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« : 11 Декабрь 2010, 11:53:39 » |
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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=50Там 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. 
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Виктор Воропаев
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« Ответ #391 : 16 Май 2019, 08:35:25 » |
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TITLE: GCN CIRCULAR NUMBER: 24556 SUBJECT: GRB 190515A: Kitab Observatory optical upper limit DATE: 19/05/15 18:43:38 GMT FROM: Alexei Pozanenko at IKI, Moscow
S. Belkin (IKI), A. Novichonok (KIAM), A. Pozanenko (IKI), E. Mazaeva (IKI), A. Volnova (IKI), I. Molotov (KIAM) report on behalf of larger IKI GRB FuN collaboration:
We observed the field of the Swift GRB 190515A (Moss et al., GCN 24553) with RC-36 0.36-m telescope of Kitab Observatory starting on May 15 (UT) 16:13:02 in Clear filter. We do not find any optical source neither in the first image, nor in a stacked image within prompt enhanced Swift-XRT position (Evans et al., GCN 24554). Preliminary photometry of the field is following.
Date UT start t-T0 Filter Exp. OT Err. UL(3sigma) (mid, days) (s)
2019-05-15 16:13:02 0.00655 CR 1*90 n/d n/d 18.6 2019-05-15 16:13:02 0.02686 CR 40*90 n/d n/d 20.3
The photometry is based on the nearby USNO-B1 (R2) star: USNO-B1.0_id R2 1422-0205150 15.02
The closest object which is not presented in any catalogs marginally detected in our stacked image has coordinates (J2000) 06:35:24.07 +52:19:12.4 with uncertainty of 1 arcsec in both coordinates and brightness of 20.4m (S/N =2). The position of the object is 12 arcsec apart from the the center of prompt enhanced Swift-XRT position (Evans et al., GCN 24554). At this time we cannot say about variability of the object.
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Виктор Воропаев
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« Ответ #392 : 02 Июнь 2019, 16:07:22 » |
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TITLE: GCN CIRCULAR NUMBER: 24712 SUBJECT: GRB 190530A: Mondy and AbAO optical observations DATE: 19/06/02 09:53:20 GMT FROM: Alexei Pozanenko at IKI, Moscow
S. Belkin (IKI), E. Klunko (ISTP), R. Ya. Inasaridze (AbAO), A. Pozanenko (IKI), V.R. Ayvazian (AbAO), E. Mazaeva (IKI), A. Volnova (IKI) report on behalf of IKI GRB FuN collaboration:
We continue observations the optical afterglow (Lipunov et al., GCN 24680, 24693 and also e.g. Kann et al., GCN 24684; Melandri et al., GCN 24689; Heintz et al., GCN 24686; Lzzo et al., GCN 24687; Xin et al., GCN 24688; Watson et al., GCN 24690; Xin et al., GCN 24697) of the Fermi GRB 190530A (Fermi GBM Team, GCN 24676; Longo et al., GCN 24679) with AZT-33IK telescope of Sayan observatory (Mondy) and AS-32 (0.7m) telescope of Abastumani Observatory. The afterglow is clearly visible in stacked images. Preliminary photometry of the afterglow is following.
Date UT start t-T0 Filter Exp. OT Err. UL (mid, days) (s)
2019-06-01 15:35:00 2.23638 R 29*60 19.62 0.07 21.2 2019-06-01 17:38:57 2.31769 R 30*60 19.70 0.14 20.6
The photometry is based on the nearby USNO-B1.0 stars
USNO-B1.0_id R2 1255-0157926 13.35 1254-0159410 12.63 1255-0157793 13.56
The photometry might be influenced by nearby optical source presented in Pan-STARRS DR1 catalog (ID 150571205309266249) mentioned in (Lipunov et al., GCN 24680).
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Виктор Воропаев
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« Ответ #393 : 06 Июнь 2019, 00:34:10 » |
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TITLE: GCN CIRCULAR NUMBER: 24754 SUBJECT: GRB 190604B: Kitab observatory optical upper limit DATE: 19/06/05 19:24:37 GMT FROM: Alexei Pozanenko at IKI, Moscow
S. Belkin (IKI), A. Novichonok (KIAM), A. Pozanenko (IKI), E. Mazaeva (IKI), A. Volnova (IKI), I. Molotov (KIAM), Sh. Ehgamberdiev (UBAI) report on behalf of larger IKI GRB FuN collaboration:
We observed the field of the Swift GRB 190604B (Page et al., GCN 24742) with RC-36 0.36-m telescope of Kitab Observatory starting on June 04 (UT) 22:26:32 in Clear filter. We do not find any optical source within enhanced Swift-XRT position (Evans et al., GCN 24746). The non-detection is consistent with BOOTES-3 results (Hu et al., GCN 24750).
Preliminary photometry of the field is following.
Date UT start t-T0 Filter Exp. OT Err. UL(3sigma) (mid, days) (s)
2019-06-04 22:26:32 0.32068 CR 21*60 n/d n/d 18.6
The photometry is based on the nearby USNO-B1 (R2) stars.
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« Ответ #394 : 15 Июнь 2019, 12:48:31 » |
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TITLE: GCN CIRCULAR NUMBER: 24838 SUBJECT: GRB 1906013A: Kitab and AbAO optical upper limit DATE: 19/06/15 09:38:38 GMT FROM: Alexei Pozanenko at IKI, Moscow
S. Belkin (IKI), A. Novichonok (KIAM), A. Zhornichenko (KIAM), R. Ya. Inasaridze (AbAO), V.R. Ayvazian (AbAO), A. Pozanenko (IKI), E. Mazaeva (IKI), A. Volnova (IKI), I. Molotov (KIAM), Sh. Ehgamberdiev (UBAI) report on behalf of larger IKI GRB FuN collaboration:
We observed the field of the GRB 190613A (Ambrosi et al., GCN 24798) with RC-36 telescope of Kitab Observatory and AS-32 of Abastumani observatory . We do not detect the optical afterglow (Ambrosi et al., GCN 24798; Zheng et al., GCN 24801; Lipunov et al., GCN 24803). Preliminary photometry of the field is following.
Date UT start t-T0 Filter Exp. OT Err. UL(3sigma) Telescope (mid, days) (s)
2019-06-13 16:26:41 0.54575 CR 5500 n/d n/d 20.6 RC-36 2019-06-13 21:33:40 0.73706 R 1800 n/d n/d 21.0 AS-32
The photometry is based on the nearby USNO-B1 (R2) stars USNO-B1.0_id R2 1572-0165015 13.62 1572-0164999 14.91 1572-0164916 14.28
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Виктор Воропаев
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« Ответ #395 : 16 Июнь 2019, 17:15:43 » |
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TITLE: GCN CIRCULAR NUMBER: 24841 SUBJECT: GRB 190613B: Kitab observatory optical upper limit DATE: 19/06/16 14:10:05 GMT FROM: Alexei Pozanenko at IKI, Moscow
S. Belkin (IKI), A. Novichonok (KIAM), A. Zhornichenko (KIAM), A. Pozanenko (IKI), E. Mazaeva (IKI), A. Volnova (IKI), I. Molotov (KIAM), Sh. Ehgamberdiev (UBAI) report on behalf of larger GRB IKI FuN collaboration:
We observed the field of the GRB 190613B (D'Aiet al., GCN 24807) with RC-36 0.36-m telescope of Kitab Observatory starting on June 13 (UT) 22:26:32 in Clear filter. We do not detect the optical afterglow (D'Aiet al., GCN 24807; Marshall al., GCN 24817; Zheng al., GCN 24818; Ugarte Postigo al., GCN 24825; Hu al., GCN 24826). Preliminary photometry of the field is following.
Date UT start t-T0 Filter Exp. OT Err. UL(3sigma) (mid, days) (s)
2019-06-13 20:55:3 0.43001 CR 3600 n/d n/d 20.0
The photometry is based on the nearby USNO-B1 (R2) stars.
USNO-B1.0_id R2 0853-0556521 16.14 0853-0556781 16.31
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Виктор Воропаев
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« Ответ #396 : 01 Июль 2019, 23:54:02 » |
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TITLE: GCN CIRCULAR NUMBER: 24947 SUBJECT: GRB 190630C: ISON-Castelgrande optical upper limit DATE: 19/07/01 20:07:58 GMT FROM: Alexei Pozanenko at IKI, Moscow
S. Belkin (IKI), S. Schmalz (KIAM), A. Pozanenko (IKI), A. Volnova (IKI), E. Mazaeva (IKI), I. Molotov (KIAM) report on behalf of larger GRB IKI FuN collaboration:
We observed the field of GRB 190630C (Ukwatta et al., GCN 24927) with ORI-22 (22 cm) telescope of ISON-Castelgrande observatory in Clear filter starting on July 01 (UT) 00:03:42. We do not detect any object within enhanced Swift-XRT position (Goad et al., GCN 24930). Preliminary photometry of the field is following
Date UT start t-T0 Filter Exp. OT Err. UL (mid, days) (s)
2019-07-01 00:03:42 0.02584 CR 53*60 n/d n/d 18.8
The photometry is based on nearby USNO-B1.0 (R2) stars.
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Виктор Воропаев
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« Ответ #397 : 09 Сентябрь 2019, 10:45:37 » |
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TITLE: GCN CIRCULAR NUMBER: 25683 SUBJECT: ZTF19abvizsw: AbAO and CrAO photometry DATE: 19/09/07 14:05:41 GMT FROM: Alexei Pozanenko at IKI, Moscow
S. Belkin (IKI), A. Pozanenko (IKI), R. Ya. Inasaridze (AbAO), V. Rumyantsev (CrAO), A. Volnova (IKI), E. Mazaeva (IKI), I. Molotov (KIAM) report on behalf of IKI GRB FuN collaboration:
We observed the ZTF19abvizsw/AT2019pim (Kool et al., GCN 25616; Burdge et al., GCN 25639; Wei et al., GCN 15640; Perley et al., GCN 25643; Levan et al., GCN 25653; Becerra et al., GCN 25655;) with AS-32 (0.7m) telescope of Abastumani Observatory and ZTSh telescope of CrAO. Preliminary photometry of the the optical transients is following.
date UT start MJD Filter Exp. OT OT_err Obs./Tel. (mid, d) (s)
2019-09-04 16:54:07 58730.723 R 54*60 21.27 0.16 AbAO/AS-32 2019-09-05 21:49:03 58731.923 R 20*120 21.33 0.14 CrAO/ZTSh
The photometry of the latest epoch of 2019-09-05 might be slightly contaminated by red southward star (see also Burdge et al., GCN 25639). We note the flattening of the initial decay previously reported by Becerra (GCN 25655).
The photometry is based on nearby USNO-B1.0 stars USNO-B1.0_id R2 1514-0239703 18.81 1514-0239806 19.68
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