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Standard photometric systems
▪ Abstract Standard star photometry dominated the latter half of the twentieth century
reaching its zenith in the 1980s. It was introduced to take advantage of the high sensitivity …
reaching its zenith in the 1980s. It was introduced to take advantage of the high sensitivity …
Evolution of asymptotic giant branch stars-II. Optical to far-infrared isochrones with improved tp-agb models
We present a large set of theoretical isochrones, whose distinctive features mostly reside on
the greatly-improved treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) …
the greatly-improved treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) …
Spectral Irradiance Calibration in the Infrared. XIV. The AbsoluteCalibration of 2MASS
Element by element, we have combined the optical components in the three cameras of the
Two Micron All Sky Survey (2MASS), and incorporated detector quantum efficiency curves …
Two Micron All Sky Survey (2MASS), and incorporated detector quantum efficiency curves …
The angular sizes of dwarf stars and subgiants-Surface brightness relations calibrated by interferometry
The availability of a number of new interferometric measurements of Main Sequence and
subgiant stars makes it possible to calibrate the surface brightness relations of these stars …
subgiant stars makes it possible to calibrate the surface brightness relations of these stars …
An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars
JT Van Loon, MRL Cioni, AA Zijlstra, C Loup - Astronomy & Astrophysics, 2005 - aanda.org
We present an empirical determination of the mass-loss rate as a function of stellar
luminosity and effective temperature, for oxygen-rich dust-enshrouded Asymptotic Giant …
luminosity and effective temperature, for oxygen-rich dust-enshrouded Asymptotic Giant …
First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001-Implications for the r-process site (s) and radioactive cosmochronology
We present a high-resolution (75 000, S/N) spectroscopic analysis of the bright (11.7),
extreme halo giant CS 31082-001 ([Fe/H]=-2.9), obtained in an ESO-VLT Large Programme …
extreme halo giant CS 31082-001 ([Fe/H]=-2.9), obtained in an ESO-VLT Large Programme …
Magellanic Cloud structure from near-infrared surveys. I. The viewing angles of the Large Magellanic Cloud
RP van der Marel, MRL Cioni - The Astronomical Journal, 2001 - iopscience.iop.org
We present a detailed study of the viewing angles of the LMC disk plane. We find that our
viewing direction differs considerably from the commonly accepted values, which has …
viewing direction differs considerably from the commonly accepted values, which has …
Measurement of stellar age from uranium decay
The ages of the oldest stars in the Galaxy indicate when star formation began, and provide a
minimum age for the Universe. Radioactive dating of meteoritic material and stars relies on …
minimum age for the Universe. Radioactive dating of meteoritic material and stars relies on …
The tip of the red giant branch and distance of the Magellanic Clouds: results from the DENIS survey
MRL Cioni, RP van der Marel, C Loup… - arxiv preprint astro-ph …, 2000 - arxiv.org
We present a precise determination of the apparent magnitude of the tip of the red giant
branch (TRGB) in the I (0.8 micron), J (1.25 micron), and K_S (2.15 micron) bands from the …
branch (TRGB) in the I (0.8 micron), J (1.25 micron), and K_S (2.15 micron) bands from the …
JHK observations of faint standard stars in the Mauna Kea Observatories near-infrared photometric system
SK Leggett, MJ Currie, WP Varricatt… - Monthly Notices of …, 2006 - academic.oup.com
JHK photometry in the Mauna Kea Observatories (MKO) near-infrared system is presented
for 115 stars. Of these stars, 79 are United Kingdom Infrared Telescope (UKIRT) standards …
for 115 stars. Of these stars, 79 are United Kingdom Infrared Telescope (UKIRT) standards …