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GRAMS carbon-star model grid
Synthetic spectra and photometry for the GRAMS carbon-star set of radiative transfer models is provided in FITS form. Also included are various stellar and dust shell parameters... -
Mock spectro-photometric catalog of galaxies
Future dark energy space missions such as JDEM and EUCLID are being designed to survey the galaxy population to trace the geometry of the universe and the growth of structure,... -
Synthetic spectrophotometry for C-rich giants
Carbon rich objects represent an important phase during the late stages of evolution of low and intermediate mass stars. They contribute significantly to the chemical enrichment... -
SSP models for star clusters in tidal fields
Evolutionary synthesis models are the primary means of constructing spectrophotometric models of stellar populations, and deriving physical parameters from observations compared... -
Transiting planet OGLE-TR-132b
OGLE-TR-132b transits a very metal-rich F dwarf about 2000 pc from the Sun, in the Galactic disc towards Carina. It orbits very close to its host star (a=0.03AU) and has an... -
XMM-Newton survey in the Marano Field. I.
We report on a medium deep XMM-Newton survey of the Marano Field and optical follow-up observations. The mosaicked XMM-Newton pointings in this optical quasar survey field cover... -
L- & M-band imaging of the Galactic Center
Photometric data of the sources detected in NAOS/CONICA H- and K-band (1.6 and 2.1{mu}m) and ISAAC L- and M-band (3.8 and 4.7{mu}m) images of the Galactic Center, obtained in... -
Extremely Red Objects XMM-Newton observations
We present the results of a deep (about 80ks) XMM-Newton survey of the largest sample of near-infrared selected Extremely Red Objects (R-K>5) available to date to... -
15-color BATC photometry of Landolt SA95 field
In this paper, we present a set of photometric observations in 15 colors of stars in the Landolt SA95 field with the BATC (Beijing-Arizona-Taipei-Connecticut) system. The... -
H{alpha} surface photometry in Virgo
H{alpha}+[NII] imaging observations of 369 late-type (spiral) galaxies in the Virgo cluster and in the Coma/A1367 supercluster are analyzed, covering 3 rich nearby clusters... -
Spectral analysis of Lockman Hole
We present the results of the X-ray spectral analysis of the first deep X-ray survey with the XMM-Newton observatory during Performance Verification. The X-ray data of the... -
NTT SUSI Deep Field
This catalog contains BVrI photometry of galaxies in a 5.62arcmin^2^ field 80arcsec south of the high redshift (z=4.7) quasar BR 1202-0725, derived from observations with the... -
Low-mass stars evolutionary models
Physical properties and absolute magnitudes of low-mass stars for different initial metallicity [M/H], helium mass fraction Y and mixing length parameter Lmix: mass (in solar... -
Brightest Cluster Galaxies from CFH TLS
Brightest cluster galaxies (BCGs) are very massive elliptical galaxies found at the centres of clusters. Their study gives clues to the formation and evolution of the clusters... -
MASCARA-4 b light and RV curves
Ultra-hot Jupiters (UHJs), rendering the hottest planetary atmospheres, offer great opportunities of detailed characterisation with high-resolution spectroscopy. The extremely... -
Two long-period transiting exoplanets
Long-period transiting planets provide the opportunity to better understand the formation and evolution of planetary systems. Their atmospheric properties remain largely... -
Gl514 RVs and activity diagnostics
Statistical analyses based on Kepler data show that most of the early-type M dwarfs host multi-planet systems consisting of Earth to sub-Neptune sized planets with orbital... -
TOI-1468 photometry and radial velocities
We report the discovery and characterization of two small transiting planets orbiting the bright M3.0 V star TOI-1468 (LSPM J0106+1913), whose transit signals were detected in... -
Galaxy subtypes in the VIPERS survey
This study aims to explore the relation between the physical properties of different galaxy subclasses, from red passive to blue star-forming, and their environment. Our work is... -
The Scrolling Infinite Lightcurve
A web-based GUI to the infinite microlensing lightcurve.