VizieR Online Data Catalog: Physical properties of SFRs in NGC 3395/NGC 3396 (Weistrop+, 2020)

The star-forming regions in NGC 3395 and NGC 3396 were identified from UBVR images obtained at the 1 m telescope at Mount Laguna Observatory on 1997 May 8 UT using the 2048x2048 CCD camera. The instrument configuration, seeing, reductions, and calibration of the images have been previously described (Weistrop et al. 2012, J/AJ/143/98).

Spectra were obtained with the 2.1 m telescope at NOAO's Kitt Peak Observatory on 1998 March 21-24 UT. The instrument configuration is described in Weistrop et al. (2012, J/AJ/143/98). Long-slit spectra at seven position angles (PA), selected to obtain spectra for as many blue regions as possible, were acquired. The individual integrations were 1000 s with the following exceptions: one 300 s integration for PA 136°, one 300 s integration for PA 12°; all integrations for PA 83° were 1500 s. The spectra were calibrated and reduced as described in Weistrop et al. (2012, J/AJ/143/98).

(3 data files).