[vsnet-grb 308529] New GCN Notice type: Actual pointing direction of Swift
Bacodine
vxw at capella2.gsfc.nasa.gov
Thu Nov 17 08:28:46 JST 2016
TO: All GCN Sites
RE: Swift_Actual_PointDir Notices Added
DT: 16 Nov 16
SWIFT_ACTUAL_POINTDIR NOTICE TYPE ADDED:
Swift has long had the SWIFT_POINTDIR notice type which contains
the pre-planned pointings for the Swift mission, and they are distributed
~30 sec before the beginning of the slew to that location. But because
of on-board triggers and uploaded ToO's, the fraction of time
that Swift is not looking at the pre-planned location is ~9%.
Now the SWIFT_ACTUAL_POINTDIR notice type has been added. It contains
the actual pointing direction of the Swift spacecraft, and is distributed
~30 sec after the end of each slew to the new location. This information
is derived from monitoring the real-time housekeeping information
coming down the TDRSS DAS link (24/7).
UTILITY OF THIS NOTICE TYPE:
This notice will: (a) allow automated instruments to "follow" the Swift
observation direction. These instruments can then have a shorter
slew time themselves should there be a Swift-BAT burst detection, and
(b) allow people to monitor if/when their TOO request is being executed
or if their pre-planned observation was interrupted by an AT or TOO.
(This notice is blocked to public sites when Swift is observing LVC targets.)
OCCURRENCE RATE:
Since observations can be as short as ~90 sec (ie during special tiling operations)
to as long as ~45 minutes, there will be ~70-100 of these notices per day.
RELIABILITY:
Because this notice type is derived from the real-time TDRSS DAS link,
there will be holes in the sequence due to (a) gaps in this housekeeping
stream when a regular data downlink session is happening (ie 7-13 times per day
for 8-12 minutes each, ie 5-12%)), and (b) other gaps/outages in TDRSS (<1%).
A slew during a TDRSS gap is not lost (unless the observation is shorter
than the TDRS gap); rather, the new pointing direction is just reported late.
DISTRIBUTION METHODS:
This notice type (ike all the other types in GCN) is available by all the
socket-based (binary and voevent) and email-based.
CONTENTS and FORMATS:
A detailed description of this new notice type (and all the Swift Notices)
is found at: http://gcn.gsfc.nasa.gov/gcn/swift.html
and for the socket sites, the packets are defined in:
http://gcn.gsfc.nasa.gov/gcn/sock_pkt_def_doc.html
ACTION ITEM:
If you want to receive these SWIFT_ACTUAL_POINTDIR notices,
please send me a request to have them enabled. You can do this
by forwarding this email (which has your sitename identifier & current configuration)
to sbarthel at milkyway.gsfc.nasa.gov .
OR
You can go to http://gcn.gsfc.nasa.gov/gcn/config_builder.html
and select "#2 Modify an existing config" (and type in your sitename).
You can also take this opportunity to make other changes to your configuration.
REMINDER OF RECENT ADDITIONS TO GCN:
In case you have missed them, here is a brief list of the most recent additions
to the GCN system. You might consider signing up for these Notice types as well.
The full announcements/descriptions for each of these can be found at:
http://gcn.gsfc.nasa.gov/gcn/whats_new.html
AMON_ICECUBE_EHE (July 2016) // ICECUBE Extreme High Energy events
AMON_ICECUBE_HESE (Apr 2016) // ICECUBE High Energy Starting Events
CALET_LC (Mar 2016) // The Flight- & Ground-produced CALET-GBM lightcurves
SNEWS (Dec 2015) // SNEWS neutrino coincidences and singles from supernovae
2nd VOEvent Ver 2.0 server (Nov 2015) // A redundant Ver 2.0 VOevent server added
FERMI_GBM LOCATION MAPS (Apr 2014) // GBM Location_Map URL available
FERMI_GBM_LIGHTCURVE (Apr 2014) // GBM Lightcurve URL available
FERMI_LAT_OFFLINE (Feb 2014) // LAT detections found in off-line ground processing
SUZAKU_LIGHTCURVE (Nov 2013) // Lightcurves from Suzaku-WAM
IPN_RAW resumes (Aug 2012) // IPN Team resumes producing the IPN_RAW notices
SWIFT_BAT_SUB_SUB_THRESHOLD (May 2012) // Swift-BAT Triggers with very low significance; use for temporal coincidences
VOEvent Direct Server (Mar 2012) // Added 3 VOEvent servers to allow for direct distribution of VOEvents
FERMI_LAT_MON/_TRANS (Aug 2011) // Flare-ups from known sources monitored by Fermi-LAT & non-GRB transients
FERMI_LAT_GND (Aug 2011) // Automated ground processing to get GRB positions
Sincerely,
Scott Barthelmy NASA-GSFC, Code 661, Greenbelt, MD 20771
PHONE: 301-286-3106 (office)
PHONE: 301-346-3733 (cell)
EMAIL: scott at milkyway.gsfc.nasa.gov
PAGER: 3013463733 at cingularme.com
WEB: http://gcn.gsfc.nasa.gov/gcn
///////////////////////// your current configuration ////////////////////////////
BEGIN_SITE
SITE_NAME VSNET
DATES 25jun05 23oct07
SITE_LON_LAT 135.75 35.00
DIST_METHOD EMAIL
DIST_ADDRESS vsnet-grb at ooruri.kusastro.kyoto-u.ac.jp
POC_NAME Daisaku Nogami
POC_ADDRESS vsnet-grb at ooruri.kusastro.kyoto-u.ac.jp
DAILY_REPORT_ENABLE 0
DAILY_REPORT_ADDRESS vsnet-grb at ooruri.kusastro.kyoto-u.ac.jp
CONFIG_REPORT 0
# Site-specific items:
TRIGGER_ID 0
INTENSITY -1.000
ERROR 360.1000
DELAY 999.9
SIGNIFICANCE 0.00
CONF_LEVEL 0.00
OBSERVABILITY ALL
ATTACHMENT NONE
SIMBAD_NED 0
# Type-specific items:
IPN_POS sim_ned=0
INTEGRAL_SPIACS
INTEGRAL_WAKEUP sim_ned=0
INTEGRAL_REFINED sim_ned=0
INTEGRAL_OFFLINE sim_ned=0
SWIFT_BAT_GRB_ALERT
SWIFT_BAT_GRB_POS trig_id=0
SWIFT_BAT_GRB_NACK_POS
SWIFT_BAT_GRB_LC trig_id=0
SWIFT_FOM_2OBS trig_id=0
SWIFT_SC_2SLEW trig_id=0
SWIFT_XRT_POS
SWIFT_XRT_NACK_POS
SWIFT_XRT_IMAGE
SWIFT_XRT_PROC_IMAGE
SWIFT_UVOT_POS inten=99.000
SWIFT_UVOT_IMAGE
SWIFT_UVOT_PROC_IMAGE
SWIFT_UVOT_SRCLIST
SWIFT_UVOT_PROC_SRCLIST
SWIFT_POINTDIR
SWIFT_TOO_FOM
SWIFT_TOO_SLEW
END_SITE
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