalmont-Everton, KM, McGinn, C, Migliorini, L, Moffatt, J, Muszynski, M, Nystrom, V, Osborne, D, Packard, M, Peterson, CA, Redick, M, Reedy, LH, Ross, SE, Spencer, B, Steward, K, Van Cleve, JE, Vinicius de Miranda Cardoso, J, Weschler, T, Wheaton, A, Bulger, J, Chambers, KC, Flewelling, HA, Huber, ME, Lowe, TB, Magnier, EA, Schultz, ASB, Waters, CZ, Willman, M, Baron, E, Chen, Z, Derkacy, JM, Huang, F, Li, L, Li, W, Li, X, Mo, J, Rui, L, Sai, H, Wang, L, Wang, X, Xiang, D, Zhang, J, Zhang, K, Zhang, T, Zhang, X, Zhao, X, Brown, PJ, Hermes, JJ, Nordin, J, Points, S, Sodor, A, Strampelli, GM
Publikováno v: 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, P, Dong, S, Holmbo, S, Katz, B, Munoz, J A, Mutel, R L, Post, R S, Prieto, J L, Shields, J, Tallon, D, Thompson, T A, Vallely, P J, Villanueva, S J, Denneau, L, Flewelling, H A, 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 & ASAS 2019, ' Seeing Double : ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve ', Astrophysical Journal, vol. 870, no. 1, 13 . https://doi.org/10.3847/1538-4357/aaec79
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: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9d85898e8028352f3955a55276465e1
https://curis.ku.dk/ws/files/256068094/Shappee_2019_ApJ_870_13.pdf
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6
Seeing Double:ASASSN-18bt Exhibits a two-component Rise in the Early-Time K2 Light Curve
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., Jr, S. Villanueva, 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., Spencer, B., Steward, K., Cleve, J. E. Van, Cardoso, J. Vinicius De Miranda, Weschler, T., Wheaton, A., Bulger, J., Lowe, T. B., Magnier, E. A., 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.
Publikováno v: Shappee, B J, Holoien, T W, 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, P, Dong, S, 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, Jr, S V, 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, Spencer, B, Steward, K, Cleve, J E V, Cardoso, J V D M, Weschler, T, Wheaton, A, Bulger, J, Lowe, T B, Magnier, E A, Waters, C Z, Willman, M, Baron, E, Chen, Z, Derkacy, J M, Huang, F, Li, L, Li, W, Li, X, Rui, L, Sai, H, Wang, L, Wang, L, Wang, X, Xiang, D, Zhang, J, Zhang, J, Zhang, K, Zhang, T, Zhang, X, Zhao, X, Brown, P J, Hermes, J J, Nordin, J, Points, S, Strampelli, G M & Zenteno, A 2019, ' Seeing Double : ASASSN-18bt Exhibits a two-component Rise in the Early-Time K2 Light Curve ', The Astrophysical Journal, vol. 870, no. 13 .
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 $z=0.010981$ and a peak apparent magnitude of $B_{max}=14.31$, ASASSN-18bt is the nearest and brightest SN
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::85499b4c4079c539d2b5778777cfe674
https://pure.au.dk/portal/da/publications/seeing-double(e0723921-98d9-43ec-840b-e21dbb4fb772).html
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