- GCN/BACODINE POSITION NOTICE
TITLE: GCN/SWIFT NOTICE
NOTICE_DATE: Sat 16 Jul 05 12:36:37 UT
NOTICE_TYPE: Swift-BAT GRB Position
TRIGGER_NUM: 146227, Seg_Num: 0
GRB_RA: 338.598d {+22h 34m 23s} (J2000),
338.659d {+22h 34m 38s} (current),
338.039d {+22h 32m 09s} (1950)
GRB_DEC: +38.696d {+38d 41' 46"} (J2000),
+38.725d {+38d 43' 29"} (current),
+38.437d {+38d 26' 14"} (1950)
GRB_ERROR: 4.00 [arcmin radius, statistical only]
GRB_INTEN: 10377 [cnts] Image_Peak=203 [image_cnts]
TRIGGER_DUR: 2.048 [sec]
TRIGGER_INDEX: 486 E_range: 25-100 keV
BKG_INTEN: 102376 [cnts]
BKG_TIME: 45328.00 SOD {12:35:28.00} UT
BKG_DUR: 24 [sec]
GRB_DATE: 13567 TJD; 197 DOY; 05/07/16
GRB_TIME: 45363.63 SOD {12:36:03.63} UT
GRB_PHI: 42.67 [deg]
GRB_THETA: 39.14 [deg]
SOLN_STATUS: 0x3
RATE_SIGNIF: 9.38 [sigma]
IMAGE_SIGNIF: 8.00 [sigma]
MERIT_PARAMS: +1 +0 +0 +2 +2 +5 +0 +0 +30 +1
SUN_POSTN: 115.97d {+07h 43m 52s} +21.29d {+21d 17' 38"}
SUN_DIST: 107.88 [deg]
MOON_POSTN: 223.55d {+14h 54m 12s} -19.30d {-19d 18' 16"}
MOON_DIST: 121.28 [deg]
MOON_ILLUM: 69 [%]
GAL_COORDS: 95.61,-16.80 [deg] galactic lon,lat of the burst (or transient)
ECL_COORDS: 359.00, 43.38 [deg] ecliptic lon,lat of the burst (or transient)
COMMENTS: SWIFT-BAT GRB Coordinates.
COMMENTS: This is a rate trigger.
COMMENTS: A point_source was found.
COMMENTS: This does not match any source in the on-board catalog.
COMMENTS: This does not match any source in the ground catalog.
COMMENTS: This is a GRB.
- red DSS finding chart
ps-file
- GCN/SWIFT NOTICE
TITLE: GCN/SWIFT NOTICE
NOTICE_DATE: Sat 16 Jul 05 12:39:45 UT
NOTICE_TYPE: Swift-BAT GRB Lightcurve
TRIGGER_NUM: 146227, Seg_Num: 0
GRB_RA: 338.598d {+22h 34m 23s} (J2000),
338.659d {+22h 34m 38s} (current),
338.039d {+22h 32m 09s} (1950)
GRB_DEC: +38.696d {+38d 41' 46"} (J2000),
+38.725d {+38d 43' 29"} (current),
+38.437d {+38d 26' 14"} (1950)
GRB_DATE: 13567 TJD; 197 DOY; 05/07/16
GRB_TIME: 45363.63 SOD {12:36:03.63} UT
TRIGGER_INDEX: 486
GRB_PHI: 42.67 [deg]
GRB_THETA: 39.14 [deg]
DELTA_TIME: 65530.00 [sec]
LC_URL: sw00146227000msb.lc
SUN_POSTN: 115.97d {+07h 43m 52s} +21.29d {+21d 17' 38"}
SUN_DIST: 107.88 [deg]
MOON_POSTN: 223.55d {+14h 54m 12s} -19.30d {-19d 18' 16"}
MOON_DIST: 121.28 [deg]
MOON_ILLUM: 69 [%]
GAL_COORDS: 95.61,-16.80 [deg] galactic lon,lat of the pointing direction
ECL_COORDS: 359.00, 43.38 [deg] ecliptic lon,lat of the pointing direction
COMMENTS: SWIFT-BAT GRB Lightcurve.
COMMENTS:
COMMENTS: The next comments were copied from the BAT_POS Notice:
COMMENTS: This is a rate trigger.
COMMENTS: A point_source was found.
COMMENTS: This does not match any source in the on-board catalog.
COMMENTS: This does not match any source in the ground catalog.
COMMENTS: This is a GRB.
- GCN notice #3623
E. Rol, C. Hurkett, K. Page (U. Leicester), S. Barthelmy, L. Barbier,
A. Parsons (GSFC), J. Cummings (NRC, GSFC), D. Palmer (LANL),
D. Burrows, J. Kennea (PSU), K. McGowan (MSSL), N. Gehrels (GSFC),
report for the Swift team:
At 12:36:04 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 050716 (trigger=146227). The BAT on-board calculated
location is RA,Dec 338.598d {+22h 34m 23s}, +38.696d {+38d 41' 46"}
(J2000), with an uncertainty of 4 arcmin (radius, including estimated
systematic uncertainty; 90% containment). The BAT light curve showed
a multi-peak structure with a duration of at least 40 seconds. The
15-350 keV peak count rate was ~1300 counts/sec, measured by BAT at
~10 seconds after the trigger.
The spacecraft slewed immediately and the XRT began observing the
burst at 12:37:40 UT (96 seconds after the BAT trigger). The XRT found
a bright, uncatalogued X-ray source. The on board calculated position
is:
RA: 22h 34m 20.4s (J2000),
Dec: -38d 40' 56.7" (J2000).
This position is 60.6 arcseconds from the BAT position. The estimated
uncertainty is 6 arcseconds radius (90% containment).
The Swift Ultra Violet/Optical Telescope (UVOT) observations began at
12:37:43 UT, 99 seconds after the BAT trigger. The first data taken
after the spacecraft settled was a 100 sec exposure using the V filter
with the midpoint of the observation at 149 sec after the BAT
trigger. Based on comparisons to the DSS, we detect no new source at
the XRT position.
- GCN notice #3624
J. Kennea, D. Burrows (PSU), E.Rol, C. Hurkett, K. Page (U. Leicester) and
N. Gehrels (GSFC) report for the Swift/XRT Team:
In GCN 3623 we reported an incorrect sign on the declination of the XRT
position for GRB050716. The corrected position is:
RA: 22h 34m 20.4s (J2000),
Dec: +38d 40' 56.7" (J2000).
With an estimated uncertainty of 6 arcseconds radius (90% containment).
- GCN notice #3625
C. Guidorzi, A. Gomboc, A. Monfardini, I. A. Steele, C.J. Mottram,
C.G. Mundell, R.J. Smith, D. Carter, M.F. Bode (Liverpool JMU),
E. Rol, P. O'Brien, N. Bannister (Leicester) report:
"The 2-m Faulkes North Telescope followed up robotically the GRB050716
detected by SWIFT (Rol et al. GCN 3623) 3.8 min after the GRB trigger
time. The automatic "detection mode" procedure did not detect any obvious
candidate up to about R=19.8 from 3 10-s images (mean epoch of 4.3 min
after the GRB), with FOV of 4.6'x4.6' centred on the BAT in-flight
location.
The limiting magnitude is automatically calculated with respect to the
USNOB1.0 'R2' values of the field objects.
Further observations are ongoing.
This message can be cited"
- GCN notice #3626
K. Torii (Osaka U.) reports on behalf of the ART collaboration:
The error region of GRB 050716 (Rol et al. GCN 3623) was observed by
the Automated Response Telescope. The observation started at 2005 July
16 12:38:26 UT (142 s after the trigger) and BVRcIc frames of 60s
integration were acquired.
We do not detect an optical counterpart of the X-ray afterglow (GCN
3623, 3624) and derive its 3-sigma upper limit relative to
USNO-B1.0 magnitude as follows.
================================
Start(UT) Filter Mag Exposure
--------------------------------
12:55:06 Ic >16.5 60s x27
--------------------------------
- GCN notice #3627
E.Sonoda,S.Maeno,Y.Tokunaga,Myamauchi
(University of Miyazaki)
We have observed the field covering the error circle
of GRB 050716 (GCN 3623,3624;Swift BAT Trigger time is
12:36:04 UT) with the unfiltered CCD camera on the
30-cm telescope at University of Miyazaki. The observation was started
14:28:47 UT on July.16. We have compared with the USNO A2.0 catalog.
Preliminary analysis shows there is no new source brighter than 16.8 mag.
- GCN notice #3628
Z.Y. Lin(NCU), K.Y. Huang, W.H. Ip (NCU), Y. Urata(RIKEN),
Y. Qiu (BAO), Y.Q. Lou (THCA) on behalf of EAFON report:
"We have imaged the GRB 050716 X-ray afterglow position (Rol et
al. GCN 3623; J. Kennea et al. 3264) with B and R band using Lulin
1-m telescope. The observation was started at 14:30 (0.079 days after
the burst) after rising the field. These images show no optical
counterpart brighter than B=21.6 and R=21.3. These 3-sigma limiting
magnitudes are derived from the USNO-B1.0 catalogue.
This message may be cited."
- GCN notice #3629
S. Barthelmy (GSFC), L. Barbier (GSFC), J. Cummings (GSFC/NRC),
E. Fenimore (LANL), N. Gehrels (GSFC), D. Hullinger (GSFC/UMD),
H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), D. Palmer (LANL),
A. Parsons (GSFC), T. Sakamoto (GSFC/NRC), J. Tueller (GSFC),
M. Chester (PSU), L. Angelini (GSFC/JHU)
on behalf of the Swift-BAT team:
Using the full data set from the recent telemetry downlink, we report
further analysis of Swift-BAT Trigger #146227 (E. Rol, et al., GCN 3623).
The ground-analysis position is RA,Dec 338.607, 38.682 (J2000) with an
uncertainty of 3 arcmin (radius, 90%, stat+sys). T90 is 69 +/-1 sec.
The burst had a slow rise and slow decay with two broad peaks centered
at T+12 and T+44 seconds. Fitting a cutoff power law over the full interval
from T-14 to T+76 seconds, the photon index is 0.79 +/- 0.26, Epeak is
104 +29 -15 keV and the Norm at 1 keV is 0.34 +0.38 -.19 with a fluence
of 8.3 +1.3 -0.6 X 10^-6 erg/cm^2 in the 15-350 keV band (90% c.l.).
The peak flux in a 1-sec wide window starting at T+12.2 seconds
is 2.23 +/- 0.41 ph/cm^2/sec (15-350 keV).
- GCN notice #3630
C. Hurkett, E. Rol, K. Page (U. Leicester), D. Burrows (PSU), J. Norris
(GSFC), K. Hurley (Berkeley) and N. Gehrels (GSFC) report for the Swift
XRT team:
We have analysed the XRT data for GRB 050716 (GCN 3623, Rol et al) taken
104 seconds after the trigger. PSF fitting of the candidate afterglow in
the photon counting (PC) mode observations yields a refined position of
(J2000)
RA 22:34:20.5
Dec +38:40:57.1
with an uncertainty of 6 arcseconds (90% containment). This position is
less than 1 arcsecond from the position reported in GCN 3624 (Kennea et
al).
XRT observations began in Windowed Timing (WT) mode 104 seconds after the
trigger and show a decline with a power-law decay index of 1.68
+/- 0.04 with flares at approximately 177 and 386 seconds.
The decay index appears to stay the same at least until 6000 seconds after
the trigger.
The spectrum between 104 and 517 seconds after the trigger (WT data) has
an average photon index of 1.32 (+/-0.04), with the absorption fixed at
its Galactic value of 1.1e21 cm^-2. There is no evidence at the present
time for excess absorption. The mean unabsorbed flux in WT mode at 230s
(logarithmic mean time) is 7.02 (+0.27/-0.24) x 1e-10 erg/cm^2/s in the
0.5-10.0 keV energy range
- GCN notice #3631
K. McGowan (MSSL), E. Rol (U. Leicester), J. Nousek (PSU),
F. Marshall, N. Gehrels (GSFC) report on behalf of the
Swift UVOT team:
Using summed images from Swift/UVOT of the field of
GRB 050716 (Rol et al., GCN 3623), taken from 99
seconds after the BAT trigger, no new source is detected
within the XRT error circle (Hurkett et al., GCN 3630) in
any of the six filters down to the following 3-sigma
magnitude upper limits:
Filter Exposure (s) T_mid (s) 3-sig limit
V 178 487 19.1
B 979 3121 21.1
U 978 2660 20.7
UVW1 178 2200 19.7
UVM2 88 545 19.5
UVW2 755 3468 20.8
where T_mid is the mid-point of the summed observation.
We caution that the instrument is not yet fully
calibrated and that the magnitude limits presented here
may need to be refined.
- GCN notice #3632
N. Tanvir, K. Lowe, T. Gledhill (U. of Hertfordshire), A. Levan,
E. Rol, P. O'Brien, N. Bannister (U. of Leicester), T. Carroll (JACH),
C. Guidorzi, A. Gomboc, A. Monfardini, I. Steele, C. Mundell,
C. Mottram, M. Bode R. Smith, D. Carter (Liverpool JMU) report:
We imaged the Swift/XRT error circle of GRB 050716 (GCN 3623/3624)
with UKIRT/UFTI starting about 56 minutes post-burst.
Just outside the XRT error circle we find a fading point source
at position (astrometry relative to nearby 2MASS star):
22 34 20.73 +38 41 03.6 (J2000)
Provisional photometry indicates that this source declines from K~17.8
to K~18.3 between two integrations separated by about 30 mins, making it
very likely to be the afterglow of GRB 050716.
Interestingly, it also appears to be red with J-K~2.5. A reanalysis
of the very early FT-N data (GCN 3625), however, shows excess flux in
R and I at the source position which, although not a clear detection
(due to the faintness and proximity of nearby USNO star), suggests
that the source is probably reddened rather than at very high
redshift.
Images can be found at:
http://star-www.herts.ac.uk/~nrt/050716.html
Further observations are planned.
This message may be cited.
- GCN notice #3641
J. Gorosabel, A.J. Castro-Tirado (IAA-CSIC, Granada), R. Lopez (Univ. of
Barcelona), G. Andreuzzi (TNG, La Palma), A. de Ugarte Postigo, S. Guziy,
M. Jelinek (IAA-CSIC, Granada), O. Bogdanov (Nikolaev State Univ.),
report:
"We have observed the field of GRB 050716 (Rol et al., GCN Circ. 3623)
with the 3.5m TNG telescope on June 17.231-17.242 UT in the J-band (Texp =
15 min). The afterglow candidate reported by Tanvir et al. (GCN Circ. 3632)
is not detected in our final combined image, which has a 3 sigma limiting
magnitude of J~22."
This message can be cited.
- GCN notice #3789
C. Rodgers, E. Hausel, D. Allen and R. Canterna report on behalf of
the Red Buttes Observatory GRB Team as
part of the FUN GRB Collaboration. We responded to GRB 050714A (GCN 3607) at
05:11:41 UT with a series of 10 minute R and I exposures centered on
the positon of the original
Integral GRB Position under excellent conditions. No new source was
detected after comparison with DSS.
UT Time Since Filter Limiting
Start GRB Magnitude
05:11 5:06 I 17.4
05:33 5:28 R 18.4
05:43 5:38 R 18.4
We also responded to GRB 050716 (GCN 3623) at 2005-07-17 05:52:03 UT.
We took a series of 5 and 10 minute
exposures in R and I with limiting magnitues of 18.6 in R and 17.4 in
I. These observations were started 17
hours after the BAT trigger. No new source was
detected after comparison with DSS.
10 sigma limiting magnitudes were derived from the USNO-B1.0 catalogue
- astro-ph/0611554 from 17 Nov 2006
Rol: The early and late-time spectral and temporal evolution of GRB 050716
We report on a comprehensive set of observations of Gamma Ray Burst 050716,
detected by the Swift satellite and subsequently followed-up rapidly in X-ray,
optical and near infra-red wavebands. The prompt emission is typical of
long-duration bursts, with two peaks in a time interval of T90 = 68 seconds (15
- 350 keV). The prompt emission continues at lower flux levels in the X-ray
band, where several smaller flares can be seen, on top of a decaying light
curve that exhibits an apparent break around 220 seconds post trigger. This
temporal break is roughly coincident with a spectral break. The latter can be
related to the extrapolated evolution of the break energy in the prompt
gamma-ray emission, and is possibly the manifestation of the peak flux break
frequency of the internal shock passing through the observing band. A possible
3 sigma change in the X-ray absorption column is also seen during this time.
The late-time afterglow behaviour is relatively standard, with an electron
distribution power-law index of p = 2 there is no noticable temporal break out
to at least 10 days. The broad-band optical/nIR to X-ray spectrum indicates a
redshift of z ~> 2 for this burst, with a host-galaxy extinction value of
E(B-V) ~ 0.7 that prefers an SMC-like extinction curve.
- astro-ph/0611554 from 17 Nov 2006
Rol: The early and late-time spectral and temporal evolution of GRB 050716
We report on a comprehensive set of observations of Gamma Ray Burst 050716,
detected by the Swift satellite and subsequently followed-up rapidly in X-ray,
optical and near infra-red wavebands. The prompt emission is typical of
long-duration bursts, with two peaks in a time interval of T90 = 68 seconds (15
- 350 keV). The prompt emission continues at lower flux levels in the X-ray
band, where several smaller flares can be seen, on top of a decaying light
curve that exhibits an apparent break around 220 seconds post trigger. This
temporal break is roughly coincident with a spectral break. The latter can be
related to the extrapolated evolution of the break energy in the prompt
gamma-ray emission, and is possibly the manifestation of the peak flux break
frequency of the internal shock passing through the observing band. A possible
3 sigma change in the X-ray absorption column is also seen during this time.
The late-time afterglow behaviour is relatively standard, with an electron
distribution power-law index of p = 2 there is no noticable temporal break out
to at least 10 days. The broad-band optical/nIR to X-ray spectrum indicates a
redshift of z ~> 2 for this burst, with a host-galaxy extinction value of
E(B-V) ~ 0.7 that prefers an SMC-like extinction curve.
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