... A second advantage is that Cepheid light curves in the infrared have smaller amplitudes and are much more symmetrical than their opticalcounterparts, making it possible to measure a Cepheid's mean K-band brightness just from a very few, and in principle ...
... A second advantage is that Cepheid light curves in the infrared have smaller amplitudes and are much more symmetrical than their opticalcounterparts, making it possible to measure a Cepheid's mean K-band brightness just from a very few, and in principle ...
... A second advantage is that Cepheid light curves in the infrared have smaller amplitudes and are much more symmetrical than their opticalcounterparts, making it possible to measure a Cepheid's mean K-band brightness just from a very few, and in principle ...
... Looking for opticalcounterparts of X-ray sources * fire up the AVO prototype portal as described on the installation page * click on Load, enter target CDFS and radius = 30 arcmin, press Submit * click on Data Tree * load V-band WFI preview image of ...
... A second advantage is that Cepheid light curves in the infrared have smaller amplitudes and are much more symmetrical than their opticalcounterparts, making it possible to measure a Cepheid's mean K-band brightness just from a very few, and in principle ...
... and hence, oldest stars, accurate cosmochronological dating by means of Uranium and Thorium spectral lines, high-redshift galaxy rotation curves, micro-quasars, properties of the opticalcounterparts of gamma-ray bursts, high-redshift supernovae, etc ...