JHKs[3.5][4.5] photometry of NGC 3372 (Tapia+, 2006)

Details JHKs[3.5][4.5] photometry of NGC 3372 (Tapia+, 2006) JHKs[3.5][4.5] photometry of NGC 3372 (Tapia+, 2006)

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..73670513t&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/367/513. Originally published in: 2006MNRAS.367..513T

Physics

H Ii Regions, Molecular Clouds, Photometry: Infrared

Scientific paper

The narrow-band optical images in several of the most important atomic lines and neighbouring continuum were secured at Las Campanas Observatory (LCO) in 1994 March 17-22, using the 40-in. telescope (LCO-40) and the TEK1 1024x1024 pixel detector. The narrow-band filters are centred in the following emission lines: H{beta}, [OIII] 5007{AA}, Hα, [NII] 6584{AA} and [SII] 6731{AA}. Additionally, a filter centred at 6724{AA} lets through both lines of the [SII] doublet. Continuum images were taken with filters centred at 3792, 4772, 5954 and 6253{AA}.
The near-infrared images were obtained during two runs, with the Clay and Baade Magellan telescopes and Persson's Auxiliary Nasmyth Infrared Camera (PANIC) attached. The JHK frames were obtained in 2003 May 17 on the Clay telescope.
In 2004 April 2, a quick survey of a small region of size 40x30arcsec2 (fully sampled region) centred at RA=10:43:26.7, DE=-59:34:37 (J2000) was performed at 8.9m (0.78m FWHM), 9.8m (0.93m FWHM) and 11.9m (1.16m FWHM) with TIMMI2 on the European Southern Observatory (ESO) 3.6-m telescope at La Silla.
(1 data file).

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