The primary MAST HST search page (http://archive.stsci.edu/hst/search.php) now includes the means for finding, or excluding, scan data taken with any HST instrument. The update also includes "Scan Type" as a default output column on the HST Search Results page.
To enable searches for scan data (see Figure 1):
Select "Scan Type" from either the "User-specified field 1" or the “User-specified field 2" pull-down menu.
Set "Field Description" to "!\null" in order to locate only scanned data.
Adjust any other desired qualifiers. In the example shown, we restrict the search to WFC3 data only. Then select "Search".
Figure 2 illustrates the output from a sample search for any scanned WFC3 data. The output has been sorted in time-order, showing the oldest images at the top, by clicking on the “Start Time” column heading. Note the new "Scan Type" column; all WFC3 and other current instrument scans will be of type “C” (continuous) only. Earlier instruments such as FOC, FOS, WFPC2, etc. took both “C” and “D" (dwell) type scans; the D scan is no longer available as an observing option.
Normal staring mode images will have a blank "Scan Type". To exclude scans from the MAST search and locate only staring mode observations, set the "Field Description" to "\null".
Any questions regarding accessing scanned HST data from the MAST archive can be sent to firstname.lastname@example.org.
With no future space ultraviolet instruments currently planned, the data from the UV spectrographs aboard the Hubble Space Telescope have a legacy value beyond their initial science goals. Since Cycle 24, the astronomical community has been offered a novel way of mining the Hubble data archive through the Hubble Spectroscopic Legacy Archive (HSLA). This archive provides quicklook spectra for raw COS/FUV, coadded COS/FUV spectra and raw COS/NUV data, as well as tools for measuring signal-to-noise and flux variability.
We announce the second release of the HSLA. In this release, all public raw COS/FUV spectra, all COS/FUV coadded spectra, and all raw COS/NUV spectra accessible through the HSLA are using the latest updates to the COS/FUV and COS/NUV reference files. The HSLA contents are also augmented with all COS datasets that entered the public domain since March 2016. The HSLA products are available on MAST at: https://archive.stsci.edu/hst/spectral_legacy/ together with a description of their contents. Questions about the content of the HSLA can be sent to email@example.com.
POLAR (Barros et al. 2016) is a set of detrended light curves from K2 Campaigns 1-6. The team makes use of a pipeline to reduce target pixel files, including optimized apertures and decorrelations of systematic noise dominated by the frequent thruster firings of the spacecraft to maintain pointing. The pipeline is optimized for bright stars, and achieves a maximum precision of six ppm over six hours. In addition, the team uses their detrended light curves to search for exoplanets and eclipsing binaries. The team has provided the detrended light curves, catalogs of exoplanets and eclipsing binaries, and summary plots containing statistics on the detected objects.
The STARBurst IRregular Dwarf Survey (STARBIRDS; PI: Kristen McQuinn) is a collection of new and archival observations for twenty nearby (d < 6 Mpc) starburst and post-starburst dwarf galaxies. The first public release includes flux-calibrated and background-subtracted images – all registered to a common world coordinate system -- from GALEX (FUV and NUV), HST (V and I), and Spitzer (MIPS). In addition, three complementary sets of images are available: (1) a set of GALEX and Spitzer images cropped to match the field-of-view of HST; (2) HST images convolved and rebinned to match GALEX and Spitzer resolutions; and (3) GALEX images with a field-of-view extending significantly beyond optical diameter observed with HST. Future updates to the archive include additional data from Chandra, Spitzer IRAC, ground-based H-alpha, and Green Bank Telescope neutral hydrogen imaging.
This newsletter is a MAST publication produced by Jonathan Hargis and Randy Thompson, on behalf of the entire MAST staff, who welcome your comments and suggestions.
The Mikulski Archive for Space Telescopes (MAST) is a NASA funded project to support and provide to the astronomical community a variety of astronomical data archives, with the primary focus on scientifically related data sets in the optical, ultraviolet, and near-infrared parts of the spectrum. MAST is located at the Space Telescope Science Institute (STScI).