Abstract
Direct CCD images of the gravitationally lensed BAL quasar H1413+117 (Bessel B, V, R, I; Gunn r and i), obtained during 1989−1994 in the framework of photometric monitorings at ESO and with the NOT, have been carefully (re-)analyzed. Simultaneous fitting of 4 PSFs, fixing the relative positions of components B, C and D with respect to A, has been achieved successfully. The relative light curves of the 4 lensed QSO images, with respect to a stable nearby comparison star, confirm the general trend already presented by Arnould et al. (1993). The amplitude of the light curves is found to be about 0.5 magnitude, peak-to-peak in the V filter. The four lensed components display brightness variations quasi-simultaneously and in parallel. In addition to these intrinsic light variations due to the source, we find that component D shows extra light variations with respect to the other components. These are very likely caused by micro-lensing.
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References
Angonin, M.-C., et al., 1990, A&A, 223, L5
Arnould, P., et al., 1993, in Gravitational Lenses in the Universe, eds. J. Surdej et al., (Liège: Université de Liège) 169
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© 1996 International Astronomical Union
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Remy, M., Gosset, E., Hutsemékers, D., Revenaz, B., Surdej, J. (1996). The Clover Leaf Quasar H1413+117: New Photometric Light Curves. In: Kochanek, C.S., Hewitt, J.N. (eds) Astrophysical Applications of Gravitational Lensing. International Astronomical Union / Union Astronomique Internationale, vol 173. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0221-3_70
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DOI: https://doi.org/10.1007/978-94-009-0221-3_70
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