Boris Sbarufatti at PSU <[email protected] Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. C. Sbarufatti (INAF-OAB/PSU), J. Page (U. 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. 11440), from 126. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks after the BAT trigger. 17385, Hurley et al. edu> P. 5 edit Updated on Nov 18, 2022 Research works(15) Cited By Date of paper 2004 2023 Number of authors 10 authors or less 8. Sbarufatti 1, A. 2 ks of XRT data for GRB 130518B (Cummings GCN Circ. Leicester), C. Pagani (U. Leicester), P. We use the 80cm telescope of CHanging Event Survey at the YaoAn observation station(101. Boris Sbarufatti at INAF-OAB/IASFPA <boris. . 9 days) (Cummings, GCN Circ. There will be no XRT or UVOT data until this time. Leicester), A. H. 10983), from 68 s to 58. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 4 ks after the BAT trigger. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Boris Sbarufatti at INAF-OAB/IASFPA <boris. R. derived absolute magnitudes of the host galaxies are consistent with the distribution of M R of BL Lac hosts given. Mangano (INAF-IASF PA) on behalf of the Swift XRT team Swift XRT started a ToO observation of the INTEGRAL burst GRB080120 at 19:47 UT. B. Page (U. La Parola (INAF-IASFPA), S. T reves. Kennea (PSU), A. 11813 ). 0 seconds after the BAT trigger. Sbarufatti (INAF-OAB/IASFPA) and S. Boris Sbarufatti at INAF-OAB/IASFPA <boris. D. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. J. Krimm (GSFC/USRA), M. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Maselli (INAF-IASFPA), A. Overview; Fingerprint; Abstract. We have analysed 12 ks of XRT data for GRB 150801B (Sbarufatti et al. Sbarufatti (INAF-OAB/PSU) and M. Melandri (INAF-OAB) and B. 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. it). View publication. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. T. it> B. Krimm (GSFC/USRA), M. Roma-BZCA T blazars in the P alermo BA T Survey B. it> B. Sbarufatti (PSU) report on behalf of. A. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. it). Boris Sbarufatti at INAF-OAB/IASFPA <boris. 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. Boris Sbarufatti at INAF-OAB/IASFPA <boris. B. 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. 1086/519450 Corpus ID: 14317593; Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine @article{Troja2007SwiftOO, title={Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine}, author={Eleonora Troja and Gaspare. D. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti@brera. 3 ks of XRT data for GRB 110915A (Holland et al. 2 ks and T+516. it>. inaf. D'Avanzo (INAF-OAB), J. Cummings (GSFC), M. sbarufatti@brera. it> Via. The data are entirely in. Barthelmy (GSFC), P. D'Avanzo (INAF-OAB), J. Boris Sbarufatti; Stefano Ciprini; Jari Kotilainen [. sbarufatti AT brera. Kennea (PSU), A. Gianpiero Tagliaferri, Ruben Salvaterra, Sergio Campana, Stefano Covino, Paolo D'Avanzo, Dino Fugazza, Giancarlo Ghirlanda, Gabriele Ghisellini, Andrea Melandri, Lara. We have analyzed 14. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. The outburst, produced by a rare X-ray nova, announced the presence of a previously unknown stellar-mass black hole. inaf. P. Lien (GSFC/UMBC) and S. R. 1S", "createdOn": 1423508950000, "circularId": 17429, "submitter": "Boris. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. sbarufatti@brera. Sbarufatti (PSU), K. L. 29529). The data are entirely in Photon Counting (PC. 8 ks after the BAT trigger. Margutti (INAF-OAB), S. 3 ks after the BAT trigger. 5 @inproceedings{Pasquale2017GRB1R, title={GRB 130831A: Rise and demise of a magnetar at z = 0. E. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. Cummings (GSFC), M. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Margutti (INAF-OAB), S. 11944), from 2. Leicester) and P. C. Sbarufatti (INAF-OAB/PSU), H. Find Boris Sbarufatti's email address, contact information, LinkedIn, Twitter, other social media and more. 11440), from 126. Sbarufatti, V. Leicester), J. Raised by her mother, Sara and her. Dr. The authors thank Andres Escala, Lucio Mayer, Ruben Salvaterra, Javier Sanchez, Boris Sbarufatti and Alberto Sesana for fruitful comments and suggestions, and Franz Livio and Luca Paredi for technical support. Leicester), J. D'Avanzo (INAF-OAB), A. A. The source has faded with respect to the initial. We report the observations for the GRB191122A (B. Lien (GSFC/UMBC), A. 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. Margutti (INAF-OAB), S. it> V. Authors: L Rhodes, M Caleb, BW Stappers, A Andersson, MC Bezuidenhout, LN Driessen, I Heywood. 11525), from 339 s to 30. A. In this framework, initially proposed to explain GRBs with precursor activity, the prompt emission is produced by accretion of matter onto a newly–born magnetar, and. GCN Circ. et al. 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. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester) and P. Authors: Marco Landoni, Renato Falomo, Aldo Treves, Boris Sbarufatti. inaf. N. { "subject": "GRB 200901A: Swift-XRT refined Analysis", "bibcode": "2020GCN. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status," said Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy, who currently is working. edu> B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti Research Astronomer at INAF 1y Report this post Day 2 of the "Astrophysical Polarimetry in the Time-Domain Era" conference in Lecco. Sbarufatti (INAF-OAB/IASFPA), S. , GCN Circ. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks, with a 3. Sbarufatti (INAF-OAB/IASFPA), V. Perugia Section, Via A. GCN Circ. Siegel (PSU) report on behalf of the Swift-XRT team: We have analysed 15 ks of XRT data for GRB. Mangano, B. Melandri (INAF-OAB), J. Sbarufatti (INAF-OAB/IASFPA), J. Content may be subject to copyright. A. Leicester), V. Fogli freschi d'inchiostro; Dita D'Inchiostro's Club; Passato; Mappe d'InchiostroJ. D'Elia (ASDC), N. Evans (U. Hello, today I imported a . Fig 1 - uploaded by Boris Sbarufatti. L. Download. inaf. inaf. Aarseth. (2008). L. Here’s how you knowA. 5}, author={Massimiliano de Pasquale and M. L. 345 was measured for. Burrows (PSU), [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Y. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks in Photon Counting mode. inaf. Sbarufatti, V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. 5 ks of XRT data for GRB 100117A (De Pasquale et al. We report on Swift XRT observations of the field of the Fermi-LAT discovered GRB 170424A (N. 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). III. Osborne (U. 6 ks, with a 3. Due to an observing constraint, Swift will not slew until T0+49. Y. We fit the continuum by a power law after correction for the host. 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. Osborne (U. 8462) at 17:46:11. 1 ks. Sbarufatti (INAF OAB/IASF PA), V. The spectrum reported by Chavushyan et al. 11813 ). Barun Sobti’s childhood image. D'Ai (INAF-IASFPA), D. Leicester) and M. 9905). Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. Evans (U. A. it> B. Burrows (PSU), J. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. Melandri (INAF-OAB), V. GCN Circ. 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. Sbarufatti (INAF OAB/INAF IASF-PA) and C. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. GCN Circ. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. McCauley (PSU), J. (Feb 11, 2013) Published in: Astron. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 05:00 UT on 2011 April 11. GCN [email protected] ks in Photon Counting mode. Sbarufatti (INAF-OAB/IASFPA), R. Lien. D. it> B. Sbarufatti, V. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. Evans (U. Boris Sbarufatti at PSU <bxs60@psu. A. inaf. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the MAXI-detected burst. D. Barthelmy (GSFC), J. Dive into the research topics where Boris Sbarufatti is active. Detailed description of the adopted techniques and results are reported in Sbarufatti et al. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Barthelmy (GSFC), P. 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. The data are all in Photon Counting (PC) mode. Evans (U. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status,” said Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy,. N. These. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. . Evans (U. 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. Beardmore (U. , GCN Circ. Sbarufatti, V. , GCN Circ 26269). it> B. De Pasquale (MSSL) report on behalf of the Swift Team. 7685) in Window Timing mode, 146 s after the BAT trigger. it> B. Mangano (INAF-IASFPA), K. Sbarufatti (INAF-OAB/IASFPA) and S. 10998), from 48 s to 39. it> Sbarufatti B. Mangano (INAF IASF-PA), B. : New ESO VLT spectroscopy of BL Lacertae objects Fig. de Pasquale (INAF-IASFPA), A. D'ai (INAF-IASFPA), A. , GCN Circ. , GCN circ. it> S. Fariborz Besarati (born 23 August 1966) is a Swedish former wrestler who competed in the 1992 Summer Olympics and in the 1996 Summer Olympics. A. D. 2 ks of XRT data for GRB 110106B (Sbarufatti et [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Roegiers (PSU), L. Mangano (INAF/IASF PA) and D. Imaging redshifts of BL Lac ob jects. So exactly what is the Cow? Using data from multiple NASA missions, including the Neil Gehrels Swift Observatory and the Nuclear Spectroscopic Telescope Array (NuSTAR), two groups are publishing papers that provide possible explanations for the Cow’s origins. sbarufatti AT brera. it Stefano Ciprini 1. Cummings (GSFC), M. Sbarufatti (INAF/OAB-IASF Pa) reports on behalf of the Swift-XRT team: We have analysed 24 ks of XRT data for GRB 101204A (Cummings et al. Oates. Sbarufatti et al. inaf. Swift immediately slewed to the target. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:32:56 UT, the Swift Burst Alert. et al. { "subject": "GRB 130725B - UVOT-enhanced XRT position", "bibcode": "2013GCN. P. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. Sbarufatti (INAF-OAB/IASFPA), R. Barthelmy (GSFC), J. 21822), from 63 s to 924 s after the BAT trigger. inaf. The data comprise 177 s in Windowed Timing (WT). Sbarufatti (INAF-OAB/IASFPA), J. 6 ks in. R. M. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Mangano (INAF/IASF_PA) and C. GCN Circ. P. inaf. edu) Subjects: X-ray, Neutron Star, Transient. La Parola, B. 11944), from 2. Leicester), A. it> V. it> B. Kennea (PSU), B. Page and Silvia Zane and A. B. Leicester), J. Melandri (INAF-OAB), K. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Kennea (PSU), A. 10979), from 82 s to [email protected]. 2 ks of XRT data for GRB 130518B (Cummings GCN Circ. B. Mangano (INAF-IASFPA) and J. GCN Circ. Barthelmy (GSFC), P. A. Leicester), M. Breeveld, Samantha R. Sbarufatti (INAF-OAB/IASFPA), V. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. inaf. afterglows. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. E. it> B. We have analyzed 14. error circle (Sbarufatti et al. , GCN Circ 7790) on June 3, 14:11 UT, 173 minutes after the trigger. " Reply replyAstronomers have spotted a rare X-ray star explosion near the center of our Milky Way galaxy, revealing a previously unknown black hole munching on gas from a neighboring sun-like star. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. Mangano (INAF-IASF PA) and D. Perugia Section, Via A. LaPorte (PSU) report on behalf of the. J. 4 ks after the BAT trigger. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. A. Content may be subject to copyright. inaf. 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.