Optical novae: the major class of supersoft X-ray sources in M 31
Not Available
Pietsch, W. et al.
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8
2006
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Optical observations of GRB 060218/SN 2006aj and its host galaxyThe supernova SN 2006aj associated with GRB 060218 is the second-closest GRB-SN observed to date (z=0.033) and is the clearest example of a SN associated with a Swift GRB with the earliest optical spectroscopy. Its optical data showed that this is the fastest evolving and among the least luminous GRB-SNe (70% as luminous as SN1998bw). However, itsFerrero, Patrizia et al.
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82007 -
Optical Observations of Space Debris in High-Altitude OrbitsNot AvailableSchildknecht, T. et al.
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82005 -
Optical photometry and Halpha Spectroscopy of SWIFT J1910.2-0546/MAXI J1910-057We report on optical photometry and spectroscopy of the black hole X-ray transient Swift J1910.2-0546/MAXI J1910-057 (Krimm at al. ATel #4139, Usui et al. ATel #4140). R-band photometry (time resolution 27s) over an interval of 3.1 hr was obtained using ALFOSC on the 2.5m Nordic Optical Telescope (NOT) on the night of 21 July 2012. The light curveCasares, J. et al.
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82012 -
Optical polarimetric monitoring of the type II-plateau SN 2005afAims.Core-collapse supernovae may show significant polarization that implies non-spherically symmetric explosions. We observed the type II-plateau SN 2005af using optical polarimetry in order to verify whether any asphericity is present in the supernova temporal evolution. Methods: .We used the IAGPOL imaging polarimeter to obtain optical linearPereyra, A. et al.
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82006 -
Optical re-brightening of the black hole transient XTE J1752-223We observed the black hole candidate XTE J1752-223 (ATel #2258) with the William Herschel Telescope (WHT) and the ACAM imager/spectrograph at the Observatorio del Roque de los Muchachos, La Palma, Spain. Two R-band exposures of 60 and 200 s and one I-band exposure of 200 s were taken under photometric conditions and 1.0-1.2-arcsec seeing on Aug 8Corral-Santana, J. M. et al.
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82010