This catalogue is a simulation of the Gaia DR2 stellar content using
Galaxia (a tool to sample stars from a Besancon-like Milky Way model),
3d dust extinction maps and the latest PARSEC Isochrones. It is
mimicking the Gaia DR2 data model and an apparent magnitude limit of
g=20,7. Extinctions and photometry in different bands have also been
included in a supplementary table as well as uncertainty estimates
using a scaled nominal error model.
This catalogue is a simulation of the Gaia EDR3 stellar content using
Galaxia (a tool to sample stars from a Besancon-like Milky Way model),
3d dust extinction maps and the latest PARSEC Isochrones. It is
mimicking the Gaia DR2 data model and an apparent magnitude limit of
G=20,7. Extinctions and photometry in different bands have also been
included in a supplementary table as well as uncertainty estimates
using scaled GDR2 errors. Additional magnitude limit per HEALpix maps
are provided, based on the mode in the magnitude distribution of Gaia
DR2 data.
Planetary Atmospheres Research Unit - Royal Belgian Institute for
Space Aeronomy
Description:
Profiles of pressure, temperature and species of the Martian
atmosphere simulated with the GEM-Mars general circulation model. See
for the main model descritpion Neary, L., et al. 2018. The GEM-Mars
general circulation model for Mars: Description and evaluation. Icarus
300, 458-476. https://doi.org/10.1016/j.icarus.2017.09.028. See for
the chemistry description Dearden, F. et al., 2019, Mars atmospheric
chemistry simulations with the GEM-Mars general circulation model,
Icarus, 326, 197-224, https://doi.org/10.1016/j.icarus.2019.02.030.
Simulated non-Gaussian temperature and polarization CMB maps. The
non-Gaussian simulations have been generated using the algorithm described in
:bibcode:`2009ApJS..184..264E` up to a multipole moment of l_max = 1024. The
transfer functions were computed with CAMB version February 2009 and RECFAST
1.5.
TheoSSA provides spectral energy distributions based on model
atmosphere calculations. Currently, we serve results obtained using
the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact
stars.
TheoSSA provides spectral energy distributions based on model
atmosphere calculations. Currently, we serve results obtained using
the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact
stars.
TMAW -- Tübingen Model Atmosphere Package WWW Interface
Short Name:
TMAW
Date:
23 Mar 2022 13:13:07
Publisher:
The GAVO DC team
Description:
The Tübingen NLTE Model-Atmosphere Package (`TMAP
<http://astro.uni-tuebingen.de/%7ETMAP/TMAP.html>`_) is a tool to calculate
stellar atmospheres in spherical or plane-parallel geometry in hydrostatic
and radiative equilibrium allowing departures from local thermodynamic
equilibrium (LTE) for the population of atomic levels./TMAP/ is based on
the so-called Accelerated Lambda Iteration (ALI) method and is able to
account for line blanketing by metals. All elements from hydrogen to nickel
may be included in the calculation with model atoms which are tailored for
the aims of the user.
