it> B. 9603) comprising 6 ks in Photon Counting (PC) mode from T+16. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. Axelsson. Leicester), A. , GCN Circ. 8600,8602). Evans (U. Leicester), A. 528N) in Yunnan Province, China. GCN Circ. Kennea (PSU), B. The analysis of the initial. N. We have analysed 12 ks of XRT data for GRB 150801B (Sbarufatti et al. La Parola (INAF-IASF PA) and W. 0 ks to 196. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: Swift performed a second target of opportunity observation of GRB 110319B on March 23, 2011. (GCN 12067). Sbarufatti (INAF-OAB/IASFPA) and V. it> S. 11813), from 27. C. Cummings (NASA/UMBC) report on behalf of the Swift-XRT team The XRT began observing the field of GRB 090531B (trigger 353728, Cummins, et al. Table 1 - uploaded by Boris Sbarufatti. Gropp (PSU), J. edu> B. edu> B. inaf. GCN Circ. D. Here’s how you knowNASA's Swift satellite detected high-energy X-rays a few degrees from the center of our galaxy, toward the constellation Sagittarius. it> B. 4 ks. N. Marshall (NASA/GSFC), A. it> S. it> B. { "subject": "BAT trigger 778435 is not a GRB. it). , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. Sholtis is the 2021-2022 Reveal Benjamin von Sternenfels Rosenthal Grantee for. In the context of detection of Ultra High Energy Cosmic Ray (UHECR) showers from space the details of fluorescence light production and transmission in the atmosphere are. Leicester), A. We have analyzed 14. 9 ks of XRT data for GRB 101204A (Cummings et al. Holland (CRESST/USRA/GSFC) report on behalf of the Swift XRT team: We have analysed the first two orbits of XRT data of GRB 070529 (Holland et al. Leicester), A. it> V. 0 ks to 196. it>. 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. Y. it> B. GCN Circ. it> B. Boris Sbarufatti at PSU <bxs60@psu. Fynbo (CoI) (ESA Member) University of Copenhagen, Niels Bohr Institute Dr. Cummings (GSFC), M. These. it> B. GCN Circ. The data are entirely in Photon Counting (PC. From: Boris Sbarufatti [v1] Thu, 28 Oct 2004 11:39:10 UTC (112 KB) Full-text links: Access Paper: Download a PDF of the paper titled ESO-VLT optical spectroscopy of BL Lac objects: I. La Parola (INAF-IASF PA) and W. it> B. GCN Circ. Download full-text PDF Read full-text. The data are all in Photon Counting (PC) mode. A. Leicester), A. A. Sbarufatti (INAF-IASFPA), P. A. inaf. 11525), from 339 s to 30. Embed figure. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Cummings (GSFC/UMBC), N. Content may be subject to copyright. We have analyzed 14. Barthelmy (GSFC), P. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. 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). inaf. Cummings 1,3,7,. M. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. Here’s how you knowDOI: 10. 0 ks after the BAT trigger. Beardmore (U Leicester), J. inaf. 17429. The enhanced XRT position was given in Osborne et al. Ralph A. Evans (U. These topic labels come from the works of this person. P. Evans (U. Page (U. it> B. Burrows (PSU), B. 9 ks exposure. Leicester) and K. The observation is in PC mode and consists of 1. We have analyzed 14. A. Of the two unknown sources reported by. 1 ks after the BAT trigger. it> S. it> Sbarufatti B. it> B. Stamatikos (NASA/ORAU) and D. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. We analyzed 3. A. , GCN Circ. P. D. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. GCN Circ. Burrows's 797 research works with 17,426 citations and 9,283 reads, including: Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run///// TITLE: GCN CIRCULAR NUMBER: 26346 SUBJECT: GRB 191130A: Swift-XRT observations DATE: 19/12/05 17:22:42 GMT FROM: Boris Sbarufatti at PSU B. Evans (U. Sbarufatti, V. (GCN 6891) due to the large offset between the initial BAT position and XRT position. Guidorzi (Univ. B. sbarufatti@brera. Mangano, V. ///// TITLE: GCN CIRCULAR NUMBER: 5856 SUBJECT: GRB 061126: Swift/UVOT Afterglow Detection DATE: 06/11/26 09:53:47 GMT FROM: Daniel E. it> B. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. Boris Sbarufatti at INAF-OAB/IASFPA <boris. In the XRT field of view we detect a single faint. La Parola, V. View publication. Mingo (U. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status,” said Dr Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy, who currently is working with other Swift team. Ukwatta (GSFC/GWU) report on behalf of the Swift-XRT team: Swift-XRT began observing the field of GRB 081102 (trigger 333427, Ukwatta et al. Y. La Parola, B. L. Mangano (INAF/IASF PA) and D. Boris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. et al. 11944), from 2. Breeveld, Samantha R. T. October 25, 2023 Source: NASA/Goddard Space Flight Center Summary: A team of scientists has used multiple space and ground-based telescopes to observe an. P. GCN Circ. 10968 ), from 96 s to 25. The spectrum reported by Chavushyan et al. Margutti (INAF-OAB), S. The data are entirely in. inaf. Burst Advocate for this burst is B. it> B. Together they form a unique [email protected]@brera. GCN Circ. 11525), from 339 s to 30. Page (U. GCN Circ. Under the assumption that the host gal-axy luminosity is confined in a narrow range (e. D. , 2006Shaw et al. sbarufatti@brera. Table 1 - uploaded by Boris Sbarufatti. it). Sbarufatti (INAF OAB/IASF PA), V. 16, 2012, resulted from a flood of gas. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. The data comprise 24 s in Windowed Timing (WT) mode with the. Melandri (INAF. N. Here’s how you knowUsing Webb’s spectacular sensitivity, scientists captured the first mid-infrared spectrum from space of a kilonova, which marked Webb’s first direct look at an individual heavy element from such an event. His mother was often. Pascoli, I-06123 Perugia, Italy 2. Mangano (INAF-IASFPA), K. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. P. it> B. sbarufatti AT brera. edu> P. inaf. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. Imaging redshifts of BL Lac ob jects. Sbarufatti 1, A. Boris Sbarufatti; Stefano Ciprini; Jari Kotilainen [. A. 17722). it). Burrows (PSU), J. Page (U. inaf. A. ) has clearly shown that the host galaxies are massive and luminous ellipticals. , GCN [email protected] Sbarufatti at INAF-OAB/IASFPA <[email protected] is concluded that, if the X-ray source is physically associated with the optical-UV transient, then ASASSN-15lh most likely represents the tidal disruption of a main-sequence star by the most massive spinning black hole detected to date. , GCN Circ 7790) on June 3, 14:11 UT, 173 minutes after the trigger. it> B. We report on Swift-XRT observations of GRB 081203B (Copete et al. Boris Sbarufatti, Stefano Ciprini, Jari Kotilainen, Roberto Decarli, Aldo Treves, Angelo Veronesi, Renato Falomo Astronomy & Astrophysics Research output : Contribution to journal › Conference article › peer-reviewA. it> B. An extension of the sample, by B. inaf. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Leicester), C. Sbarufatti (INAF OAB/INAF IASF-PA) , V. McCauley (PSU), J. sbarufatti@brera. GCN Circ. N. 9 ks to T+391. 5 UT, 92. Boris Sbarufatti at INAF-OAB/IASFPA <boris. H. Boris Sbarufatti at INAF-OAB/IASFPA <boris. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. it> B. 2591 [astro-ph. sbarufatti@brera. Aarseth. 4 ks after the BAT trigger. Stroh (PSU), D. 7685) in Window Timing mode, 146 s after the BAT trigger. A. it> B. Please contact the BA by email if you require additional information regarding Swift followup of this burst. inaf. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Amaral-Rogers (U. D. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:32:56 UT, the Swift Burst Alert. Leicester), K. L. K. Mangano (INAF/IASF_PA) and C. 7685) in Window Timing mode, 146 s after the BAT trigger. Chornock, D. In extremely urgent cases, after trying the Burst Advocate, you can contact the. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. Leicester) and P. Sbarufatti, V. The data are entirely in Photon. , GCN circ. , GCN Circ. 11813), from 27. The source has faded with respect to the initial. , & Falomo, R. Rhaana L. 0 seconds after the BAT trigger. Sbarufatti (INAF-OAB/PSU), H. We report on Swift-XRT observations of GRB 081203B (Copete et al. Melandri (INAF-OAB) and B. it> B. M. 6466 ) with total exposure time of 3. Mangano (INAF-IASF Pa) report on behalf of the Swift-XRT team: Swift began observing the field of the Swift BAT Slew Survey (BATSS) GRB 081203B (Copete et al. it> Sbarufatti B. M. inaf. 4-3658}, author={Craig B. H. Please contact the BA by email if you require additional information regarding Swift followup of this burst. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. In the XRT field of view we detect a single faint. B. Tohuvavohu (U. Copy reference. A. Sbarufatti, V. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. (Sbarufatti et al. Strazzeri, O. 3 ks after the BAT trigger. it> D. Copy reference. 22007). An extension of the sample, by B. INFN - Sezione di Milano-Bicocca, Piazza della Scienza 2, Milano (MI), Italy. Sbarufatti (INAF OAB/IASF PA), V. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. GCN 17385 table; GRB_name: GRB150202B: GCN_number: 17385: Detection_method: Fermi LAT Det: t_trigger: 23:59:08. Pagine. Osborne (U. Sbarufatti, V. Evans (U. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. sbarufatti@brera. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. ", "bibcode": "2017GCN. ) is showing up in garmin connect. A. Sbarufatti (INAF-OAB/IASFPA), R. Hagen (PSU) report on behalf of the Swift team Swift performed a follow up observation of GRB 150418A, with a pointing in the direction of Source #1 reported by Sbarufatti et al. B. 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. A. Leicester), P. Gehrels (GSFC), S. La Parola, B. Barun Sobti’s childhood image. Sbarufatti, V. Sbarufatti (PSU), A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. N. Page (U. D. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. We fit the continuum by a power law after correction for the host. 11813 ). Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 13:37:25 UT, the Swift Burst Alert Telescope (BAT) detected a peak in an image at a location near to the known. C. 270 UTC: ra: 86. Sbarufatti (INAF-OAB/IASFPA) and S. Mangano, B. 8600, 8602) 16. Detailed description of the adopted techniques and results are reported in Sbarufatti et al. 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. N. GCN Circ. 6 ks to 14. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. , Mangano V. 10968 ), from 96 s to 25. 6 ks, with a 3. The data are entirely in Photon. it). 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. , GCN Circ. inaf. Evans (U. Page, Silvia Zane, Alice A. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. sbarufatti@brera. 26031), from 3. inaf. GCN Circ. Barthelmy (GSFC), P. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. Barun was a naughty child. Melandri (INAF-OAB), B. McCauley (PSU), J. GCN Circ. . A redshift of z 0. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. III. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. R. 1. inaf. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Osborne (U. R. GCN Circ. Download. E. Kennea (PSU), A. 0 ks after the BAT trigger. 7195. Sbarufatti (PSU) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:02:36 UT, the Swift Burst Alert Telescope (BAT) triggered and. inaf. View publication. et al. D'ai (INAF-IASFPA), [email protected]@brera. it> B. D. Burrows (PSU), J. Mangano (INAF-IASFPA) on behalf of the Swift-XRT [email protected] paper argues that the Cow is a monster black hole shredding a. 1S", "createdOn": 1423508950000, "circularId": 17429, "submitter": "Boris. Melandri (INAF-OAB), D. Racusin, Eleonora. 9 ks exposure. , GCN Circ. Burst Advocate for this burst is B. Y. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: Swift performed a second target of opportunity observation of GRB 110319B on March 23, 2011. A. Barun Sobti consuming alcohol. 17722). P. it> P.