Search VO collections, the Hubble Source Catalog, and create DOIs for data you publish |
On this page... |
The Portal enables searches of a few special collections, most of which can be selected from the collection menu.
The Virtual Observatory (VO) is composed of electronic archives from many astronomical centers around the world. These archives contain a wide variety of data and other resources, including catalogs, images, and spectra. The results of a VO search will look similar to that shown in the figure below.
A search of the VO for the target M 57. The results table shows all VO resources (images, spectra, or catalogs) within a 1 arcmin radius. The Data Load button in each row will provide more descriptive information and links to retrieve the data. |
Searching the VO with the Portal differs from a basic search in a few important respects:
VO searches are effectively simultaneous searches of multiple astronomical archives. It may take considerable time (minutes) for the last archive to return results. Since the results are displayed as they become available, it is possible to browse or download some results while others are still being loaded. |
The Hubble Source Catalog (HSC) consists of photometry of sources that have been imaged with one or more instruments on HST. MAST supports multiple ways to search the HSC; the Portal allows searches in a circular region around a user-specified position on the sky (a cone search). Searching the HSC is a form of catalog search, and the chapter on Demos and Tutorials shows several science-motivated example searches.
Although an earlier version of the HSC is still available, it is best to search the version 3 catalog (HSCv3), which is substantially better and now contains the Hubble Catalog of Variables. |
As with VO searches, an HSC search returns results that differ from a basic search in a few important respects:
A Digital Object Identifier (DOI) is a persistent link to a resource on the internet, and is often used in astronomy to provide access to specific data collections. Investigators can use a special instance of the Portal to generate a DOI for one or more datasets hosted by MAST. This will generate a permanent link that may be included in a research paper to refer to the data that were analyzed.
DOIs for many collections, including High-Level Science Products, certain catalogs, and Kepler/K2 campaigns have already been created. To use them in your work, see the detailed DOI documentation. To create a new custom DOI for data you wish to publish, see the following how-to video, or follow the written instructions below.
Create-a-DOI walkthrough video. |
Instruction | Notes | ||
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1 | Navigate to the DOI Portal at: https://mast.stsci.edu/portal/Mashup/Clients/DOI/DOIPortal.html.
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2 | Execute a Portal search for observations that include the data to be published. | ||
3 | Select rows in the results table that correspond to the specific observations to which the DOI should refer, and place them in the download basket.
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4 | Click the My DOI Basket button to bring up Download Manager, which will look something like the picture below. | ||
5 | Select the rows corresponding to the desired observation IDs and filters, then click the button to create a DOI. If you need to update an existing DOI you created, contact MAST. | ||
6 | Fill in the DOI requested metadata in the dialog box, then click the Create DOI button. |
To update a DOI you created with new information, contact the HelpDesk. |
There are three ways to access the data that a MAST DOI points to:
Resolve the DOI in your browser. For example, for the TESS Input Catalog (doi:10.17909/fwdt-2x66, from the list of pre-made MAST DOIs), the following URLs will both work:
https://dx.doi.org/10.17909/fwdt-2x66
https://archive.stsci.edu/doi/resolve/resolve.html?doi=10.17909/fwdt-2x66
These will lead you to a landing page, where you can follow a link to "display data":
Depending on the nature of the data cited by the DOI, the "display data" link will either load a set of observations in the Portal, or lead to another webpage with information about retrieving the data.
You can search for a MAST DOI's observations using the general-purpose MAST Portal as follows. This will only work if the DOI you wish to access points directly to observations in the MAST Portal. (So it won't work for the TESS Input Catalog pre-made DOI we used above. We'll instead use 10.17909/t9-z1c2-ye93, a DOI created using the MAST DOI Portal by the authors of a paper who wanted a permanent reference to the data that they employed. You would typically find a DOI like this one by encountering it in a paper.)
Instruction | Notes | |
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1 | Navigate to the Portal at: https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html | |
2 | Under the Select a collection... dropdown menu, choose Observations in a DOI. | |
3 | Enter the DOI string (e.g., 10.17909/t9-z1c2-ye93) into the search field, and click Search. |
This method will not work for certain pre-made MAST DOIs for catalogs, HLSP webpages, or bulk mission data, which point to informational webpages or custom download scripts even when the data actually are available in the Portal.
You can use the MAST DOI Portal view any DOIs that you have created using your account. You will not be able to download data using this method; see above for data retrieval options.
Instruction | Notes | ||
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1 | Navigate to the DOI Portal at: https://mast.stsci.edu/portal/Mashup/Clients/DOI/DOIPortal.html.
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2 | Select Show my DOIs in the Search by... dropdown menu, and click the Load All button. | ||
3 | Select the Show DOI Data entry in the Actions column. |
A few special searches enable access to lesser-used or mission-specific collections, which are listed in the table below.
Collection | Description |
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HSC Spectra | A collection of tens of thousands of spectra in various bands associated with sources in the Hubble Source Catalog. Many of the sources are categorized by astrophysical type. |
Hubble Spectroscopic Legacy Archive | View representative UV spectra from a variety of astrophysical objects (just over 2000 sources in all). The data include co-added spectra where possible. See the HSLA Mission page for details. |
WFC3 PSF | Search a library of observed point-spread functions (PSFs) from archived HST/WFC3 observations. These PSFs enable higher precision photometry of WFC3 observations. See PSF Search for more information about this collection. |
JWST Instrument Keywords | Search for JWST science data using header keyword metadata. See the Data Search page for more information about how to perform a search on JWST data. |
JWST WSS | Search for JWST wavefront sensing (optical path difference) data. See the Supplemental Products page for details about this and other ancillary file types. |