Results 21 to 30 of about 924,536 (300)
WFV (Wide Field of View) cameras on-board Gaofen-1 satellite (gaofen means high resolution) provide unparalleled global observations with both high spatial and high temporal resolutions.
Juan Li +4 more
doaj +1 more source
XMM-Newton (cross)-calibration
ESA's large X-ray space observatory XMM-Newton is in its fifth year of operations. We give a general overview of the status of calibration of the five X-ray instruments and the Optical Monitor. A main point of interest in the last year became the cross-calibration between the instruments.
Kirsch, M. +9 more
openaire +3 more sources
To obtain more abundant target information for vegetation remote sensing research, the wide field of view (WFV) of the GaoFen-6 (GF-6) satellite utilizes eight bands, including four new bands.
Jie Han +5 more
doaj +1 more source
Cross-correlation redshift calibration without spectroscopic calibration samples in DES Science Verification Data [PDF]
12 pages, 5 figures. Submitted to MNRAS. Comments welcome!
Davis, C. +76 more
openaire +5 more sources
The relationship between two reflectances of different bands is often encountered in cross calibration and parameter retrievals from remotely-sensed data.
Munenori Miura +3 more
doaj +1 more source
Optical satellite sensor generally suffers from drifts and biases relative to their prelaunch calibration, caused by launch and the space environment.
Caixia Gao +10 more
doaj +1 more source
The sources of the highest energy cosmic-rays are still a mystery. One way to try to understand these sources is to measure the energies and composition of cosmic rays and build models that describe their energy spectrum. However, at the highest energies, energy scales between experiments are inconsistent.
Mulrey, Katharine +22 more
openaire +2 more sources
Radiometric Cross-calibration of KOMPSAT-3A with Landsat-8 [PDF]
In this study, Cross calibration was conducted at the Libya 4 PICS site on 2015 using Landsat-8 and KOMPSAT-3A. Ideally a cross calibration should be calculated for each individual scene pair because on any given date the TOA spectral profile is ...
D. Y. Shin +4 more
doaj +1 more source
Absolute Flux Calibration of the IRAC Instrument on the Spitzer Space Telescope using Hubble Space Telescope Flux Standards [PDF]
The absolute flux calibration of the James Webb Space Telescope will be based on a set of stars observed by the Hubble and Spitzer Space Telescopes. In order to cross-calibrate the two facilities, several A, G, and white dwarf (WD) stars are observed ...
A. Noriega-Crespo +52 more
core +2 more sources
INTEGRAL Cross-calibration Status
The status of the INTEGRAL cross-calibration is presented for a standard X-ray astronomy source, the Crab Nebula, as well as for some weaker sources. The relative flux normalization for the different INTEGRAL instruments is discussed together with spectral shape features.
Lubiński, P. +4 more
openaire +3 more sources

