Lyman-alpha Emission Objects

Three small fields near radio galaxy MRC 1138-262 as observed with VLT ANTU + FORS1 in a narrow-band filter at the redshifted wavelength of Lyman-alpha emission in that galaxy (left) and a broader filter in the surrounding spectral region (right), respectively. Three excellent candidates of Lyman-alpha emitters are seen at the centres of the fields. They are clearly visible in the narrow-band image (that mostly shows the gas), but are not detected in the broad-band image (that mostly shows the stars). Each field measures 24 x 24 arcsec 2, corresponding to about 620,000 x 620,000 light-years (190 x 190 kpc); North is up and East is left.

Narrow and broad-band imaging was carried out on April 12 and 13, 1999, with the ESO VLT ANTU (UT1), using the FORS1 multi-mode instrument in imaging mode. A narrow-band filter was used which has a central wavelength of 381.4 nm and a bandpass of 6.5 nm. For MRC 1138-262 (redshift z = 2.2), the emission of Lyman-alpha at 121.6 nm is redshifted to 383.8 nm, which falls in this narrow band. The broad-band filter was a Bessel-B with central wavelength of 429.0 nm. The detector was a Tektronix CCD with 2048 x 2046 pixels and an image scale of 0.20 arcsec/pixel. Eight separate 30-min exposures were taken in the narrow band and six 5-min in the broad band, shifted by about 20 arcsec with respect to each other to minimize problems due to flat-fielding and to facilitate cosmic ray removal. The average seeing was 1.0 arcsec. Image reduction was carried out by means of the IRAF reduction package. The individual images were bias subtracted and flat-fielded using twilight exposures (narrow band) or an average of the unregistered science exposures (broad-band). The images were then registered by shifting them in position by an amount determined from the location of several stars on the CCD. The registered images were co-added and dark pixels from cosmic rays were cleaned. To improve the signal-to-noise ratio, the resulting images were smoothed with a Gaussian function having full-width-at half-maximum (FWHM) = 1 arcsec (5 pixels).

Credit:

ESO

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About the Image

Id:eso9939b
Type:Observation
Release date:30 July 1999
Related releases:eso9939
Size:1982 x 2572 px

About the Object

Name:MRC 1138-262
Type:• X - Cosmology

Image Formats

Large JPEG
527.3 KB
Screensize JPEG
184.9 KB

Wallpapers

1024x768
123.7 KB
1280x1024
180.0 KB
1600x1200
224.5 KB
1920x1200
237.4 KB
2048x1536
311.9 KB

Colours & filters

BandWavelengthTelescope
Optical 381 nm Very Large Telescope
FORS1
Optical
B
429 nm Very Large Telescope
FORS1

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