The Cornell Digital HI Archive is a homogeneous compilation of HI spectral parameters extracted from global 21 cm line spectra for some 9000 galaxies in the local universe (heliocentric velocity -200 < V > 28,000 km/s) obtained with a variety of large single dish radio telescopes but reanalyzed using a single set of parameter extraction algorithms. The database contains a catalog of HI parameters (systemic velocities, integrated HI line fluxes and full widths), plots of the HI spectra, and the digital spectra themselves. The Cornell Digital HI Archive data is currently served by NED.
This catalog includes CoRoT targets from the exoplanet channel which were identified as possible red giants and actually presents acoustic oscillations of solar-like type, as published by Hekker et al. (A&A, 2009, vol. 506, p. 465).
Data for numerical modeling of planetary atmospheres
Date:
12 Jun 2017 10:19:38
Publisher:
Instituto de Astrofisica de Andalucia-CSIC; INTA-CAB
Description:
Numerical modeling of composition and thermal balance of planetary
atmospheres requires a considerable amount of laboratory data. Among
them, the absorption cross sections in the UV range are needed both
for computing the heating in the atmosphere and the photodissociation
coefficients to initiate a rich disequilibrium chemistry. Prompted by
these needs in the community and by the sparse collection of data in
several other web pages (http://www.science-softcon.de/ or
http://satellite.mpic.de/spectral_atlas/index.html whose data depend
on some pre-processing before being ingested in these models), this
web page aims at providing the community with absorption cross
sections in the range 20 nm to 400 nm equally spaced every 0.2, 0.5
and 1.0 nm. Also, original data as appearing in the refereed journal
and the reference itself are downloadable.
The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.
VO-compliant publication of Schmidt survey ESO-R of the southern sky digitized with the MAMA microdensitometer at the Observatoire de Paris Image Analysis Centre (CAI).
*** EUV-SYN *** Synchronous synoptic maps of the corona in the
extreme-UV (EUV), built from series of SoHO/EIT observations, in each
of the 4 wavelength bands of the instrument.
Synchronous synoptic maps are maps of the EUV radiance in different
wavelength bands on the full solar sphere, in heliographic
(Carrington) longitude and latitude, where data are taken as close as
possible to a reference time. They capture the state of the corona at
any given reference time by including data taken as close as possible
to this time.
EUV-SYN is available as part of the generic MEDOC interface which is
currently located at https://idoc-medoc.ias.u-psud.fr/. These
interfaces are based on the CNES SiTools2 framework. EUV-SYN is also
available from IDL and Python scripts, using a specialization of the
generic SiTools2 IDL and Python clients developed by MEDOC.
"The data consists in topographic maps of synthetic 3D bodies
generated by a 3 parameters statistical model : the fractionally
integrated flux (FiF) (Lavallee, D., Lovejoy, S., Schertzer, D.,
Ladoy, P. (1993). Nonlinear variability and landscape topography:
analysis and simulation) adapted for spherical coordinates and
topography (Landais, F., Schmidt, F., and Lovejoy, S, (2018)
Topography of exoplanets, MNRAS). The 3 parameters are the following :
H: degree of smoothness; C1: degree of intermittency; alpha: degree of
multifractality; The service contains topographic maps (in Fits
format) and texture maps (in png format)."
VO-compliant publication of the properties of the 3838 galaxies that were monitored for SNe events, including newly determined morphologies and their DENIS and POSS-II/UKST I, 2MASS and DENIS J and Ks and 2MASS H magnitudes.
The principal research topics of the GEPI (Galaxy - Star - Physics - Instrumentation) Laboratory are the formation and evolution of stars in our Galaxy as well as in numerous other galaxies, which constitute the luminous matter (baryonic matter) component of the Universe. This research calls upon many disciplines, from chemistry to physics, from instrumentation to data-processing engineering, and from project management to financial management within an international framework.
Galileo EPD Calibrated Corrected Delta Event Data Collection
Short Name:
EPD-DELTA-EVE
Date:
15 Dec 2022 19:26:15
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle
Detector (EPD) instrument onboard the Galileo spacecraft that orbited
Jupiter and measured intensities of ion and electron radiation in the
keV and MeV energy range. This set is version 31 of reprocessing and
version 1.0 of PDS delivery. The TOFxE and DeltaExE files include
event data of ion measurements. Event data are different than the
channelized data in the high, medium, and low resolution files. Event
data record the full information of a measured particle. Every "event"
is the measurement of a time of flight (TOF) within the instrument and
energy deposited within a detector (TOFxE file), or two energy values
deposited within the two detector layers (DeltaExE file). The
deposited energy values are generally different from the energy the
particle has in the ambient space. Event data provides measured values
in the native resolution of the instrument. Because such high
resolution increases data volume, event data cannot be taken
continuously and downlinked all the time. Only the provided subset of
this data was kept. The files are comma separated. Invalid entries
will have values of -1.000000E+38. Times are provided in the format
Year.DOYHHMMSSM (first column) and fractional year (second column)
More information can be found in the User Guide. This file includes
measurements by the EPD/CMS/DeltaExE instrument. For each counted
event, the energy deposited in the two solid state detector layers
(Ej_keV and Ek_keV columns) of the instrument are recorded.
Galileo EPD Calibrated Corrected High Res Data Collection
Short Name:
EPD-HIGH-RES
Date:
15 Dec 2022 19:27:32
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle
Detector (EPD) instrument onboard the Galileo spacecraft that orbited
Jupiter and measured intensities of ion and electron radiation in the
keV and MeV energy range. This set is version 31 of reprocessing and
version 1.0 of PDS delivery. Data in the high resolution files include
measurements that are binned into channels responding to certain
energy and species ranges. The files are comma separated. Invalid
entries will have -1.000000E+38 as an entry. The first 4 lines of each
data text file provide information on the channels included here: The
first line of each file lists the names of the channels included. The
second line lists the center energies of these channels in keV. The
third line lists the channels again. The forth line lists the mass of
the measured particle in AMU. Zero mass refers to electrons. The forth
line in the data text file labels the columns that follow in the file.
The columns include times, radiation measurements, spacecraft
location, instrument look direction, and some supplementary
information. Radiation measurements are provided both as best
calibrated and cleaned intensities as well as raw, uncorrected count
rates. Columns with channel names followed by a "j" include calibrated
differential intensities of the given channel. If the value is
negative, it should be ignored and particularly not included in
averages. For the difference between -1.000000E+38 and all other
negative values, see the User Guide. Columns ending with "f" provide
differential intensities based on a combination of various channels.
Columns ending with "i" include calibrated integral intensities.
Columns with plain channel names describe the raw uncorrected count
rate. Columns ending with "bg" are raw count rates measured behind the
calibration shield. Each following line will provide the same data but
for different times. More information can be found in the User Guide.
This file provides data with the highest available time and pitch
angle resolution. Only a small set of channels is provided, limiting
the energy resolution and coverage. If columns with plain channel
names have -1.000000E+38 values, you might find valid values in the
lower resolution files.
Galileo EPD Calibrated Corrected Low Res Data Collection
Short Name:
EPD-LOW-RES
Date:
15 Dec 2022 19:28:50
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle
Detector (EPD) instrument onboard the Galileo spacecraft that orbited
Jupiter and measured intensities of ion and electron radiation in the
keV and MeV energy range. This set is version 31 of reprocessing and
version 1.0 of PDS delivery. Data in the low resolution files include
measurements that are binned into channels responding to certain
energy and species ranges. The files are comma separated. Invalid
entries will have -1.000000E+38 as an entry. The first 4 lines of each
data text file provide information on the channels included here: The
first line of each file lists the names of the channels included. The
second line lists the center energies of these channels in keV. The
third line lists the channels again. The forth line lists the mass of
the measured particle in AMU. Zero mass refers to electrons. The forth
line in the data text file labels the columns that follow in the file.
The columns include times, radiation measurements, spacecraft
location, instrument look direction, and some supplementary
information. Radiation measurements are provided both as best
calibrated and cleaned intensities as well as raw, uncorrected count
rates. Columns with channel names followed by a "j" include calibrated
differential intensities of the given channel. If the value is
negative, it should be ignored and particularly not included in
averages. For the difference between -1.000000E+38 and all other
negative values, see the User Guide. Columns ending with "f" provide
differential intensities based on a combination of various channels.
Columns ending with "i" include calibrated integral intensities.
Columns with plain channel names describe the raw uncorrected count
rate. Columns ending with "bg" are raw count rates measured behind the
calibration shield. Each following line will provide the same data but
for different times. More information can be found in the User Guide.
This includes the full set of channels covering the full energy and
species range of EPD. The time and pitch angle resolution is low.
Higher resolution is available for some channels that can be found in
the medium and high resolution files.the energy deposited in the one
solid state detector (Energy_keV column) and the time of flight
(TOF_ns) within the instrument are recorded.
Galileo EPD Calibrated Corrected Medium Res Data Collection
Short Name:
EPD-MED-RES
Date:
15 Dec 2022 19:27:13
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle
Detector (EPD) instrument onboard the Galileo spacecraft that orbited
Jupiter and measured intensities of ion and electron radiation in the
keV and MeV energy range. This set is version 31 of reprocessing and
version 1.0 of PDS delivery. Data in the medium resolution files
include measurements that are binned into channels responding to
certain energy and species ranges. The files are comma separated.
Invalid entries will have -1.000000E+38 as an entry. The first 4 lines
of each data text file provide information on the channels included
here: The first line of each file lists the names of the channels
included. The second line lists the center energies of these channels
in keV. The third line lists the channels again. The forth line lists
the mass of the measured particle in AMU. Zero mass refers to
electrons. The forth line in the data text file labels the columns
that follow in the file. The columns include times, radiation
measurements, spacecraft location, instrument look direction, and some
supplementary information. Radiation measurements are provided both as
best calibrated and cleaned intensities as well as raw, uncorrected
count rates. Columns with channel names followed by a "j" include
calibrated differential intensities of the given channel. If the value
is negative, it should be ignored and particularly not included in
averages. For the difference between -1.000000E+38 and all other
negative values, see the User Guide. Columns ending with "f" provide
differential intensities based on a combination of various channels.
Columns ending with "i" include calibrated integral intensities.
Columns with plain channel names describe the raw uncorrected count
rate. Columns ending with "bg" are raw count rates measured behind the
calibration shield. Each following line will provide the same data but
for different times. More information can be found in the User Guide.
This includes a limited set of channels with intermediate time and
pitch angle resolution. If columns with plain channel names have
-1.000000E+38 values, you might find valid values in the lower
resolution files.
Galileo EPD Calibrated Corrected Time-of-Flight Event Data Collection
Short Name:
EPD-TOF-EVE
Date:
15 Dec 2022 19:26:10
Publisher:
Planetary Data System
Description:
These are reprocessed measurements by the Engergetic Particle
Detector (EPD) instrument onboard the Galileo spacecraft that orbited
Jupiter and measured intensities of ion and electron radiation in the
keV and MeV energy range. This set is version 31 of reprocessing and
version 1.0 of PDS delivery. The TOFxE and DeltaExE files include
event data of ion measurements. Event data are different than the
channelized data in the high, medium, and low resolution files. Event
data record the full information of a measured particle. Every "event"
is the measurement of a time of flight (TOF) within the instrument and
energy deposited within a detector (TOFxE file), or two energy values
deposited within the two detector layers (DeltaExE file). The
deposited energy values are generally different from the energy the
particle has in the ambient space. Event data provides measured values
in the native resolution of the instrument. Because such high
resolution increases data volume, event data cannot be taken
continuously and downlinked all the time. Only the provided subset of
this data was kept. The files are comma separated. Invalid entries
will have values of -1.000000E+38. Times are provided in the format
Year.DOYHHMMSSM (first column) and fractional year (second column)
More information can be found in the User Guide. This file includes
measurements by the EPD/CMS/TOFxE instrument. For each counted event,
the energy deposited in the one solid state detector (Energy_keV
column) and the time of flight (TOF_ns) within the instrument are
recorded.
Galileo HIC Derived Ion Fluxes October 89 Solar Event Data Collection
Short Name:
GO-HIC-PJ-DER
Date:
15 Dec 2022 19:30:31
Publisher:
Planetary Data System
Description:
This collection contains values for the fluxes of heavy ions
associated with an energetic particle event of solar origin. The
values are derived from HIC data taken during the Interplanetary
Cruise to Jupiter.
Galileo Jupiter HIC Derived Energetic Ion Competition Data Collection
Short Name:
GO-HIC-J-DER
Date:
15 Dec 2022 19:25:36
Publisher:
Planetary Data System
Description:
This collection contains energetic (MeV) ion fluxes for a variety of
different Z values (carbon, oxygen, sulfur) derived from the Heavy Ion
Counter (HIC) instrument on the Galileo spacecraft. The data set
includes all recorded intervals at Jupiter.
Galileo Jupiter HIC High Resolution Raw Data Collection
Short Name:
GO-HIC-J-RAW
Date:
15 Dec 2022 19:24:14
Publisher:
Planetary Data System
Description:
This collection contains raw energetic (MeV) particle data measured
by the Heavy Ion Counter (HIC) instrument on the Galileo spacecraft.
This data set contains both real-time and recorded data for all
Jupiter orbits.
Galileo Jupiter HIC Survey Energetic Ion Count Rate Calibrated
Collection Data Collection
Short Name:
HIG-J-SRVY-CNT
Date:
15 Dec 2022 19:30:33
Publisher:
Planetary Data System
Description:
This collection contains energetic (MeV) ion count rates and events
measured by the Heavy Ion Counter (HIC) instrument on the Galileo
spacecraft. The data are derived from the raw real-time science (RTS)
data. There are two basic types of data files associated with the
full-rate reduced data: Detector Count Rates and Events (Pulse
Heights).
Galileo Jupiter Magnetometer Highres Callisto Data Collection
Short Name:
GO-MAG-JUP-CAL
Date:
15 Dec 2022 19:29:16
Publisher:
Planetary Data System
Description:
This data collection contains high time resolution magnetic field
vectors acquired by the Galileo magnetometer (MAG). It includes
satellite flyby Callisto data. These data were acquired in order to
characterize various portions of the Jovian magnetosphere at high time
resolution.
Galileo Jupiter Magnetometer Highres Europa Data Collection
Short Name:
GO-MAG-JUP-EUR
Date:
15 Dec 2022 19:29:32
Publisher:
Planetary Data System
Description:
This data collection contains high time resolution magnetic field
vectors acquired by the Galileo magnetometer (MAG). It includes
satellite flyby Europa data. These data were acquired in order to
characterize various portions of the Jovian magnetosphere at high time
resolution.
Galileo Jupiter Magnetometer Highres Ganymede Data Collection
Short Name:
GO-MAG-JUP-GAN
Date:
15 Dec 2022 19:25:05
Publisher:
Planetary Data System
Description:
This data collection contains high time resolution magnetic field
vectors acquired by the Galileo magnetometer (MAG). It includes
satellite flyby Ganymede data. These data were acquired in order to
characterize various portions of the Jovian magnetosphere at high time
resolution.
Galileo Jupiter Magnetometer Highres Io Data Collection
Short Name:
GO-MAG-JUP-IO
Date:
15 Dec 2022 19:28:54
Publisher:
Planetary Data System
Description:
This data collection contains high time resolution magnetic field
vectors acquired by the Galileo magnetometer (MAG). It includes
satellite flyby Io data. These data were acquired in order to
characterize various portions of the Jovian magnetosphere at high time
resolution.
Galileo Jupiter Magnetometer Highres Magnetosphere Data Collection
Short Name:
GO-MAG-JUP-MAGN
Date:
15 Dec 2022 19:24:33
Publisher:
Planetary Data System
Description:
TThis data collection contains high time resolution magnetic field
vectors acquired by the Galileo magnetometer (MAG). It includes
satellite flyby data. These data were acquired in order to
characterize various portions of the Jovian magnetosphere at high time
resolution.
Galileo Jupiter Magnetometer Magnetospheric Survey Data Collection
Short Name:
GO-MAG-JUP-MS
Date:
15 Dec 2022 19:28:55
Publisher:
Planetary Data System
Description:
Galileo MAG calibrated optimal averager magnetic field data near
Jupiter, and in the solar wind from the Jupiter Approach phase in
Despun Spacecraft (IRC) coordinates. The data cover 1995-11-01T00:06
to 1995-12-06T02:09 to 1995-12-06T02:09.
Galilieo Jupiter HIC Highres Energetic Ion Count Rate Data Collection
Short Name:
HIG-J-HI-AMA
Date:
15 Dec 2022 19:30:11
Publisher:
Planetary Data System
Description:
This collection contains Galileo HIC high resolution (LPW) pulse
height data acquired at Jupiter and Amalthea between 2002-11-05T02:45
and 2002-11-05T06:35.
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.
All data for the Herschel SPIRE and PACS guaranted time program on Interstellar Medium (SAG-4) and other public data processed at IDOC. All data have been reprocessed at IDOC using advanded reprocessing pipeline.
All data for the Herschel SPIRE and PACS guaranted time program on Interstellar Medium (SAG-4) and other public data processed at IDOC. All data have been reprocessed at IDOC using advanded reprocessing pipeline.
H.E.S.S. is a system of Imaging Atmospheric Cherenkov Telescopes that investigates cosmic gamma rays in the 100 GeV to 100 TeV energy range. The name H.E.S.S. stands for High Energy Stereoscopic System.
HST observations of planets, dwarf planets, and satellites, extracted
from the CADC database catalogue (with daily updates). Data are linked
to the CADC repository, with file names common to all HST archives.
Both calibrated and derived products are included. The main target is
identified. Physical ephemeris and thumbnails are provided when
available. Files and previews are not accessible during the
proprietary period.
This database provides access to IDOC catalogues and complementary information on clusters of galaxies observed through the Sunyaev-Zeldovich (SZ) effect.