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Автор Тема: Наблюдаем гамма-всплески  (Прочитано 56093 раз)
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« : 11 Декабрь 2010, 11:53:39 »

Нашёл таблицу наблюдений гамма-всплесков Swift GRB Table

•The most recent 50 of 622 bursts are displayed here.
•Database last updated: Thursday, December 09, 2010, 19:24:25 EST
•Download this table as a tab-delimited text file: grb_table_1292056730.txt

http://heasarc.gsfc.nasa.gov/docs/swift/archive/grb_table/grb_table.php?obs_swift=1&obs_ipn=1&obs_integral=1&obs_hete=1&obs_agile=1&obs_fermi=1&year=All+Years&restrict=none&grb_time=1&grb_trigger=1&other_obs=1&redshift=1&host=1&comments=1&references=1&bat_location=1&bat_t90=1&bat_fluence=1&xrt_location=1&xrt_first_obs=1&xrt_early_flux=1&uvot_location=1&uvot_first_obs=1&uvot_vmag=1&number=50

Там упоминаются 2 наших телескопа - ISON-NM в Нью-Мексико (три раза) и GAS-250 в Уссурийске.
Также встречаются ЗТШ, АЗТ-33ИК, АЗТ-14 (видимо, тоже Монды), АЗТ-22 на Майданаке, и русско-турецкий 1,5-м телескоп RTT150, АЗТ-11 в Кампо-Императоре.

Цейсс-2000 - это, видимо, Терскол. Есть еще загадочная RAS Observatory.

Почему-то МАСТЕР упоминается всего лишь 3 раза. Вот тебе и сеть для наблюдения гамма-всплесков.  В замешательстве

* grb_table_1292056730.txt (14.21 Кб - загружено 395 раз.)
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« Ответ #316 : 05 Август 2016, 19:04:24 »

TITLE:   GCN CIRCULAR
NUMBER:  19776
SUBJECT: GRB 160804A: TSHAO optical observations
DATE:    16/08/05 15:44:31 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), A. Kusakin (Fesenkov Astrophysical Institute), I. Reva
(Fesenkov Astrophysical Institute), A. Volnova (IKI), A. Pozanenko (IKI)
report on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 160804A (Marshall et al., GCN 19761)  with
Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical Observatory.
We obtained several images in R filter starting on August 04 (UT)
15:08:18. We clearly detected  optical source reported by Breeveld et
al. (GCN 19764), Tyurina et al. (GCN 19768), Malesani et al. (GCN
19770), Moskvitin et al. (GCN 19771), Xu et al. (GCN #19773) and Bolmer
et al. (GCN 19774). Preliminary photometry of a combined image is following

Date       UT start   t-T0   Filter   Exp.  OT     Err.  UL
                       (mid, days)     (s)

2016-08-04 15:08:18 0.58601  R       26*120 20.30  0.10  21.4

Photometry is based on nearby SDSS DR9 stars

SDSS-DR9_id    R(Lupton)
J144642.43+100147.7    18.068
J144642.15+100017.4    17.644
J144638.04+095917.6    17.971
J144635.67+095910.6    18.378
J144632.91+100104.9    17.910
J144619.22+095958.1    16.677
J144616.60+100018.4    16.575
J144614.88+100001.4    16.544
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« Ответ #317 : 22 Август 2016, 08:37:51 »

TITLE:   GCN CIRCULAR
NUMBER:  19829
SUBJECT: GRB 160816A: TSHAO optical observations
DATE:    16/08/21 13:37:01 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), I. Reva (Fesenkov Astrophysical Institute), A. Kusakin
(Fesenkov Astrophysical Institute),  A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of 160816A (Racusin et al., GCN 19802; Mailyan et
al., GCN 19804)  with Zeiss-1000 (East) 1-m telescope of Tien Shan
Astronomical Observatory
. We obtained several images in R filter
starting on August 17 and 18.  We detected  optical afterglow (Guidorzi
et al. GCN 19808; Troja et al. GCN 19809) on Aug. 17 and obtained upper
limit on Aug. 18. Preliminary photometry of a combined image is following

Date       UT start   t-T0   Filter   Exp.  OT     Err.  UL
                       (mid, days)     (s)

2016-08-17 21:32:28 1.19553  R      105*30 21.70  0.20  21.9
2016-08-18 19:11:47 2.11663  R      148*30 n/d    n/d   22.1


Photometry is based on nearby USNO-B1.0 stars
USNO-B1.0_id    R2
1271-0576219    17.27
1271-0576200    17.52
1271-0576190    18.12
1271-0576101    17.00
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« Ответ #318 : 26 Август 2016, 01:06:46 »

TITLE:   GCN CIRCULAR
NUMBER:  19862
SUBJECT: GRB 160824A: ISON/Terskol optical observations
DATE:    16/08/25 18:20:16 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), A. Mokhnatkin (KIAM),  A. Volnova (IKI), Molotov (KIAM),
A. Pozanenko  (IKI) report on behalf of larger GRB follow-up collaboration

We observed the field of GRB 160824A (Evans   et al., GCN 19855)  with K-800
(0.8m f/2.9)   telescope  of ISON/Terskol   observatory. We obtained several
unfiltered images starting on  August 24 (UT) 23:58:36.  We detected
optical source in coordinates
(J2000) 05:20:21.18 +40:01:43.5 with uncertainty of 1 arcsec in both
coordinates. This is 2.6 arcsec apart of the center of the enhanced XRT
error circle (Goad et al., GCN 19857).  At this time we cannot say nothing
about variability of the object.  It is not clear whether our source is the
same as the source reported by Marshall et al. (GCN 19860).  Preliminary
photometry of a combined image is following

Date               UT start   t-T0       Filter   Exp.   OT    Err.  UL
                       (mid, days)    (s)

2016-08-24 23:58:36 0.02758 CR      400    20.6   0.3  20.9

Photometry is based on nearby USNO-B1.0 stars
USNO-B1.0_id    R2
1300-0122742    18.17
1300-0122665    18.04
1300-0122653    18.66
1300-0122680    17.00
1300-0122864    17.60
1299-0128308    18.00
1300-0122784    17.56
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« Ответ #319 : 04 Октябрь 2016, 21:03:54 »

TITLE:   GCN CIRCULAR
NUMBER:  19980
SUBJECT: GRB 161004A: TSHAO optical observations
DATE:    16/10/04 17:44:41 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), I. Reva (Fesenkov Astrophysical Institute), A. Kusakin
(Fesenkov Astrophysical Institute),  A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 161004A  (Evans  et al., GCN 19979)  with
Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical Observatory.
We obtained several images in R filter starting on Oct. 04 (UT)
13:36:52.  In the XRT error circle we do not detect any new object. Wa
do not detect also candidate afterglow (Evans  et al., GCN 19979).
Preliminary photometry of a combined image is following

Date       UT start   t-T0   Filter   Exp.  OT     Err.  UL
                       (mid, days)     (s)
2016-10-04 13:36:52 0.04321  R       15*180 n/d    n/d   21.9

Photometry is based on nearby SDSS-DR9 stars (Lupton transformations):
SDSS-DR9_id         R(Lupton)
J173243.09-005731.3 17.04
J173250.91-005842.7 16.77
J173251.94-005803.2 15.75
J173253.88-005801.6 15.62
J173253.02-005938.3 16.02
J173232.00-005640.3 16.34
J173227.11-005646.8 16.41
J173227.04-005816.8 16.51
J173227.48-005856.9 16.62
J173236.27-010018.1 16.96
J173241.54-005823.1 16.26

A finding chart can be found at
http://grb.rssi.ru/GRB161004A/GRB161004A_TSHAO_161004_XRT_UVOT.png
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« Ответ #320 : 08 Октябрь 2016, 08:20:51 »

TITLE:   GCN CIRCULAR
NUMBER:  20011
SUBJECT: GRB 161004A: refined analysis of TSHAO optical observations
DATE:    16/10/07 23:58:37 GMT
FROM:    Alexei Pozanenko at IKI, Moscow  <apozanen@iki.rssi.ru>

E. Mazaeva (IKI), I. Reva (Fesenkov Astrophysical Institute), A. Kusakin
(Fesenkov Astrophysical Institute),  A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We present a refined analysis of our observations (Mazaeva et al., GCN
19980) of  the field of GRB 161004A  (Evans  et al., GCN 19979)  with
Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical Observatory.
We obtained several images in R filter starting on Oct. 04 (UT)
13:36:52.  In a combined image of the first 30 minutes of our
observations we detect the afterglow (Breeveld et al., GCN 19984).
Preliminary photometry of a combined image is following

Date       UT start   t-T0   Filter   Exp.  OT     Err.  UL
                       (mid, days)     (s)
2016-10-04 13:36:52 0.03632  R       9*180  21.65  0.25  21.7

Photometry is based on nearby SDSS-DR9 stars used in GCN 19980.
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« Ответ #321 : 12 Октябрь 2016, 11:46:37 »

TITLE:   GCN CIRCULAR
NUMBER:  20030
SUBJECT: GRB 161011A: TSHAO afterglow candidate
DATE:    16/10/11 22:10:02 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), A. Kusakin (Fesenkov Astrophysical Institute),  A.
Volnova (IKI),  I. Reva (Fesenkov Astrophysical Institute), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 161011A  (D'Elia et al., GCN 20023)  with
Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical Observatory.
We obtained several images in R filter starting on Oct. 11 (UT)
13:13:27.  In the enhanced XRT error circle (Osborne al., GCN 20026) we
marginally detect an object which is absent in SDDS-DR9 catalog.
Preliminary photometry of the object which we suggest as an afterglow
candidate is following

Date       UT start   t-T0    Filter  Exp.   OT     Err.  UL
                       (mid, days)     (s)
2016-10-11 13:13:27   0.32098 R       21*120 20.6   0.3   20.8

Photometry is based on nearby SDSS-DR9 stars (Lupton transformations):
SDSS-DR9_id            R
J162253.68+081834.3    15.26
J162242.22+082241.1    14.18
J162312.65+081527.2    14.72
J162302.30+081614.7    14.96

A finding chart can be found at
http://grb.rssi.ru/GRB161011A/GRB161011A_TSHAO_161011_fc.png
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« Ответ #322 : 15 Октябрь 2016, 12:03:27 »

TITLE:   GCN CIRCULAR
NUMBER:  20042
SUBJECT: GRB 161014A: TSHAO optical observations
DATE:    16/10/15 00:07:46 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), A. Kusakin (Fesenkov Astrophysical Institute),  I.
Reva (Fesenkov Astrophysical Institute), A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 161014A  (Racusin et al., GCN 20035)  with
Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical Observatory.
We obtained several images in R filter starting on Oct. 14 (UT)
13:48:35. We detected the afterglow of GRB 161014A (Morita et al., GCN
20036; Guidorzi et al., GCN 20037; Xin et al., GCN 20038). Preliminary
photometry of  of combined the first observational set is following

Date       UT start   t-T0   Filter   Exp.   OT   Err.  UL
                       (mid, days)     (s)
2016-10-14 13:48:35   0.07046  R      21*120 19.0 0.10  20.6

Photometry is based on nearby SDSS-DR9 stars (Lupton transformations):
SDSS-DR9_id         R(Lupton)

J221053.78+072643.3    14.88
J221018.77+072726.4    14.05
J221023.66+073006.3    15.49
J221024.28+072335.5    15.75
J221050.55+072341.7    17.10
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« Ответ #323 : 10 Ноябрь 2016, 01:00:41 »

TITLE:   GCN CIRCULAR
NUMBER:  20160
SUBJECT: GRB 161108A: TSHAO optical observations
DATE:    16/11/09 21:29:59 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), A. Kusakin (Fesenkov Astrophysical Institute),  I.
Reva (Fesenkov Astrophysical Institute), A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 161108A  (Beardmore et al., GCN 20145)
with Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical
Observatory
. We obtained several images in R filter starting on Nov. 08
(UT) 23:06:16. Within enhanced XRT position (Beardmore et al., GCN
20147) we detected a source coinciding with the afterglow of GRB 161014A
(Malesani et al., GCN 20146; Butler et al., GCN 20149). Preliminary
photometry of the source is following

Date       UT start   t-T0   Filter   Exp.   OT   Err.  UL
                       (mid, days)     (s)
2016-11-08 23:06:16   0.83869  R      28*120 21.8 0.20  22.0

Our photometry of the afterglow might be  affected by nearby galaxy
mentioned in GCN 20149 (Malesani et al.)

Photometry is based on nearby SDSS-DR9 stars (Lupton transformations):
SDSS-DR9_id         R(Lupton)
J120315.88+245217.4 18.37
J120326.17+245228.7 18.71
J120318.05+245356.7 18.52
J120250.21+245354.3 18.35
J120258.81+245024.2 16.90
J120314.67+244944.0 17.06
J120321.43+244829.2 16.79
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« Ответ #324 : 11 Ноябрь 2016, 13:45:50 »

TITLE:   GCN CIRCULAR
NUMBER:  20167
SUBJECT: GRB 161108A: continued TSHAO optical observations
DATE:    16/11/10 20:53:57 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), A. Kusakin (Fesenkov Astrophysical Institute),  I.
Reva (Fesenkov Astrophysical Institute), A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 161108A  (Beardmore et al., GCN 20145) with
Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical Observatory.
We obtained several images in R filter starting on Nov. 09 (UT)
22:52:14. Within enhanced XRT position (Beardmore et al., GCN 20147) we
detected the afterglow of GRB 161014A (Malesani et al., GCN 20146;
Butler et al., GCN 20149). Preliminary photometry of the afterglow is
following

Date       UT start   t-T0   Filter   Exp.   OT   Err.  UL
                       (mid, days)     (s)
2016-11-09 22:52:14   1.83762  R      41*120 22.0 0.24  22.2

The photometry of the afterglow might be  affected by nearby galaxy
mentioned in GCN 20149 (Malesani et al.)

Photometry is based on nearby SDSS-DR9 stars (Mazaeva et al., GCN 20160).
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« Ответ #325 : 14 Ноябрь 2016, 05:15:43 »

Сели на точку GRB161113A
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« Ответ #326 : 15 Ноябрь 2016, 09:51:29 »

TITLE:   GCN CIRCULAR
NUMBER:  20175
SUBJECT: GRB 161113A: Kuban State University optical upper limit
DATE:    16/11/14 19:08:55 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), A. Ivanov (KubSU), V. Ivanov (KubSU), V. Lysenko
(KubSU), D. Ivanova (KubSU), A. Volnova (IKI), A. Pozanenko (IKI) report
on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 161113A (D'Avanzo, et al., GCN 20172) with
the RC510 telescope (0.51-m f/8) of Kuban State University Astrophysical
Observatory
. We obtained several unfiltered  images   starting on Nov.
14 (UT) 02:02:08. Within enhanced XRT position (Evans et al., GCN 20174)
we do not detect any source. Preliminary photometry of the field is
following

   Date       UT start   t-T0    Filter  Exp.  OT   Err. UL(3 sigma)
                        (mid, days)      (s)
2016-11-14   02:02:08   0.37062 CR      52*30 n/d  n/d  18.9

Photometry is based on nearby USNO-B1.0 stars (R2 magnitudes).
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« Ответ #327 : 29 Ноябрь 2016, 19:54:46 »

TITLE:   GCN CIRCULAR
NUMBER:  20215
SUBJECT: GRB 161129A: TSHAO optical observations / possible afterglow+host galaxy
DATE:    16/11/29 16:41:01 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), I. Reva (Fesenkov Astrophysical Institute), A. Kusakin
(Fesenkov Astrophysical Institute),  A. Volnova (IKI), A. Pozanenko
(IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of 161129A  (Kocevski et al., GCN 20210)  with
Zeiss-1000 (East) 1-m telescope of Tien Shan Astronomical Observatory.
We obtained several images in R filter starting on 2016-11-29 (UT)
12:51:12.  Within enhanced XRT position (Beardmore et al. GCN 20211)  we
detected  optical source which is absent in USNO-B1.0 but barely visible
in DSS2 (red). At the moment we can not say anything about the source
variability. The source might be a superposition of the afterglow and a
host galaxy.  Preliminary photometry of the source  is following

Date       UT start   t-T0   Filter  Exp.   OT     Err.  UL
                       (mid, days)    (s)

2016-11-29 12:51:12 0.25949  R       13*300 20.60  0.06  22.4

Photometry is based on nearby USNO-B1.0 stars
USNO-B1.0_id    R2
1221-0612083 17.30
1221-0612140 19.02
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« Ответ #328 : 17 Декабрь 2016, 10:35:25 »

TITLE:   GCN CIRCULAR
NUMBER:  20279
SUBJECT: GRB 161214B: AbAO and ISON/Terskol optical observations
DATE:    16/12/17 07:25:30 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI), R. Inasaridze (AbAO),  A. Mokhnatkin (KIAM),  A. Pozanenko
(IKI), A. Volnova (IKI),  V. Ayvazian  (AbAO), V. Zhuzhunadze,  (AbAO),
O.Kvaratskhelia  (AbAO), G. Inasaridze (AbAO),  I. Molotov (KIAM)  report on
behalf of  larger GRB follow-up collaboration:

We observed the field of  GRB 161214B  (D'Avanzoet al., GCN 20257) with
AS-32 (0.7m) telescope of Abastumani Observatory  and with K-800 (0.8m)
telescope  of ISON/Terskol   observatory  on December, 15.  We obtained
several unfiltered images in each observatory. The source previously
reported (Malesani et al. GCN 20260; Marshall et al. GCN 20261) is clearly
visible. Preliminary photometry of the source is following

Date       UT start   t-T0    Filter  Exp.     OT     Err.  UL
                      (mid, days)      (s)

2016-12-15 15:31:49  0.97738   CR     85*60   18.79   0.05  22.2  AS-32
2016-12-15 18:07:05  1.06047   CR    142*30  18.76   0.13  21.4  K-800

Photometry is based on R-magnitudes the same stars used in (Mazaeva et al.,
GCN  20275)
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« Ответ #329 : 22 Декабрь 2016, 23:37:05 »

TITLE:   GCN CIRCULAR
NUMBER:  20309
SUBJECT: GRB 161219B: ISON/Terskol optical observations
DATE:    16/12/20 21:25:52 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI),   A. Mokhnatkin (KIAM),  A. Pozanenko (IKI), A.
Volnova (IKI),   I. Molotov (KIAM)  report on behalf of  larger GRB
follow-up collaboration:

We observed the field of GRB 161219B (Swift trigger 727541; D'Ai,
GCN 20296) with K-800 (0.8m) telescope  of ISON/Terskol   observatory
starting  on December, 19 (UT) 18:57:51, i.e. about 9 minutes after GRB
onset.  We obtained several unfiltered images of 30 s exposure. The
optical afterglow (D'Ai et al., GCN 20296; Kruehler et al., GCN 20299;
Guidorzi et al., GCN 20300; Martin-Carrillo et al., GCN 20305) is
clearly visible in separate images. Preliminary light curve of the
afterglow can be found in

http://grb.rssi.ru/GRB161219B/GRB161219B_161219_K800.png

Photometry is based on nearby USNO-B1.0 stars
USNO-B.1_id     R2
0631-0120570    13.78
0632-0119151    14.86
0632-0119187    14.03
0632-0119198    15.05
0632-0119218    14.66
0631-0120752    14.81
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« Ответ #330 : 26 Декабрь 2016, 16:15:51 »

TITLE:   GCN CIRCULAR
NUMBER:  20340
SUBJECT: GRB 161224A: TSHAO optical observations
DATE:    16/12/26 13:04:31 GMT
FROM:    Alexei Pozanenko at IKI, Moscow

E. Mazaeva (IKI),  I. Reva (Fesenkov Astrophysical Institute), A.
Kusakin (Fesenkov Astrophysical Institute), A. Volnova (IKI), A.
Pozanenko (IKI) report on behalf of larger GRB follow-up collaboration:

We observed the field of GRB 161224A  (Swift trigger=728268,
Cholden-Brownet al., GCN 20333) with Zeiss-1000 (East) 1-m telescope of
Tien Shan Astronomical Observatory. We obtained several images in R
filter starting on Dec. 25 (UT) 00:13:31 and Dec. 25 (UT) 23:45:12. We
do not detect any evident variable source in the BAT ground-calculated
position (Ukwatta  al., GCN 20337). Within enhanced XRT position
(Cholden-Brownet al., GCN 20338) we not detected any source. Preliminary
photometry of the field is following

Date       UT start   t-T0   Filter   Exp.   OT   Err.  UL
                       (mid, days)     (s)
2016-12-25 00:13:31   0.10201  R      16*180 n/d n/d   21.1
2016-12-25 23:45:12   1.07646  R      11*180 n/d n/d   20.7

Photometry is based on nearby USNO-B1.0 stars
0719-0341418 17.14
0720-0349085 17.50
0720-0348989 16.94
0719-0341338 15.94

A finding chart can be found in
http://grb.rssi.ru/GRB161224A/GRB161224A_20161225_TSHAO_fc.png
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