HLA DR7.2 release 10-23-13, improved WFC3 source lists. Now 85% of WFC3 combined images have either a SExtractor or a DAOphot source list, and the quality of the lists has been substantially improved by flagging spurious sources.
Hubble Legacy Archive Interactive Display Help
You can look at an image or 2-dimensional spectrum more carefully, and
overlay HLA source lists or external catalogs, by using the interactive display (accessible via
view). The HLA interactive display was originally based on
- The image can be moved
either by dragging using the mouse or by using the arrow buttons in the
(< > ^ v).
The o button recenters the view.
- The +
and - buttons zoom in or
out. The zoom bar shows the current zoom level; you can also click
on the zoom bar to
jump directly to a different zoom. Initially the image is displayed at
scale, with one image pixel per display pixel. The zoom changes by a
factor of two between levels
and ranges from 4 times larger (1 image
pixel per 4 display pixels) to a size where the entire image is smaller
than 256 pixels on
- The coordinate box in the upper left shows the current
position both in
X,Y pixels and in world coordinates. The world coordinates are either
the position on
the sky (RA and Dec) or, for 2-dimensional spectra, the wavelength and
the slit. Note that the wavelengths are not accurate for echelle and
spectra because they
do not have FITS header WCS keywords that describe the mapping between
and wavelength on the image.
- The third line of the coordinate box shows the actual
pixel value from the image at the mouse position when the mouse stops
- Type the S or s key on your keyboard to copy
the current cursor position into the search box on the HLA search
form. You can use this in conjunction with the
options to get quick previews from other
HLA images at the same sky position.
- Click the save icon
to save the current view. This creates a JPEG image covering
the region currently visible in the browser using the current contrast
settings. This generates a "clean" image: catalog overlays and other
graphics (e.g., the crosshair and coordinate box) are not shown. If you
want to capture the graphics as well, use your computer's screen capture
function (e.g., the Grab utility on a Macintosh).
- Click the printer icon
to print the current view.
You can also use the usual print shortcut for your browser.
- The help button opens a new window showing
Contrast and colors
- The Lighter and Darker
buttons change the
contrast. Note that the image tiles must be reloaded from the
the new contrast setting, so the results are not instantaneous. Most
cache the images, however, which makes changing back to a previous
- The advanced contrast controls link
displays a more complex set of controls. For color images, the
the Lighter and Darker
buttons can be used to adjust the color balance between the filters.
The Saturation and
Sky + and -
buttons allow adjusting the contrast parameters independently at
the bright and faint ends of the pixel values. Experimentation is the
best way to get a feel for what these buttons do; their effect varies
depending on the contents of the image. The
Reset button resets the contrast parameters
to their original values. Clicking the
advanced contrast controls link again will hide these controls.
- For color images, the filters are shown as color drop-down menus.
You can change the assignment of filters to the
bands using these menus. If the filter to color mapping is changed, the image tiles are
reloaded from the server.
- Type the L or l key on your keyboard to plot
horizontal line from the image at the current mouse position, or
type the C or c key to plot a vertical column.
The plot pops up in a new window. Note that the plot takes some time
to appear because it comes from the HLA web server (since the actual
image pixel data are not loaded into the browser.) There are controls
for zooming in on the plot, adjusting the scale, binning and smoothing
options, and units.
(e.g., equivalent width estimates) are also possible.
- Click the appropriate checkbox to overlay source lists
DAOPHOT and/or SExtractor catalogs constructed from the image. Note
the response of the display can be somewhat sluggish if the source list
is large. The source list can be hidden by clicking the checkbox again.
Keep in mind that the SExtractor sources actually use elliptical
isophotes rather than circular apertures. It is also possible to
the segmentation image that shows the actual apertures used for the
- Click the appropriate checkbox to overlay catalogs from SDSS
(Sloan Digital Sky Survey), 2MASS (Two Micron All Sky Survey), GSC2
(Guide Star Catalog 2), FIRST (Faint Images of the Radio Sky at
Twenty Centimeters) or GALEX (the Galaxy Evolution Explorer ultraviolet
survey). This can be especially useful for checking the
absolute astrometry of the image.
- You can also overlay sources from the Hubble Source Catalog (HSC),
which merges source lists from individual HLA images into a master catalog.
Note that this catalog is still in active development and is currently
in beta release.
The current version has several limitations which will be remedied
in future releases; See the
HSC Frequently Asked Questions
- The advanced HSC catalog controls provide some options when overlaying
Hubble Source Catalog objects. The Apply astrometric shift
checkbox corrects the astrometry of the HLA image using corrections that are derived
by the process that creates the HSC from individual HLA catalogs. The corrected
astrometry is used for other external catalogs that are overlaid on the image (e.g.,
2MASS). This option is available only if a shift has been determined for the image.
The Require NumImages>1 option filters the HSC to
include only objects detected in at least two images. This removes many of the
spurious sources from the catalog but also removes real sources (e.g., in fields
that have been observed in only a single filter, all objects have NumImages=1).
In some fields with many observations, it may be helpful to increase the limit
to a value larger than 1.
- Click on sources to pop up a window with information
on source positions, magnitudes, etc. If there are multiple sources
nearby or sources from several catalogs, information will be shown on
all of them. Use the All columns button
above the catalog listing to see more information, or the
Main button to get back to a limited set of