Please read the following table in HTML format from a webpage and then answer the question in detail according to the table. Each table cell is defined by a <td> and a </td> tag. Each table row starts with a <tr> and ends with a </tr> tag. 'rowspan=m' and 'colspan=n' represents a cell spaning over 'm' rows and 'n' columns.

Webpage title:
Hubble Deep Field South
Table title:
Observations
Table:
<table id='hittask' contenteditable='False'>
<tr> <th colspan=1 rowspan=1 > Camera </th><th colspan=1 rowspan=1 > Filter </th><th colspan=1 rowspan=1 > Wavelength </th><th colspan=1 rowspan=1 > Total exposure time </th><th colspan=1 rowspan=1 > Exposures </th></tr>
<tr> <td class="highlighted"  colspan=1 rowspan=1 > WFPC2 </td><td colspan=1 rowspan=1 > F300W </td><td class="highlighted"  colspan=1 rowspan=1 > 300 nm (U-band) </td><td colspan=1 rowspan=1 > 140,400 s </td><td colspan=1 rowspan=1 > 106 </td></tr>
<tr> <td class="highlighted"  colspan=1 rowspan=1 > WFPC2 </td><td colspan=1 rowspan=1 > F450W </td><td class="highlighted"  colspan=1 rowspan=1 > 450 nm (B-band) </td><td colspan=1 rowspan=1 > 103,500 s </td><td colspan=1 rowspan=1 > 67 </td></tr>
<tr> <td class="highlighted"  colspan=1 rowspan=1 > WFPC2 </td><td colspan=1 rowspan=1 > F606W </td><td class="highlighted"  colspan=1 rowspan=1 > 606 nm (V-band) </td><td colspan=1 rowspan=1 > 99,300 s </td><td colspan=1 rowspan=1 > 53 </td></tr>
<tr> <td class="highlighted"  colspan=1 rowspan=1 > WFPC2 </td><td colspan=1 rowspan=1 > F814W </td><td class="highlighted"  colspan=1 rowspan=1 > 814 nm (I-band) </td><td colspan=1 rowspan=1 > 113,900 s </td><td colspan=1 rowspan=1 > 57 </td></tr>
<tr> <td colspan=1 rowspan=1 > NICMOS NIC3 </td><td colspan=1 rowspan=1 > F110W </td><td colspan=1 rowspan=1 > 1,100 nm (J-band) </td><td colspan=1 rowspan=1 > 162,600 s </td><td colspan=1 rowspan=1 > 142 </td></tr>
<tr> <td colspan=1 rowspan=1 > NICMOS NIC3 </td><td colspan=1 rowspan=1 > F160W </td><td colspan=1 rowspan=1 > 1,600 nm (H-band) </td><td colspan=1 rowspan=1 > 171,200 s </td><td colspan=1 rowspan=1 > 150 </td></tr>
<tr> <td colspan=1 rowspan=1 > NICMOS NIC3 </td><td colspan=1 rowspan=1 > F222M </td><td colspan=1 rowspan=1 > 2,220 mm (K-band) </td><td colspan=1 rowspan=1 > 105,000 s </td><td colspan=1 rowspan=1 > 102 </td></tr>
<tr> <td colspan=1 rowspan=1 > STIS </td><td colspan=1 rowspan=1 > 50CCD </td><td colspan=1 rowspan=1 > 350–950 nm </td><td colspan=1 rowspan=1 > 155,600 s </td><td colspan=1 rowspan=1 > 67 </td></tr>
<tr> <td colspan=1 rowspan=1 > STIS </td><td colspan=1 rowspan=1 > F28X50LP </td><td colspan=1 rowspan=1 > 550–960 nm </td><td colspan=1 rowspan=1 > 49,800 s </td><td colspan=1 rowspan=1 > 64 </td></tr>
<tr> <td colspan=1 rowspan=1 > STIS </td><td colspan=1 rowspan=1 > MIRFUV </td><td colspan=1 rowspan=1 > 150–170 nm </td><td colspan=1 rowspan=1 > 52,100 s </td><td colspan=1 rowspan=1 > 25 </td></tr>
<tr> <td colspan=1 rowspan=1 > STIS </td><td colspan=1 rowspan=1 > MIRNUV </td><td colspan=1 rowspan=1 > 160–320 nm </td><td colspan=1 rowspan=1 > 22,600 s </td><td colspan=1 rowspan=1 > 12 </td></tr>
<tr> <td colspan=1 rowspan=1 > Spectroscopy </td><td colspan=1 rowspan=1 > G430M </td><td colspan=1 rowspan=1 > 302.2–356.6 nm </td><td colspan=1 rowspan=1 > 57,100 s </td><td colspan=1 rowspan=1 > 61 </td></tr>
<tr> <td colspan=1 rowspan=1 > Spectroscopy </td><td colspan=1 rowspan=1 > G140L </td><td colspan=1 rowspan=1 > 115–173 nm </td><td colspan=1 rowspan=1 > 18,500 s </td><td colspan=1 rowspan=1 > 8 </td></tr>
<tr> <td colspan=1 rowspan=1 > Spectroscopy </td><td colspan=1 rowspan=1 > E230M </td><td colspan=1 rowspan=1 > 227.8–312 nm </td><td colspan=1 rowspan=1 > 151,100 s </td><td colspan=1 rowspan=1 > 69 </td></tr>
<tr> <td colspan=1 rowspan=1 > Spectroscopy </td><td colspan=1 rowspan=1 > G230L </td><td colspan=1 rowspan=1 > 157–318 nm </td><td colspan=1 rowspan=1 > 18,400 s </td><td colspan=1 rowspan=1 > 12 </td></tr>
</table>
Question:
What wavelengths do the WFPC2 images isolate?
Answer:
The WFPC2 images isolate wavelengths at 300, 450, 606 and 814 nanometres