FEPS data deliveries: history and plans
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What is available?
FEPS delivers images, source lists, spectra, and models.Please note that when a Legacy team delivers enhanced data products to IRSA, the data must go through a quality assurance (QA) and ingestion process before being available through IRSA search engines, and this process does not happen instantaneously. Direct data access to a more recent delivery may contain errors that will be caught by the QA process; an IRSA search of an older delivery permits access to data that have passed the QA process. (More information about IRSA services, the QA process, etc.)
Delivery information listed in reverse chronological order
| Date | Delivery description | data version (S version history) | Direct data access | IRSA search engine (QA) status |
|---|---|---|---|---|
| 2006-12-23 | Full re-delivery of everything. | N/A | data access | N/A |
| 2005-11-23 a.k.a. DR 3 |
Consists of images, photometry, spectra, and models for 291 stars Explanatory Supplement v. 3.0 |
S10.5, 11.2, 12.0 | data access | IRSA search |
| 2005-06-08 a.k.a. DR 2 |
Consists of images, photometry, and spectra for 150 stars Explanatory Supplement v. 2.1 |
S10.5 | data access | N/A |
| 2004-10-27 a.k.a. DR 1 |
Consists of IRAC and MIPS photometry, reduced IRS spectra, and best-fit models for 33 objects Explanatory Supplement v.1.1; additional note |
S10.5 | data access | N/A |
Getting the original Spitzer data
All of the original Spitzer data for Legacy programs are released to the community as soon as they complete end-of-campaign reprocessing (there is no proprietary period). For general information about how to access our archive (and what to do with the data when you get in), please see our archives and analysis page.To access data specifically from FEPS, you can search by this program id (pid):
- pid 148 - rubble
