Cummings (GSFC), M. it> B. D. GCN Circ. Sbarufatti (INAF-OAB/IASFPA), J. Leicester), J. B. It is not an astrophysical event. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. Download. Melandri (INAF-OAB), D. GCN Circ. Burst Advocate for this burst is. 2005b). Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. V. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. G. 4 ks after the BAT trigger. B. Beardmore (U. Embed figure. it> B. 7195. View publication. Boris Sbarufatti at INAF-OAB/IASFPA <boris. it). Lien (GSFC/UMBC) and B. J. 4 ks. Sbarufatti (INAF OAB/INAF IASF-PA) , V. Holland1,2,3, Boris Sbarufatti4, Rongfeng Shens, Patricia Schady6, Jay R. it> B. La Parola (INAF-IASF Pa) report on behalf of the Swift-XRT team The XRT began observations of GRB 080605 (trigger=313299, Sbarufatti et al. Page (U. Leicester) report on behalf of the Swift XRT team. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. GCN Circ. , GCN Circ. inaf. H. Cummings1,3,7, Emmanuel Fonseca1,3,8,. (GCN 12067). GCN 22992 table; GRB_name: GRB180720C: GCN_number: 22992: Detection_method: Swift-UVOT Other: Circular_text: TITLE: GCN CIRCULAR NUMBER: 22992 SUBJECT: GRB 180720C: Swift/UVOT Upper Limits DATE: 18/07/21 08:35:26 GMT FROM: Samantha Oates at MSSL S. Sbarufatti et al. sbarufatti@brera. 6 ks to 14. 12335), from 82 s to 7. 0 ks after the BAT trigger. , Mangano V. it> B. 5 minutes. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 08:58:20 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 160123A (trigger=671447). Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 10 ks of XRT data for GRB 100724A (Markwardt et al. Here’s how you knowDOI: 10. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status. Sbarufatti (INAF-OAB/IASFPA), J. Barthelmy (GSFC), P. Raffaella MARGUTTI | Cited by 12,897 | of Harvard-Smithsonian Center for Astrophysics, Cambridge | Read 383 publications | Contact Raffaella MARGUTTIBoris Sbarufatti at INAF-OAB/IASFPA <boris. , Mangano V. Boris Sbarufatti was quoted saying: "The pattern we're seeing is observed in X-ray novae where the central object is a black hole. ESO VLT optical spectroscopy of BL Lac objects. The detection and the measurement of very weak spectral features are difficult to assess because they depend on theThe peak count rate was ~6000 counts/sec (15-350 keV), at ~0 sec after the trigger. Sbarufatti, V. inaf. Burrows (PSU) report on behalf of the Swift XRT team. B. La Parola (INAF-IASF Pa) report on behalf of the Swift-XRT team The Swift XRT began observations of the INTEGRAL burst GRB 080603A (Paizis et al. Methods. Filippenko (UC Berkeley) report that: The Katzman. B. The spectrum reported by Chavushyan et al. it> B. P. P. Mangano, V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. H. The XRT onboard Swift observed the field of GRB 090531A on 2009 June 10 and 2009 June 17, after it came outside the Moon observing contstraint, for a total exposure of 35. An official website of the United States government. Sbarufatti (PSU), P. GCN [email protected] ks in Photon Counting mode. N. Leicester) and D. A. 21822), from 63 s to 924 s after the BAT trigger. Barun was born in a Punjabi Family in Delhi. Name Institution Dr. Sbarufatti (INAF OAB/IASF PA), V. D'Avanzo (INAF-OAB), J. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Download PDF. Palmer (LANL), M. N. INFN - Sezione di Milano-Bicocca,. (INAF-IASFPA), A. Melandri (INAF-OAB), D. 9603) on 2009 July 2 at 14:15 UT, 3. Leicester), A. inaf. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. 11813 ). Mangano (INAF/IASF_PA) and C. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti, V. it> B. (2005b, 2006a, 2009), Paper I, II. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. 9 ks of XRT data for GRB 101204A (Cummings et al. Page (U Leicester), [email protected]. Astronomy & Astrophysics; Research output: Contribution to journal › Article › peer-review. Sbarufatti, V. Download. sbarufatti@brera. sbarufatti AT brera. D'Avanzo (INAF-OAB), A. Evans ([email protected]> S. 10968 ), from 96 s to 25. Credential Certification: Boris Sbarufatti (bxs60@psu. 9 ks to T+391. sbarufatti@brera. Imaging redshifts of BL Lac ob jects. Sbarufatti (INAF-OAB/IASFPA), R. Fynbo (CoI) (ESA Member) University of Copenhagen, Niels Bohr Institute Dr. 270 UTC: ra: 86. inaf. 10998), from 48 s to 39. , GCN Circ. Sbarufatti (INAF-OAB/PSU), P. Sbarufatti, V. 7198). it> S. Krimm (GSFC/USRA), M. An extension of the sample, by B. The XRT onboard Swift observed the field of GRB 090531A on 2009 June 10 and 2009 June 17, after it came outside the Moon observing contstraint, for a total exposure of 35. Barthelmy (GSFC), P. Sbarufatti (boris. inaf. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. sbarufatti@brera. sbarufatti@brera. A. E. D. , GCN Circ. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (boris. The Swift Burst Alert Telescope (BAT) triggered on the high mass X-ray binary IGR J16418-4532 on 2021 September 18 at07:58:20 UT (image trigger 1073821). Holland (GSFC/USRA), H. { "subject": "GRB 150202B: Swift/XRT afterglow confirmation", "bibcode": "2015GCN. 11813 ). inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. GCN Circ. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. La Parola, V. Kennea (PSU), B. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. inaf. Boris Sbarufatti, Martina Barattini. We have analyzed 14. Together they form a unique [email protected]@brera. 9603) on 2009 July 2 at 14:15 UT, 3. Ralph A. GCN Circ. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 10 ks of XRT data for GRB 100724A (Markwardt et al. We analyzed 3. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. D'Avanzo (INAF-OAB), J. 3 ks after the BAT trigger. La Parola (INAF-IASF PA) and W. Swift-XRT performed further observations on the afterglow candidate announced in Sbarufatti et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 7 ks to 35. Omodei et al. GCN 7789 table; GRB_name: GRB080603A: GCN_number: 7789: Detection_method: Other: Circular_text: TITLE: GCN CIRCULAR NUMBER: 7789 SUBJECT: GRB 080603 OA candidate DATE: 08/06/03 12:02:13 GMT FROM: Ryan Chornock at UC Berkeley R. V. Margutti (INAF-OAB), S. The observation is in PC mode and consists of 1. The data are entirely in Photon. Lien (GSFC/UMBC), A. Pagani (U. Barun Sobti consuming alcohol. (GCN Circ. A. D'Avanzo (INAF-OAB), J. (GCN Circ. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. Sbarufatti (INAF-OAB/IASFPA), S. inaf. N. GCN Circ. 1K", "createdOn": 1598983743000, "circularId": 28341, "submitter": "Boris. GCN Circ. The data are entirely in. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. B. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. Leicester), K. We analyzed 3. 2591 [astro-ph. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. A. A. inaf. inaf. Kennea (PSU), A. La Parola (INAF-IASF Pa) report on behalf of the Swift-XRT team The XRT began observations of GRB 080605 (trigger=313299, Sbarufatti et al. Sbarufatti, V. (Feb 11, 2013) Published in: Astron. Sbarufatti (INAF-OAB/PSU), M. inaf. 0 ks after the BAT trigger. D'ai (INAF-IASFPA), [email protected]@brera. Tohuvavohu (U. 17722). : New ESO VLT spectroscopy of BL Lacertae objects Fig. Leicester), A. The data are entirely in [email protected]. There will be no XRT or UVOT data until this time. Maselli (INAF-IASFPA), A. P. T. The refined position for the afterglow, obtained using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue (see. Semantic Scholar extracted view of "GRB 150527A: Swift-XRT refined Analysis. The best position for the X-ray afterglow is the XRT. Boris Sbarufatti (CoI) (ESA Member) Dr. 13 UT on 2023-08-21, is due to misidentification of a known source during a Star Tracker Loss-of-Lock. 6466 ) with total exposure time of 3. 12335), from 82 s to 7. Leicester), J. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 08:02:13 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRS 1716-249/GRO J1719-24/V2293 Oph (trigger=731535). Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the MAXI-detected burst. Y. The data comprise 8 s in Windowed Timing (WT) mode while Swift was slewing to the burst, 270 s in PC mode, a further 185 s in WT mode during a bright flare starting at T0+366 s (also seen in the BAT), with the. gamma radiation Earth & Environmental Sciences 81%. Osborne (U. sbarufatti@brera. 3 ks after the BAT trigger. Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio (CoI) (ESA Member) Observatoire de Paris Prof. V. g. 3 ks after the BAT trigger. De Pasquale (MSSL) report on behalf of the Swift Team. A. Boris Sbarufatti at INAF-IASF-Pa <[email protected] AT brera. The data are entirely in Photon Counting (PC) mode. sbarufatti AT brera. Boris Sbarufatti at PSU <bxs60@psu. LaPorte (PSU) report on behalf of the. Malesani (DARK/NBI) report on behalf of the Swift team A second epoch of observations on the ground discovered GRB 150204A (Cummings, GCN 17404 ) was performed by Swift from T+378. Sbarufatti (INAF-OAB/PSU), L. 1. Stroh (PSU), D. Sbarufatti (INAF-OAB/PSU), A. 2 ks to 383. 10983), from 68 s to 58. 17429. Lien (GSFC/UMBC) and B. Sbarufatti (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. 5. Mangano (INAF IASF-PA), B. , 2006Shaw et al. Osborne (U. A. We obtained James Webb Space Telescope mid-infrared (mid-IR) imaging and spectroscopy 29 and 61 days after. 4 ks after the BAT trigger. We use the 80cm telescope of CHanging Event Survey at the YaoAn observation station(101. inaf. B. inaf. inaf. A. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. 1 Similar Profiles; gamma ray bursts Physics & Astronomy 100%. Crossref. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. Kuin (UCL-MSSL), S. Barthelmy (GSFC), P. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. L. 10968 ), from 96 s to 25. GCN Circ. Osborne (U. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. inaf. inaf. Lien (GSFC/UMBC), A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti@brera. Sbarufatti, V. D. Gropp (PSU), J. Burst Advocate for this burst is B. Our earliest-time LRIS images do not cover the position of the X-ray source reported by Sbarufatti et al. Leicester), K. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. P. Evans (U. Due to an observing constraint, Swift will not slew until T0+49. D. inaf. 1 arcsec away from the first XRT position given in Sbarufatti & Mangano (GCN Circ. We show that GRB 230307A belongs to the class of long-duration gamma-ray bursts associated with compact object mergers 4-6, and contains a kilonova similar to AT2017gfo, associated with the gravitational-wave merger GW170817 7-12. DOI: 10. La Parola (INAF-IASF Pa), T. 2002) and the possible host galaxy of GRB 090417B. GCN [email protected]@brera. Sbarufatti (INAF-OAB/PSU), P. Johan P. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. 1000° Circular_text: TITLE: GCN CIRCULAR NUMBER: 17385 SUBJECT: GRB 150202B: Fermi-LAT detection DATE: 15/02/03 08:25:40 GMT FROM: Magnus Axelsson at Stockholm U. Page (U. it> B. Mangano (INAF/IASF Pa) report on behalf of the Swift XRT team Swift XRT began observations of GRB 080710 (Sbarufatti et al. Burst Advocate for this burst is B. TITLE: GCN CIRCULAR NUMBER: 28307 SUBJECT: GRB 200829A: Swift detection of a burst with an optical afterglow DATE: 20/08/29 14:18:33 GMT FROM: Boris Sbarufatti at PSU M. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Melandri (INAF-OAB), B. In extremely urgent cases, after trying the Burst Advocate,. Amaral-Rogers (U. Melandri (INAF-OAB), K. . The enhanced XRT position was given in Osborne et al. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. it> B. Mangano, B. Leicester), V. 6 ks to 14. 6 ks in. Palmer (LANL) report on behalf of the Swift-XRT team: We have analysed 6. Cummings (GSFC), M. Dive into the research topics where Boris Sbarufatti is active. Evans ([email protected] ks of XRT data for GRB 110106B (Sbarufatti et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Holland (GSFC/USRA), H. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. L. N. (GCN Circ. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Fermi/LAT-detected burst. inaf. Sbarufatti (INAF-OAB/IASFPA), J. Barthelmy (GSFC) report on behalf of the Swift team: UVOT took a finding chart exposure of 100. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. Find Boris Sbarufatti's email address, contact information, LinkedIn, Twitter, other social media and more. 6560 ), consisting of 150 s in Window Timing. Swift immediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. inaf. Sbarufatti, V. B. inaf. The Neil–Gehrels Swift Observatory has added extensively to our understanding of small bodies in our solar system through its capabilities to rapidly respond to short-live events such as outbursts and collisions, through its near-ultraviolet coverage, and by its ability to track time-dependent changes through monitoring campaigns. it> B. 8 ks after the BAT trigger. Sbarufatti (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. Kennea (PSU), B. Cummings (GSFC), M. D. H. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 10979), from 82 s to [email protected]. 1 ks after the BAT trigger. GCN Circ. L. We report on Swift XRT observations of the field of the Fermi-LAT discovered GRB 170424A (N.