Near-IR follow-up on GRB971227: #028 Message from: S. Klose, Thueringer Landessternwarte Tautenburg, Germany, klose@tls-tautenburg.de The 1.5 arcmin radius error box of GRB 971227 (Piro et al., IAUC 6797) was imaged with the Calar Alto 2.2-m telescope on January 9.1 UT using one of the MAGIC near-infrared cameras. The total integration time was 5000 seconds in the K'-band and 5000 seconds in the J-band, centered at RA, DEC (J2000) = 12:57:15.0, 59:24:02. MAGIC was used in its wide-field mode giving a field of view of 415 times 415 arcsec. The sky was clear, but the sky conditions presumably not very photometric. Final images and final results of the data reduction will be published within about 2-4 weeks. Preliminary results of the image reduction can already be obtained via http://www.tls-tautenburg.de/research/grb.html. Both, the J and the K'-band image are obtained by combining 1000 frames taken at 5 overlapping positions. If the optical counterpart of the GRB afterglow is strongly affected by extinction, then the most promising candidates for the NIR counterpart might be very red and faint objects. Two such objects are visible in the GRB error box. Both have only a faint counterpart on the Keck R-band image published by Djorgovski et al. (GCN #025). Coordinates are (+/- 2"): Object A: RA, DEC (J2000) = 12:57:10.3, 59:24:14 Object B: RA, DEC (J2000) = 12:57:22.8, 59:23:48. A photometry has still not been performed, but one can guess that both objects might have K' = 19.0 +/- 1.0. The most promising object is object A. Currently, it seems unlikely that this is an artifact, but remind please, these are preliminary data. At the moment it is impossible to decide whether one object is physically related to GRB 971227, or whether both objects are only very red objects in the field. To be careful, one should assume the latter. ROSAT/HRI data could help. This message may be cited. Please send any communications to klose@tls-tautenburg.de