Zobrazeno 1 - 10
of 227
pro vyhledávání: '"Pojmański, G."'
Autor:
Holoien, T. W.-S., Brown, J. S., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Prieto, J. L., Dong, Subo, Brimacombe, J., Bishop, D. W., Basu, U., Beacom, J. F., Bersier, D., Chen, Ping, Danilet, A. B., Falco, E., Godoy-Rivera, D., Goss, N., Pojmanski, G., Simonian, G. V., Skowron, D. M., Thompson, Todd A., Woźniak, P. R., Ávila, C. G., Bock, G., Carballo, J.-L. G., Conseil, E., Contreras, C., Cruz, I., Andújar, J. M. F., Guo, Zhen, Hsiao, E. Y., Kiyota, S., Koff, R. A., Krannich, G., Madore, B. F., Marples, P., Masi, G., Morrell, N., Monard, L. A. G., Munoz-Mateos, J. C., Nicholls, B., Nicolas, J., Wagner, R. M., Wiethoff, W. S.
This manuscript presents information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during 2015, its second full year of operations. The same information is presented for bright (m(V)
Externí odkaz:
http://hdl.handle.net/10150/623927
http://arizona.openrepository.com/arizona/handle/10150/623927
http://arizona.openrepository.com/arizona/handle/10150/623927
Autor:
Shappee, B. J., Piro, A. L., Holoien, T. W.-S., Prieto, J. L., Contreras, C., Itagaki, K., Burns, C. R., Kochanek, C. S., Stanek, K. Z., Alper, E., Basu, U., Beacom, J. F., Bersier, D., Brimacombe, J., Conseil, E., Danilet, A. B., Dong, Subo, Falco, E., Grupe, D., Hsiao, E. Y., Kiyota, S., Morrell, N., Nicolas, J., Phillips, M. M., Pojmanski, G., Simonian, G., Stritzinger, M., Szczygieł, D. M., Taddia, F., Thompson, T. A., Thorstensen, J., Wagner, M. R., Woźniak, P. R.
On 2014 December 9.61, the All-sky Automated Survey for SuperNovae (ASAS-SN or "Assassin") discovered ASASSN-141p just similar to 2 days after first light using a global array of 14 cm diameter telescopes. ASASSN-141p went on to become a bright super
Externí odkaz:
http://hdl.handle.net/10150/621393
http://arizona.openrepository.com/arizona/handle/10150/621393
http://arizona.openrepository.com/arizona/handle/10150/621393
Observations of the star EPIC 220208795 (2MASS J01105556+0018507) reveal a single, deep and asymmetric eclipse, which we hypothesize is due to an eclipsing companion surrounded by a tilted and inclined opaque disk, similar to those seen around V928 T
Externí odkaz:
http://arxiv.org/abs/2110.15086
Autor:
Jayasinghe, T., Kochanek, C. S., Stanek, K. Z., Shappee, B. J., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, Subo, Pawlak, M., Pejcha, O., Pojmanski, G., Otero, S., Hurst, N., Will, D.
The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline (${\sim}4$ yrs) $V-$band light curves for sources brighter than V$\lesssim17$ mag across the whole sky. We produced V-band light curves for a total of ${\sim}61.5$ million s
Externí odkaz:
http://arxiv.org/abs/2006.10057
Autor:
Jayasinghe, T., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Pinsonneault, M. H., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Pawlak, M., Pejcha, O., Pojmanski, G., Otero, S., Hurst, N., Will, D.
We characterize ${\sim} 71,200$ W UMa type (EW) contact binaries, including ${\sim} 12,600$ new discoveries, using ASAS-SN $V$-band all-sky light curves along with archival data from Gaia, 2MASS, AllWISE, LAMOST, GALAH, RAVE, and APOGEE. There is a c
Externí odkaz:
http://arxiv.org/abs/1911.09685
Autor:
Jayasinghe, T., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, Subo, Pawlak, M., Pejcha, O., Shields, J. V., Pojmanski, G., Otero, S., Hurst, N., Britt, C. A., Will, D.
The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline (${\sim}4$ yrs) light curves for sources brighter than V$\lesssim17$ mag across the whole sky. As part of our effort to characterize the variability of all the stellar sourc
Externí odkaz:
http://arxiv.org/abs/1907.10609
Autor:
Pawlak, Michal, Pejcha, O., Jakubcik, P., Jayasinghe, T., Kochanek, C. S., Stanek, K. Z., Shappee, B. J., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, S., Shields, J. V., Pojmanski, G., Britt, C. A., Will, D.
We explore the synergy between photometric and spectroscopic surveys by searching for periodic variable stars among the targets observed by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) using photometry from the All-Sky Automate
Externí odkaz:
http://arxiv.org/abs/1906.06340
Autor:
Jayasinghe, T., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, Subo, Pawlak, M., Pejcha, O., Shields, J. V., Pojmanski, G., Otero, S., Hurst, N., Britt, C. A., Will, D.
The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline (${\sim}4$ yrs) light curves for sources brighter than V$\lesssim17$ mag across the whole sky. The Transiting Exoplanet Survey Satellite (TESS) has started to produce high-q
Externí odkaz:
http://arxiv.org/abs/1901.00009
Autor:
Holoien, T. W. -S., Brown, J. S., Vallely, P. J., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Prieto, J. L., Dong, Subo, Brimacombe, J., Bishop, D. W., Bose, S., Beacom, J. F., Bersier, D., Chen, Ping, Chomiuk, L., Falco, E., Holmbo, S., Jayasinghe, T., Morrell, N., Pojmanski, G., Shields, J. V., Strader, J., Stritzinger, M. D., Thompson, Todd A., Wozniak, P. R., Bock, G., Cacella, P., Carballo, J. G., Conseil, E., Cruz, I., Farfan, R. G., Fernandez, J. M., Kiyota, S., Koff, R. A., Krannich, G., Marples, P., Masi, G., Monard, L. A. G., Munoz, J. A., Nicholls, B., Post, R. S., Stone, G., Trappett, D. L., Wiethoff, W. S.
Publikováno v:
MNRAS, 484, 1899 (2019)
In this catalog we compile information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) as well as all other bright ($m_{peak}\leq17$), spectroscopically confirmed supernovae found in 2017, totaling 308 supernova
Externí odkaz:
http://arxiv.org/abs/1811.08904
Autor:
Jayasinghe, T., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Holoien, T. W. -S., Thompson, Todd A., Prieto, J. L., Dong, Subo, Pawlak, M., Pejcha, O., Shields, J. V., Pojmanski, G., Otero, S., Britt, C. A., Will, D.
The variable stars in the VSX catalog are derived from a multitude of inhomogeneous data sources and classification tools. This inhomogeneity complicates our understanding of variable star types, statistics, and properties, and it directly affects at
Externí odkaz:
http://arxiv.org/abs/1809.07329