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Table 2

Relative astrometry of HE 0435-1223 as derived from the simultaneous deconvolution of all NIC2 frames.

This work Morgan et al. (2005) Kochanek et al. (2006)
ID Δα (′′) Δδ (′′) Mag (F160W) Δα (′′) Δδ (′′) Δα (′′) Δδ (′′)

A 0. 0. 17.20  ±  0.01 0. 0. 0. 0.
B –1.4743  ±  0.0004 +0.5518  ±  0.0006 17.69  ±  0.01 –1.477  ±  0.002 +0.553  ±  0.002 –1.476  ±  0.003 +0.553  ±  0.001
C –2.4664  ±  0.0003 –0.6022  ±  0.0013 17.69  ±  0.02 –2.469  ±  0.002 –0.603  ±  0.002 –2.467  ±  0.002 –0.603  ±  0.004
D –0.9378  ±  0.0005 –1.6160  ±  0.0006 17.95  ±  0.01 –0.938  ±  0.002 –1.615  ±  0.002 –0.939  ±  0.002 –1.614  ±  0.001
G –1.1706  ±  0.0030 –0.5665  ±  0.0004 16.20  ±  0.12 –1.169  ±  0.002 –0.572  ±  0.002 –1.165  ±  0.002 –0.573  ±  0.002

Notes. The 1σ error bars are the internal errors after deconvolution. Additional 2-mas systematic errors must be added to these (see text). The magnitudes are in the Vega system. For comparison we show the results from Morgan et al. (2005) using HST/ACS images and from Kochanek et al. (2006) using HST/NIC2 images.

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