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LVL Data Deliveries
What is available?
LVL delivers images, for Spitzer+optical+UV data.
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.
Delivery information listed in reverse chronological order
| Date | Delivery description |
Data version |
Direct data access |
IRSA search engine (QA) status |
| 2009-12-15 |
Final delivery: GALEX images for 249 galaxies and Halpha and R-band images for 175 galaxies. |
N/A |
data access |
IRSA search |
| 2009-07-31 |
Cumulative delivery of 256 galaxies for MIPS and 76 reprocessed archival galaxies for IRAC. Including all deliveries to date, now 256 galaxies have IRAC and MIPS data. For 38 galaxies, additional 70 um mosaics with values interpolated over low-weight pixels are provided.
See delivery documentation. |
S18 |
data access |
IRSA search |
| 2009-02-27 |
IRAC and MIPS images for 31 more galaxies.
DELIVERY DOCUMENTATION. |
S16, S17, S18 |
data access |
IRSA search |
| 2008-09-30 |
IRAC and MIPS images of 136 galaxies within the 11Mpc local volume.
DELIVERY DOCUMENTATION. |
S16, S17, S18 |
data access |
IRSA search |
| 2008-05-15 |
GALEX, H alpha, IRAC, and MIPS images of 12 galaxies within the 11Mpc local volume.
DELIVERY DOCUMENTATION. |
S16, S17 |
data access |
IRSA search |
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 Data Archive and Data Analysis & Tools.
To access data specifically from LVL, you can search by program id 40204.
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