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Blog for Gamma Ray Bursts

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Burst Time 04:56:25 GCN4615
RA 15:16:53.76 GCN4615
DEC -36:54:43.20 GCN4615
Radius 2.00' GCN4615
Fluence (20-200 keV) 3e-07 erg cm-2 GCN4616
Peak Flux (20-200 keV) 2e-08 erg cm-2 s-1 GCN4616
OT? no (plot data)
Flter: H in 0 of 1 obs
Flter: I in 0 of 1 obs
Flter: J in 0 of 1 obs
Flter: K' in 0 of 1 obs
Flter: R in 0 of 4 obs
XT? no (plot data)
Range: 0.2-10 keV in 0 of 1 obs
Grab a ' X '
Or see the " JHKs band

Warning: pg_exec(): Query failed: ERROR: ltsWriteBlock: failed to write block 156 of temporary file Perhaps out of disk space? . in /home/grad40/www/display_burst.php on line 463


Displaying Bursts 1 to 1
Search matched 9 messages (refine search)
Displaying messages 1 to 9

GRB 060130: PROMPT Observations
Haislip et al.
Posted by Josh Haislip
06/01/31 19:21:35 GMT

We observed the localization of GRB 060130 (Mereghetti et al., GCN 4615) with three of the PROMPT telescopes simultaneously in r'Iz' beginning 23.8 hours after the burst under the automated control of Skynet: ...Full Text

GRB 060130: Further R-band imaging
Nielsen et al.
Posted by Johan U. Fynbo
06/01/31 12:39:48 GMT

"Using DFOSC on the Danish 1.5m telescope at La Silla, we have obtained further (3x600sec) R-band imaging of the field of the Integral-detected GRB 060130 (Mereghetti et al., GCN 4615) around Jan 31.3. By comparing to our image taken 4.3 hr after the burst (GCN 4620) we place a 3-sigma upper limit of R=23 on any transient sources 4.3 hr after the burst." ...Full Text

GRB 060130: Swift/XRT observation
Kennea et al.
Posted by Jamie A. Kennea
06/01/31 03:07:12 GMT

Swift began a target of opportunity observation of the INTEGRAL detected burst GRB 060130 (GCN 4615) at 15:18:04 UT January 30th 2006, 10.3 hours after the burst. We have analyzed 10ks of Swift/XRT data of the field of the INTEGRAL burst and detect no source in or near the 2 arcmin INTEGRAL error circle. Assuming a Crab like spectrum and galactic absorption, we calculate a 3 sigma upper...Full Text

GRB 060130: Optical imaging
Nielsen et al.
Posted by Johan U. Fynbo
06/01/30 13:53:50 GMT

"Using DFOSC on the Danish 1.5m telescope at La Silla, we have obtained R-band imaging of the field of the Integral-detected GRB 060130 (Mereghetti et al., GCN 4615) starting at Jan 30.375 (4.5h after the trigger). Visual comparison with the DSS-2 does not reveal any transient sources brighter than the DSS-2 limit. Our image reaches a detection limit slightly deeper than R=22....Full Text

GRB 060130: REM infrared observations
Testa et al.
Posted by Vincenzo Testa
06/01/30 11:28:03 GMT

The field of GRB 060130 (Mereghetti et al. GCN 4615) was observed with the REM telescope located in La Silla (Chile)....Full Text

GRB 060130, SMARTS optical observations
Cobb
Posted by Bethany Cobb
06/01/30 10:28:05 GMT

Using the ANDICAM instrument on the 1.3m telescope at CTIO, we obtained optical imaging of the error region of GRB 060130 (GCN 4615, Mereghetti et al.) starting 09:14 2006-01-30 UT (~4.3 hours post-burst). The imaging was conducted during twilight, which limited the number and depth of the images we were able to obtain. The ANDICAM's optical field of view is 6'x6' and, therefore, covers...Full Text

GRB 060130: FRAM optical observations
Kubanek et al.
Posted by Petr Kubanek
06/01/30 10:23:38 GMT

The wide field camera of the FRAM telescope, located at Pierre Auger observatory in Malargue, Argentina, observed the field of INTEGRAL GRB 060130 (D. Gotz et al., GCN 4615, GCN 4616) starting at 9:09:36 UT, eg. 4h 13m after GRB. Observations was manually triggered and started under dawn sky (but at favorable zenith distance ~ 25 deg)....Full Text

GRB 060130: further INTEGRAL IBIS results
Gotz & Mereghetti
Posted by Diego Gotz
06/01/30 09:28:47 GMT

GRB 060130 shows a single pulse light curve. Its peak flux integrated over 1 s (20-200 keV band) is 0.22 ph (2x10e-8 erg)/cmsq/s. Its fluence in the same energy band is 3x10e-7 erg/cmsq....Full Text

GRB 060130: a long GRB detected with INTEGRAL
Mereghetti et al.
Posted by Diego Gotz
06/01/30 08:43:36 GMT

A GRB lasting about 40 s has been detected by IBAS in IBIS/ISGRI data at 04:56:25 UT on January 30 2006....Full Text



Displaying messages 1 to 9




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