Zobrazeno 1 - 10
of 74
pro vyhledávání: '"Duev, D A"'
Autor:
Bolin, B. T., Masci, F. J., Coughlin, M. W., Duev, D. A., Ivezić, Ž., Jones, R. L., Yoachim, P., Ahumada, T., Bhalerao, V., Choudhary, H., Contreras, C., Cheng, Y. -C., Copperwheat, C. M., Deshmukh, K., Fremling, C., Granvik, M., Hardegree-Ullman, K. K., Ho, A. Y. Q., Jedicke, R., Kasliwal, M., Kumar, H., Lin, Z. -Y., Mahabal, A., Monson, A., Neill, J. D., Nesvorný, D., Perley, D. A., Purdum, J. N., Quimby, R., Serabyn, E., Sharma, K., Swain, V.
Near-sun sky twilight observations allow for the detection of asteroid interior to the orbit of Venus (Aylos), the Earth (Atiras), and comets. We present the results of observations with the Palomar 48-inch telescope (P48)/Zwicky Transient Facility (
Externí odkaz:
http://arxiv.org/abs/2409.15263
Autor:
Bolin, B. T., Masci, F. J., Duev, D. A., Milburn, J. W., Purdum, J. N., Avdellidou, C., Cheng, Y. -C., Delbo, M., Fremling, C., Ghosal, M., Lin, Z. -Y., Lisse, C. M., Mahabal, A., Saki, M.
Long-period comets are planetesimal remnants constraining the environment and volatiles of the protoplanetary disc. We report the discovery of hyperbolic long-period comet C/2022 E3 (ZTF), which has a perihelion $\sim$1.11 au, an eccentricity $\gtrsi
Externí odkaz:
http://arxiv.org/abs/2309.14336
A monitoring campaign (2013-2020) of ESA's Mars Express to study interplanetary plasma scintillation
Autor:
Kummamuru, P., Calvés, G. Molera, Cimò, G., Pogrebenko, S. V., Bocanegra-Bahamón, T. M., Duev, D. A., Said, M. D. Md, Edwards, J., Ma, M., Quick, J., Neidhardt, A., de Vicente, P., Haas, R., Kallunki, J., Maccaferri, 1 G., Colucci, G., Yang, W. J., Hao, L. F., Weston, S., Kharinov, M. A., Mikhailov, A. G., Jung, T.
The radio signal transmitted by the Mars Express (MEX) spacecraft was observed regularly between the years 2013-2020 at X-band (8.42 GHz) using the European Very Long Baseline Interferometry (EVN) network and University of Tasmania's telescopes. We p
Externí odkaz:
http://arxiv.org/abs/2302.13898
Supernova Siblings and their Parent Galaxies in the Zwicky Transient Facility Bright Transient Surve
Autor:
Graham, M. L., Fremling, C., Perley, D. A., Biswas, R., Phillips, C. A., Sollerman, J., Nugent, P. E., Nance, S., Dhawan, S., Nordin, J., Goobar, A., Miller, A., Neill, J. D., Hall, X. J., Hankins, M. J., Duev, D. A., Kasliwal, M. M., Rigault, M., Bellm, E. C., Hale, D., Mróz, P., Kulkarni, S. R.
Supernova (SN) siblings -- two or more SNe in the same parent galaxy -- are useful tools for exploring progenitor stellar populations as well as properties of the host galaxies such as distance, star formation rate, dust extinction, and metallicity.
Externí odkaz:
http://arxiv.org/abs/2112.14819
Autor:
Gal-Yam, A., Bruch, R., Schulze, S., Yang, Y., Perley, D. A., Irani, I., Sollerman, J., Kool, E. C., Soumagnac, M. T., Yaron, O., Strotjohann, N. L., Zimmerman, E., Barbarino, C., Kulkarni, S. R., Kasliwal, M. M., De, K., Yao, Y., Fremling, C., Yan, L., Ofek, E. O., Fransson, C., Filippenko, A. V., Zheng, W., Brink, T. G., Copperwheat, C. M., Foley, R. J., Brown, J., Siebert, M., Leloudas, G., Cabrera-Lavers, A. L., Garcia-Alvarez, D., Marante-Barreto, A., Frederick, S., Hung, T., Wheeler, J. C., Vinko, J., Thomas, B. P., Graham, M. J., Duev, D. A., Drake, A. J., Dekany, R., Bellm, E. C., Rusholme, B., Shupe, D. L., Andreoni, I., Sharma, Y., Riddle, R., van Roestel, J., Knezevic, N.
The final explosive fate of massive stars, and the nature of the compact remnants they leave behind (black holes and neutron stars), are major open questions in astrophysics. Many massive stars are stripped of their outer hydrogen envelopes as they e
Externí odkaz:
http://arxiv.org/abs/2111.12435
Autor:
Ofek, E. O., Adams, S. M., Waxman, E., Sharon, A., Kushnir, D., Horesh, A., Ho, A., Kasliwal, M. M., Yaron, O., Gal-Yam, A., Kulkarni, S. R., Bellm, E., Masci, F., Shupe, D., Dekany, R., Graham, M., Riddle, R., Duev, D., Andreoni, I., Mahabal, A., Drake, A.
We report on the discovery of AT2018lqh (ZTF18abfzgpl) -- a rapidly-evolving extra-galactic transient in a star-forming host at 242 Mpc. The transient g-band light curve's duration above half-maximum light is about 2.1 days, where 0.4/1.7 days are sp
Externí odkaz:
http://arxiv.org/abs/2109.10931
Autor:
van Roestel, J., Kupfer, T., Green, M. J., Wong, S., Bildsten, L., Burdge, K., Prince, T., Marsh, T. R., Szkody, P., Fremling, C., Graham, M. J., Dhillon, V. S., Littlefair, S. P., Bellm, E. C., Coughlin, M., Duev, D. A., Goldstein, D. A., Laher, R. R., Rusholme, B., Riddle, R., Dekany, R., Kulkarni, S. R.
AM CVn systems are ultra-compact, helium-rich, accreting binaries with degenerate or semi-degenerate donors. We report the discovery of five new eclipsing AM CVn systems with orbital periods of 61.5, 55.5, 53.3, 37.4, and 35.4 minutes. These systems
Externí odkaz:
http://arxiv.org/abs/2107.07573
Autor:
Malyali, A., Rau, A., Merloni, A., Nandra, K., Buchner, J., Liu, Z., Gezari, S., Sollerman, J., Shappee, B., Trakhtenbrot, B., Arcavi, I., Ricci, C., van Velzen, S., Goobar, A., Frederick, S., Kawka, A., Tartaglia, L., Burke, J., Hiramatsu, D., Schramm, M., van der Boom, D., Anderson, G., Miller-Jones, J. C. A., Bellm, E., Drake, A., Duev, D., Fremling, C., Graham, M., Masci, F., Rusholme, B., Soumagnac, M., Walters, R.
We report on SRG/eROSITA, ZTF, ASAS-SN, Las Cumbres, NEOWISE-R, and Swift XRT/UVOT observations of the unique ongoing event AT 2019avd, located in the nucleus of a previously inactive galaxy at $z=0.029$. eROSITA first observed AT 2019avd on 2020-04-
Externí odkaz:
http://arxiv.org/abs/2101.08760
Autor:
Kool, E. C., Karamehmetoglu, E., Sollerman, J., Schulze, S., Lunnan, R., Reynolds, T. M., Barbarino, C., Bellm, E. C., De, K., Duev, D. A., Fremling, C., Golkhou, V. Z., Graham, M. L., Green, D. A., Horesh, A., Kaye, S., Kim, Y. -L., Laher, R. R., Masci, F. J., Nordin, J., Perley, D. A., Phinney, E. S., Porter, M., Reiley, D., Rodriguez, H., van Roestel, J., Rusholme, B., Sharma, Y., Sfaradi, I., Soumagnac, M. T., Taggart, K., Tartaglia, L., Williams, D. R. A., Yan, L.
Publikováno v:
A&A 652, A136 (2021)
Context: Type Ibn supernovae are a rare class of stripped envelope supernovae interacting with a helium-rich CSM. The majority of the SNe Ibn reported display a surprising homogeneity in their fast lightcurves and starforming hosts. Aims: We present
Externí odkaz:
http://arxiv.org/abs/2008.04056
Autor:
Yan, Lin, Perley, D., Schulze, S., Lunnan, R., Sollerman, J., De, K., Chen, Z., Fremling, C., Gal-Yam, A., Taggart, K., Chen, T. W., Andreoni, I., Bellm, E. C., Cunningham, V., Dekany, R., Duev, D., Fransson, C., Laher, R., Hankins, M., Ho, A., Jencson, J., Kaye, S., Kulkarni, S., Kasliwal, M., Golkhou, V., Graham, M., Masci, F., Miller, A., Neill, J., Ofek, E., Porter, M., Mróz, P., Reiley, D., Riddle, R., Rigault, M, Rusholme, B., Shupe, D., Soumagnac, M., Smith, R., Tartaglia, L., Yao, Y., Yaron, O.
Helium is expected to be present in the ejecta of some hydrogen-poor superluminous supernovae (SLSN-I). However, so far only one event, PTF10hgi has been identified with He features in its photospheric spectra (Quimby et al. 2018). We present the dis
Externí odkaz:
http://arxiv.org/abs/2006.13758