Zobrazeno 1 - 10
of 16
pro vyhledávání: '"J. E. Thomas-Osip"'
Autor:
Wojtek Krzeminski, Nidia Morrell, Gaspar Galaz, Louis Gregory Strolger, Andrew C. Phillips, Thomas de Jaeger, G. Folatelli, John S. Mulchaey, William Sherry, Lluís Galbany, L. Wells, Tania Moraga, M. Malkan, José Maza, Kevin Krisciunas, Alessandro Pizzella, Patrick J. McCarthy, Nicholas B. Suntzeff, J. E. Thomas-Osip, E. M. Green, Charles F. Prosser, Joseph P. Anderson, Mario Hamuy, Mark M. Phillips, R. Antezana, Santiago González-Gaitán, Gerard M. Williger, Luis González, Robert A. Schommer, Claudia P. Gutiérrez, Brian P. Schmidt, Sofia Kirhakos, Maximilian Stritzinger, Claudio Anguita, Chris Impey, Yong-Cheol Kim, Marina Wishnjewski
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Astronomical Journal, vol 151, iss 2
Galbany, L, Hamuy, M, Phillips, M M, Suntzeff, N B, Maza, J, de Jaeger, T, Moraga, T, González-Gaitán, S, Krisciunas, K, Morrell, N I, Thomas-Osip, J, Krzeminski, W, González, L, Antezana, R, Wishnjewski, M, McCarthy, P, Anderson, J P, Gutiérrez, C P, Stritzinger, M, Folatelli, G, Anguita, C, Galaz, G, Green, E M, Impey, C, Kim, Y-C, Kirhakos, S, Malkan, M A, Mulchaey, J S, Phillips, A C, Pizzella, A, Prosser, C F, Schmidt, B P, Schommer, R A, Sherry, W, Strolger, L-G, Wells, L A & Williger, G M 2016, ' UBVRIz Light Curves of 51 Type II Supernovae ', The Astronomical Journal, vol. 151, no. 2, pp. 33 . https://doi.org/10.3847/0004-6256/151/2/33
The Astronomical Journal, vol 151, iss 2
NASA Astrophysics Data System
Galbany, L; Hamuy, M; Phillips, MM; Suntzeff, NB; Maza, J; de Jaeger, T; et al.(2016). UBVRIz LIGHT CURVES OF 51 TYPE II SUPERNOVAE. ASTRONOMICAL JOURNAL, 151(2). doi: 10.3847/0004-6256/151/2/33. UCLA: Retrieved from: http://www.escholarship.org/uc/item/5v79n0tj
CIÊNCIAVITAE
Universidad Nacional de La Plata
instacron:UNLP
Astronomical Journal, vol 151, iss 2
Galbany, L, Hamuy, M, Phillips, M M, Suntzeff, N B, Maza, J, de Jaeger, T, Moraga, T, González-Gaitán, S, Krisciunas, K, Morrell, N I, Thomas-Osip, J, Krzeminski, W, González, L, Antezana, R, Wishnjewski, M, McCarthy, P, Anderson, J P, Gutiérrez, C P, Stritzinger, M, Folatelli, G, Anguita, C, Galaz, G, Green, E M, Impey, C, Kim, Y-C, Kirhakos, S, Malkan, M A, Mulchaey, J S, Phillips, A C, Pizzella, A, Prosser, C F, Schmidt, B P, Schommer, R A, Sherry, W, Strolger, L-G, Wells, L A & Williger, G M 2016, ' UBVRIz Light Curves of 51 Type II Supernovae ', The Astronomical Journal, vol. 151, no. 2, pp. 33 . https://doi.org/10.3847/0004-6256/151/2/33
The Astronomical Journal, vol 151, iss 2
NASA Astrophysics Data System
Galbany, L; Hamuy, M; Phillips, MM; Suntzeff, NB; Maza, J; de Jaeger, T; et al.(2016). UBVRIz LIGHT CURVES OF 51 TYPE II SUPERNOVAE. ASTRONOMICAL JOURNAL, 151(2). doi: 10.3847/0004-6256/151/2/33. UCLA: Retrieved from: http://www.escholarship.org/uc/item/5v79n0tj
CIÊNCIAVITAE
We present a compilation of UBVRIz light curves of 51 type II supernovae discovered during the course of four different surveys during 1986-2003: the Cerro Tololo Supernova Survey, the Calán/Tololo Supernova Program (C&T), the Supernova Optical and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::91b211a47b8732b00fbe1d23c5dd6240
http://sedici.unlp.edu.ar/handle/10915/86651
http://sedici.unlp.edu.ar/handle/10915/86651
Autor:
Richard D. Allen, Jennifer L. Marshall, J. P. Rheault, G. Prieto, A. Berdja, Darren L. DePoy, Steven Villanueva, J. E. Thomas-Osip, D. W. Carona, K. W. Cook
Publikováno v:
Publications of the Astronomical Society of the Pacific. 124:84-93
In order to guide the adaptive optics design and aid in performance predictions, optical turbulence at the site of the future Giant Magellan Telescope (GMT) is characterized using MooSci, a lunar scintillometer, and MASS-DIMM, a combination different
Autor:
K. S. Jarvis, S. L. Leeds, Susan M. Lederer, Deborah L. Domingue, J. E. Thomas-Osip, David J. Osip, Faith Vilas
Publikováno v:
Earth, Planets and Space. 60:49-59
We present an analysis of Hapke photometric modeling applied to uniform ground-based UBVRIJHK broadband data of asteroid 25143 Itokawa collected over a wide range of solar phase angles (4°–130°) during the 2004 apparition (Thomas-Osip et al., thi
Autor:
Faith Vilas, J. E. Thomas-Osip, David J. Osip, Susan M. Lederer, K. S. Jarvis, Deborah L. Domingue, S. L. Leeds
Publikováno v:
Earth, Planets and Space. 60:39-48
In 2004, Asteroid 25143 Itokawa made its final close approach to the Earth prior to its encounter with the Japanese spacecraft Hayabusa. This apparition was superb with Itokawa reaching magnitude 12 (two magnitudes brighter than the 2001 apparition a
Publikováno v:
Icarus. 180:453-463
The surface reflectance properties of the irregular outer planets satellites are probed for evidence for the presence of aqueous alteration products on their surfaces using the strong correlation between the 3.0-μm water of hydration absorption feat
Publikováno v:
Icarus. 179:511-522
A combination of laboratory experiments, theoretical modeling, and spacecraft observations is employed to characterize the aerosols in the atmosphere of Titan. The scattering properties of model aerosols were measured using the Microwave Analog Light
Publikováno v:
Icarus. 153:285-294
On 1995 August 21, Saturn's moon Titan occulted the 13th magnitude star GSC5254-00997. The predawn event was observed at 2.3 μm with the NASA 3.0-m Infrared Telescope Facility. We measured the average atmospheric scale height between latitudes 50°S
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
We report preliminary results from optical turbulence measurements carried out in 2010 at Cerro Las Campanas, the future site for the Giant Magellan Telescope (GMT). The instruments involved are MooSci, a lunar scintillometer for the near-ground opti
Autor:
Matt Johns, Patrick J. McCarthy, David A. Naylor, Andrew McWilliam, G. Prieto, Richard Querel, Mark M. Phillips, J. E. Thomas-Osip
Publikováno v:
SPIE Proceedings.
Cerro Las Campanas located at Las Campanas Observatory (LCO) in Chile has been selected as the site for the Giant Magellan Telescope. We report results obtained since the commencement, in 2005, of a systematic site testing survey of potential GMT sit
Publikováno v:
SPIE Proceedings.
Cerro Las Campanas located at Las Campanas Observatory in Chile has been selected as the site for the Giant Magellan Telescope. We report results obtained since the commencement, in 2005, of a systematic site testing survey of potential GMT sites at