Difference between revisions of "Generating Light Curves - APT and Excel"
(Created page with 'Mysterious IRAC images, along with a chart indicating 3 stars for which you should perform photometry. Construct light curves by plotting your photometry as a function of time (…') |
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function of time (found in the image headers) | function of time (found in the image headers) | ||
| − | [ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/test_lightcurve_data.tar.gz] | + | [ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/test_lightcurve_data.tar.gz] Click here or paste this into browser ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/test_lightcurve_data.tar.gz |
Sample IRAC images from | Sample IRAC images from | ||
each channel for HAT-P-1b, TrES-2, and TrES-4 | each channel for HAT-P-1b, TrES-2, and TrES-4 | ||
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[ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/sample_images.tar.gz] | [ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/sample_images.tar.gz] | ||
| + | Click here or paste this into browser ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/sample_images.tar.gz | ||
Revision as of 16:28, 16 May 2010
Mysterious IRAC images, along with a chart indicating 3 stars for which you should perform photometry. Construct light curves by plotting your photometry as a function of time (found in the image headers)
[1] Click here or paste this into browser ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/test_lightcurve_data.tar.gz
Sample IRAC images from
each channel for HAT-P-1b, TrES-2, and TrES-4
[2]
Click here or paste this into browser ftp://anon-ftp.ipac.caltech.edu/outgoing/hoard/nitarp/sample_images.tar.gz
A note on IRAC image file names: Here's a sample image name...
SPITZER_I1_24745472_0002_0000_4_bcd.fits
This follows a general file naming convention, as follows:
"SPITZER" = in case you forgot which satellite you were using
"I1" = Instrument (I for IRAC) and channel number. In this case, channel 1 = 3.6 microns. Other channel possibilities include 2 = 4.5 microns, 3 = 5.8 microns, 4 = 8 microns. Note that, as described in the IRAC Data Handbook and the document on performing IRAC photometry that I circulated amongst you a while ago, these channel wavelengths are not the "true" (or isophotal) values that should be used during data analysis. The isophotal values are channel 1 = 3.544 microns, 2 = 4.479, 3 = 5.710, 4 = 7.844.
"24745472" = Unique AOR identifier for this observation (not for this IMAGE, but for all images comprising a single Spitzer visit to the target).
"0002" = Image sequence number in this observation; in this case, the second image of the sequence.
"0000" = Some observing modes obtain more than one exposure per "image". In such cases, this sequence number would increment upwards.
"4" = number of times this image has been reprocessed through successive (improved) versions of the data processing and calibration pipeline. All of the data I have sent to you (indeed, all of the IRAC data now available in the Spitzer archive) have been processed with the latest and greatest version of the pipeline, S18.7.0.
"bcd" = Basic Calibrated Data. The standard result from raw Spitzer data that have been run through the processing and calibration pipeline. This is the data product that we work with.
".fits" = It's a standard FITS image, can be loaded into DS9. The BCD images are flux calibrated in units of surface brightness per pixel, MJy/sr (mega-Jansky per steradian). The also include world coordinate solutions in their image headers, so can be displayed in the usual format (N up, E to the left) and have, for example, 2MASS catalogs overlaid on them, etc.
