generated from ivoa-std/doc-template
-
Notifications
You must be signed in to change notification settings - Fork 4
Commit
This commit does not belong to any branch on this repository, and may belong to a fork outside of the repository.
- Loading branch information
Showing
1 changed file
with
68 additions
and
47 deletions.
There are no files selected for viewing
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
| Original file line number | Diff line number | Diff line change |
|---|---|---|
|
|
@@ -4,56 +4,77 @@ | |
| xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" | ||
| xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" | ||
| xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" | ||
| created="2020-03-10T16:30:00Z" | ||
| created="2020-10-28T15:11:00Z" | ||
| status="active" | ||
| updated="2020-03-10T16:30:00Z" | ||
| updated="2020-10-28T15:11:00Z" | ||
| xsi:type="vs:CatalogService"> | ||
| <title>Gamma-ray Coordinates Network</title> | ||
| <shortName>GCN</shortName> | ||
| <identifier>ivo://example.ignored/eventstream</identifier> | ||
| <curation> | ||
| <publisher>yes</publisher> | ||
| <creator> | ||
| <name>Scott Barthelmy</name> | ||
| </creator> | ||
| <date role="updated">2020-03-31T15:38:21Z</date> | ||
| <contact> | ||
| <name>Scott Barthelmy</name> | ||
| <address>8800 Greenbelt Rd</address> | ||
| <email>[email protected]</email> | ||
| <telephone>301-286-3106</telephone> | ||
| </contact> | ||
| </curation> | ||
| <content> | ||
| <subject>gamma-ray-bursts</subject> | ||
| <subject>time-domain-astronomy</subject> | ||
| <description> | ||
| The GCN system distributes Locations of GRBs and other transients | ||
| detected by spacecraft, mostly in real time, as well as reports | ||
| of follow-up observations made by ground-based and space-based | ||
| instruments across the electromagnetic spectrum. | ||
| </description> | ||
| <source format="bibcode">TODO</source> | ||
| <referenceURL>https://gcn.gsfc.nasa.gov/</referenceURL> | ||
| <type>Other</type> | ||
| <contentLevel>Research</contentLevel> | ||
| </content> | ||
| <capability standardID="ivo://ivoa.net/std/VOEvent"> | ||
| <interface role="std" standardID="ivo://ivoa.net/std/VOEvent#acc-vtp" | ||
| xsi:type="voe:StreamEndpoint"> | ||
| <accessURL>TODO</accessURL> | ||
| </interface> | ||
| </capability> | ||
| <facility>Goddard Space Flight Center</facility> | ||
| <coverage> | ||
| <spatial>0/0-11</spatial> | ||
| <waveband>Radio</waveband> | ||
| <waveband>Optical</waveband> | ||
| <waveband>X-ray</waveband> | ||
| <waveband>Gamma-ray</waveband> | ||
| </coverage> | ||
| <title>Meteor Shower prediction</title> | ||
| <shortName>meteor_showers</shortName> | ||
| <identifier>ivo://vopdc.obspm/imcce/meteorshower/event</identifier> | ||
| <curation> | ||
| <publisher ivo-id="ivo://vopdc.obspm/imcce" | ||
| >Paris Astronomical Data Centre - IMCCE</publisher> | ||
| <creator> | ||
| <name>Jeremy Vaubaillon</name> | ||
| </creator> | ||
| <date role="updated">2019-03-22T15:50:42</date> | ||
| <contact> | ||
| <name>PADC support team</name> | ||
| <address>77 av. Denfert Rochereau, 75014 Paris, FRANCE</address> | ||
| <email>[email protected]</email> | ||
| <telephone>0033140512082</telephone> | ||
| </contact> | ||
| </curation> | ||
| <content> | ||
| <subject>Comet</subject> | ||
| <subject>Simulation</subject> | ||
| <description> | ||
| This is an ephemeris of meteor showers occurring on solar | ||
| system planets, produced by simulating the ejection of | ||
| meteoroids from the sunlit hemisphere of cometary nuclei, typically | ||
| from 0 to 3 au, followed by the propagation of orbits of meteoroids | ||
| in the Solar System, taking into account the gravitation of the | ||
| Sun, the 8 planets, Pluto, and the Moon, as well as the radiation | ||
| pressure and the Poynting-Robertson drag. Note that asteroid parent | ||
| bodies were considered as active (i.e. comet-like bodies) even if | ||
| they are not active today. The showers are predicted when a planet | ||
| enters a large enough set of meteoroids, at a distance less than | ||
| typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new | ||
| method to predict meteor showers. I. Description of the model, | ||
| Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: | ||
| Vaubaillon J. 2017 A confidence index for forecasting of meteor | ||
| showers, Planetary and Space Science, Volume 143 p.78-82 | ||
| </description> | ||
| <source format="bibcode">2017P%26SS..143...78V</source> | ||
| <referenceURL> | ||
| http://voparis-tap-voevent.obspm.fr/tableinfo/meteor_showers.epn_core | ||
| </referenceURL> | ||
| <type>Other</type> | ||
| <contentLevel>Research</contentLevel> | ||
| <relationship> | ||
| <!-- TAP service containing/archiving all previous | ||
| events produced by this stream --> | ||
| <relationshipType>IsSourceOf</relationshipType> | ||
| <relatedResource ivo-id="ivo://vopdc.obspm/imcce/meteorshower/epn" | ||
| >Meteor Shower prediction EPN-TAP service</relatedResource> | ||
| </relationship> | ||
| </content> | ||
| <capability standardID="ivo://ivoa.net/std/VOEvent"> | ||
| <!-- TODO: figure out if this needs a declaration like | ||
| "This is VOEvent 2 in XML serialisation" – or if that's | ||
| implied in something else we're saying here --> | ||
| <interface role="std" xsi:type="voe:StreamEndpoint" | ||
| standardID="ivo://ivoa.net/std/VOEvent#acc-vtp"> | ||
| <accessURL>x-vtp://voparis-voevent-psws.obspm.fr:8099</accessURL> | ||
| </interface> | ||
| </capability> | ||
| <facility>IMCCE</facility> | ||
| <coverage> | ||
| <waveband>Radio</waveband> | ||
| <waveband>Optical</waveband> | ||
| <waveband>Infrared</waveband> | ||
| </coverage> | ||
| </ri:Resource> | ||
|
|
||
|
|
||
| <!-- vim:et:sw=2 | ||
| --> | ||