Content Level: Amateur / Validation Level: 2 - STScI NAVO Directory Search Results

ID:: ivo://pds-ppi/cassini_rpws_electron_density/ppi/epn_core
Title:: Cassini RPWS Electron Densities from Upper Hybrid and Plasma Wave Frequencies
Short Name:: CO-RPWS-ELC-DEN
Date:: 16 Dec 2022 17:29:24
Publisher:: Planetary Data System
Description:: This collection provides electron number density values derived from features observed in plasma wave data obtained by the Cassini Radio and Plasma Wave Science (RPWS) instruments, along with observed or derived characteristic frequencies, and useful positional parameters for the spacecraft and related bodies. When present, frequency values of narrowband emissions at the upper hybrid resonance were digitized and combined with measured or model magnetic field to derive electron number density. At other times, features such as the upper cutoff in auroral hiss or electron plasma oscillations were used to determine the plasma frequency and electron density.

ID:: ivo://pds-ppi/cassini_mag_cal_shm_hkrate/ppi/epn_core
Title:: Cassini Scalar Helium MAG Calibrated Housekeeping ASCII Data Collection
Short Name:: CO-MAG-SHHKA
Date:: 01 Mar 2024 22:33:54
Publisher:: Planetary Data System
Description:: This collections contains Cassini scalar helium magnetometer (SHM) housekeeping ASCII data collected between 1999-08-18T02:56:40.391 and 2005-06-08T15:14:44.057.

ID:: ivo://pds-ppi/cassini_mag_cal_shm_hkrate_asc/ppi/epn_core
Title:: Cassini Scalar Helium MAG Calibrated Housekeeping Data Collection
Short Name:: CO-MAG-SHHK
Date:: 01 Mar 2024 22:33:40
Publisher:: Planetary Data System
Description:: This collection contains Cassini scalar helium (SHM) magnetometer housekeeping data collected between 1999-08-18 and 2005-06-08.

ID:: ivo://pds-ppi/cassini_mag_cal_shm_scirate_asc/ppi/epn_core
Title:: Cassini Scalar Helium MAG Calibrated Science ASCII Data Collection
Short Name:: CO-MAG-SHSA
Date:: 01 Mar 2024 22:27:57
Publisher:: Planetary Data System
Description:: This collection contains Cassini scalar helium magnetometer (SHM) science ASCII data collected between 1999-08-18 and 2005-10-11.

ID:: ivo://pds-ppi/cassini_mag_cal_shm_scirate/ppi/epn_core
Title:: Cassini Scalar Helium MAG Calibrated Science Data Collection
Short Name:: CO-MAG-SHS
Date:: 01 Mar 2024 22:26:13
Publisher:: Planetary Data System
Description:: This collection contains Cassini scalar helium magnetometer (SHM) science data collected between 1999-08-18 and 2005-10-11.

ID:: ivo://cxc.harvard.edu/registry
Title:: Chandra X-ray Center Publishing Registry
Short Name:: CXC-Reg
Date:: 02 Oct 2013
Publisher:: Chandra X-ray Observatory
Description:: This registry provides a simple interface for data providers who wish to register a handful of resources. It is compliant with VOResource v0.10

ID:: ivo://padc.obspm.planeto/planets/q/epn_core
Title:: Characteristics of Planets
Short Name:: Planets
Date:: 16 Jul 2024 13:55:03
Publisher:: Paris Astronomical Data Centre - LESIA
Description:: Main characteristics of Solar System planets. Data are included in the table, which includes non-standard EPN-TAP parameters. Data are retrieved from Archinal et al 2018 (IAU report 2015, 2018CeMDA.130...22A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods].

ID:: ivo://ov-gso/climso
Title:: CLIMSO coronagraphs at pic du midi de Bigorre
Short Name:: CLIMSO
Date:: 06 Sep 2024 07:01:26
Publisher:: OVGSO
Description:: Pic du Midi de Bigorre in the French Pyrenees is the place where coronagraphic images were first realized, by Bernard Lyot in the 1930s. Since then, the solar instruments at Pic du Midi regularly provide images of the solar disc, solar prominences and solar corona.

ID:: ivo://edu.gavo.org/hd/splat_redshift
Title:: Compute Redshifts of Quasars Using SPLAT-VO
Date:: 27 Dec 2024 08:31:06
Publisher:: The GAVO DC team
Description:: This tutorial uses SPLAT-VO to search the VO registry for spectra of galaxies and quasars. From the obtained spectra, the Hydrogen Lyman Alpha line will be used to compute redshift and velocity

ID:: ivo://edu.gavo.org/eurovo/aida_snconfirm
Title:: Confirmation of an apparent supernova
Date:: 27 Dec 2024 08:31:12
Publisher:: The GAVO DC team
Description:: Within this intermediate use case you learn about supernovae (see also the tutorial “Distance to the Crab Nebula“, ivo://edu.euro-vo.org/tutorials/08_m1_distance) and determine the celestial coordinates of a just discovered candidate supernova on an provided image without astrometric calibration. This use case provides a glimpse of an activity that is representative of the practical tasks that astronomers have to perform when they analyze data.

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