The Spitzer Space Telescope currently operates in the "Beyond Era", over nine years past an original cryogenic mission. As the astronomy community continues to advance scientific boundaries and push beyond original specifications, the stability of the Infrared Array Camera (IRAC) instrument is paramount. The Instrument Team (IST) monitors the pointing accuracy, temperature, and calibration and provides the information in a timely manner to observers. The IRAC IST created a calibration trending web page, available to the general astronomy community, where the team posts updates of three most pertinent scientific stability measures of the IRAC data: calibration, bias, and bad pixels. In addition, photometry and telescope properties from all t...
Spitzer observations of exoplanets routinely yield accuracies of better than one part in 10,000. How...
The Spitzer Space Telescope Infrared Array (IRAC) offers a rare opportunity to measure distances and...
We present several corrections for point-source photometry to be applied to data from the Infrared A...
The Spitzer Space Telescope currently operates in the "Beyond Era", over nine years past an original...
In more than ten years of operations, the Spitzer Space Telescope has conducted a wide range of inve...
The Spitzer space telescope (Spitzer) is currently NASA's largest and most sensitive infrared (IR) t...
Significant improvements in our understanding of various photometric effects have occurred in the mo...
We present an analysis of the stability of the Infrared Array Camera (IRAC) on board the Spitzer Spa...
The Infrared Array Camera (IRAC) on the Spitzer Space Telescope has been used to measure < 10^(-4) t...
The Spitzer Space Telescope Infrared Array Camera (IRAC) basic calibrated data reduction pipeline is...
The Spitzer Space Telescope Infrared Array Camera (IRAC) is the only space-based instrument currentl...
The Spitzer Space Telescope Infrared Array (IRAC) offers a rare opportunity to measure distances and...
Spitzer observations of exoplanets routinely yield photometric accuracies of better than one part in...
We present an overview of the calibration and properties of data from the IRAC instrument aboard the...
The Infrared Array Camera (IRAC) is now the only science instrument in operation on the Spitzer Spac...
Spitzer observations of exoplanets routinely yield accuracies of better than one part in 10,000. How...
The Spitzer Space Telescope Infrared Array (IRAC) offers a rare opportunity to measure distances and...
We present several corrections for point-source photometry to be applied to data from the Infrared A...
The Spitzer Space Telescope currently operates in the "Beyond Era", over nine years past an original...
In more than ten years of operations, the Spitzer Space Telescope has conducted a wide range of inve...
The Spitzer space telescope (Spitzer) is currently NASA's largest and most sensitive infrared (IR) t...
Significant improvements in our understanding of various photometric effects have occurred in the mo...
We present an analysis of the stability of the Infrared Array Camera (IRAC) on board the Spitzer Spa...
The Infrared Array Camera (IRAC) on the Spitzer Space Telescope has been used to measure < 10^(-4) t...
The Spitzer Space Telescope Infrared Array Camera (IRAC) basic calibrated data reduction pipeline is...
The Spitzer Space Telescope Infrared Array Camera (IRAC) is the only space-based instrument currentl...
The Spitzer Space Telescope Infrared Array (IRAC) offers a rare opportunity to measure distances and...
Spitzer observations of exoplanets routinely yield photometric accuracies of better than one part in...
We present an overview of the calibration and properties of data from the IRAC instrument aboard the...
The Infrared Array Camera (IRAC) is now the only science instrument in operation on the Spitzer Spac...
Spitzer observations of exoplanets routinely yield accuracies of better than one part in 10,000. How...
The Spitzer Space Telescope Infrared Array (IRAC) offers a rare opportunity to measure distances and...
We present several corrections for point-source photometry to be applied to data from the Infrared A...