Sbarufatti (INAF-OAB/IASFPA), R. Kennea (PSU), A. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Melandri (INAF-OAB), K. Ralph A. 6 ks in. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. 8600,8602). 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. 7 ks to 35. A. 22010. Mangano (INAF-IASFPA), report on behalf of the Swift- XRT team: Swift began observation of the XRF detected by INTEGRAL (Paizis, et al. Sbarufatti (INAF-OAB/PSU), P. it> Via. T. Please contact the BA by email if you require additional information regarding Swift followup of this burst. View publication. Copy caption. The enhanced XRT position was given in Osborne et al. 6560 ), consisting of 150 s in Window Timing. it> B. it). Kuin (UCL-MSSL), S Laha (GSFC/UMBC/CRESST) and A. inaf. The best position for the X-ray afterglow is the XRT. 9 ks after the Swift/BAT trigger. inaf. N. We have analyzed 14. 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. 2005 Sbarufatti et al. D'Avanzo (INAF-OAB), J. Mangano (INAF IASF-Pa), C. H. Sbarufatti (INAF OAB/IASF PA), V. Content may be subject to copyright. Sbarufatti (INAF OAB/INAF IASF-PA) and C. Page (U. 4-3658}, author={Craig B. La Parola (INAF-IASF PA) and W. L. 528N) in Yunnan Province, China. (INAF-IASFPA) report on behalf of the Swift Team: We have analysed the first six orbits of Swift-XRT data obtained from GRB 090417B (trigger 349450; Sbarufatti, et al. We derive here the intrinsic absorbing X–ray column densities of these GRBs making use of the Swift X–ray Telescope data. T. D'Avanzo (INAF-OAB), A. Cummings (GSFC), M. 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. B. GCN Circ. Burrows (PSU), J. Swift immediately slewed to the target. 1S", "createdOn": 1374845329000, "circularId": 15038, "submitter": "Boris. 10998), from 48 s to 39. Boris Sbarufatti at INAF-OAB/IASFPA <boris. De Pasquale (MSSL) report on behalf of the Swift Team. 4 ks after the BAT trigger. 5. Sbarufatti (PSU), P. Margutti (INAF-OAB), S. L. . 11813), from 27. D'Avanzo (INAF-OAB), J. Burrows (PSU), J. Barthelmy (GSFC), T. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. Leicester), J. 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). Cummings (GSFC), M. 7 ks after the trigger. 8 ks after the BAT trigger. The source has faded with respect to the initial. 29529). N. 6 ks to 14. inaf. We analyzed 3. inaf. Mangano (INAF-IASFPA) on behalf of the Swift-XRT [email protected] paper argues that the Cow is a monster black hole shredding a. P. Gehrels (GSFC), S. (Sbarufatti et al. K. 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. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. Barthelmy (GSFC), P. 7687). Nial Rahil Tanvir (CoI) (ESA Member) Prof. 7 ks after the BAT trigger. 14862), from 184. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. 29529). (INAF-IASFPA), A. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. A. INFN - Sezione di Milano-Bicocca, Piazza della Scienza 2, Milano (MI), Italy. C. , GCN circ. La Parola, [email protected]° decl: 59. Page (U. GCN Circ. H. The analysis of the initial. sbarufatti@brera. Osborne (U. The data are entirely in. Mangano (INAF IASF-PA), B. J. sbarufatti@brera. inaf. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. it>. There will thus be no XRT or UVOT data for this trigger before this time. Download full-text PDF Read full-text. We report on Swift-XRT observations of GRB 081203B (Copete et al. G. Cummings (GSFC/UMBC), N. , GCN circ. (GCN 12067). Burrows, report on behalf of the Swift XRT team: We have analyzed the first 3 orbits of Swift-XRT data obtained for GRB 061126 (trigger=240766, GCN 5854). 5. Roegiers (PSU), L. GCN Circ. Table 3 - uploaded by Boris Sbarufatti. The data are entirely in. Due to an observing constraint, Swift will not slew until T0+49. Evans (U. De Pasquale (MSSL) report on behalf of the Swift Team. P. edu> B. , GCN Circ. inaf. A. Boris Sbarufatti Osservatorio astronomico di Brera: Milano, Lombardia, IT 2011-10-01 to 2017-07-31 | Post-Doc Employment Show more detail Source : Boris. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. it> B. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Copy caption. Sbarufatti, V. 1 ks. 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. The data are entirely in Photon Counting (PC. : New ESO VLT spectroscopy of BL Lacertae objects Fig. Kennea (PSU), B. Sbarufatti, V. B. it> B. edu> B. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 05:00 UT on 2011 April 11. 1 ks after the BAT trigger. Markwardt and Span and David M. it> B. P. Sbarufatti (INAF IASF-Pa), V. it> S. Sbarufatti (INAF-OAB/PSU), H. , GCN Circ. inaf. GCN Circ. B. Evans (U. GCN 17385 table; GRB_name: GRB150202B: GCN_number: 17385: Detection_method: Fermi LAT Det: t_trigger: 23:59:08. We report the observations for the GRB191122A (B. inaf. H. We analyzed 3. 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. 2 ks to 383. inaf. News; Events; Alumni; Faculty and Staff DirectoryTITLE: GCN CIRCULAR NUMBER: 28859 SUBJECT: GRB 201104A: Swift-XRT observations DATE: 20/11/06 17:46:49 GMT FROM: Boris Sbarufatti at PSU V. ] Renato Falomo; We present results of an ongoing program at the ESO VLT for spectroscopy of BL Lac objects lacking a firm redshift estimate. A. Sbarufatti (INAF-OAB/IASFPA), V. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. 11813 ). Page (U. 2 ks of XRT data for GRB 130725B (Swenson et al. Sbarufatti (INAF-OAB/IASFPA), J. We report on Swift-XRT observations of GRB 081203B (Copete et al. Beardmore (U Leicester), J. Evans ([email protected]> S. D. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. 15029), from 53 s to 35. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. These topic labels come from the works of this person. inaf. E. inaf. sbarufatti@brera. Amaral-Rogers (U. 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. T. 11944), from 2. GCN Circ. Barthelmy (GSFC), P. Lien (GSFC/UMBC) and B. it> B. Embed figure. 4 ks after the BAT trigger. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. D'Avanzo (INAF-OAB), J. edu> B. [email protected] ks of exposure we don t detect. The data comprise 24 s in Windowed Timing (WT) mode with the. inaf. L. Sbarufatti (INAF-OAB) report on behalf of the Neil Gehrels Swift Observatory Team: Swift BAT trigger 1186391 at 15:25:12. Leicester) and P. From: Boris Sbarufatti [v1] Mon, 20 Oct 2008 14:06:52 UTC (133 KB) Full-text links: Download: Download a PDF of the paper titled ESO VLT optical spectroscopy of BL Lacertae objects. it> P. Sbarufatti (INAF-IASFPA), and S. Swiftimmediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. 1811E, 25. inaf. Maselli (INAF-IASFPA), A. (2008) 1 . Mangano (INAF IASF-PA), B. M. An official website of the United States government. (2005), we estimate a redshift z = 0. Download. An extension of the sample, by B. R. 10983), from 68 s to 58. it> B. Aptekar, D. Malesani (DARK/NBI), S. A. P. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. De Pasquale (MSSL) report on behalf of the Swift Team. De Pasquale (UCL-MSSL) report on behalf of the Swift-XRT team: We have analysed 5. Melandri (INAF-OAB), B. Content may be subject to copyright. Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio (CoI) (ESA Member) Observatoire de Paris Prof. inaf. La Parola (INAF-IASF PA) and W. This image from Webb’s NIRCam (Near-Infrared Camera) instrument highlights GRB 230307A’s kilonova and its former home galaxy. A. Sbarufatti (INAF-IASFPA), P. Sbarufatti, V. A. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. inaf. A. 4 ks after the BAT trigger. Siegel (PSU) report on behalf of the Swift team: Examination of the full BAT data set for Swift trigger 629693 (Siegel et al. Y. D'Avanzo (INAF-OAB) and P. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. gamma radiation Earth & Environmental Sciences 81%. Sbarufatti, V. Cancel;"The pattern we're seeing is observed in X-ray novae where the central object is a black hole," said Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy, currently working. . C. 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> Sbarufatti B. sbarufatti@brera. Vanden Berk at PSU/Swift D. sbarufatti@brera. Y. GCN Circ. Boris Sbarufatti at INAF-IASF-Pa <[email protected], the position is marginally consistent with the known X. V. H. Sbarufatti (INAF-OAB/PSU) and D. "The pattern we're seeing is observed in X-ray novae where the central object is a black hole," Boris Sbarufatti, an astrophysicist from Milan's Brera Observatory who currently is working with the. , GCN Circ. A. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 11:10:45 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRS 1716-249/GRO J1719-24/V2293 Oph. Leicester), V. 9603) comprising 6 ks in Photon Counting (PC) mode from T+16. Sbarufatti, V. 0 ks to 196. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti@brera. Dr. Boris Sbarufatti at INAF-OAB/IASFPA <boris. D. The data are all in Photon Counting (PC) mode. inaf. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks, with a 3. The data consist of 642 s in. Content may be subject to copyright. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the MAXI-detected burst. GCN 12064 table; GRB_name: GRB110604A: GCN_number: 12064: Detection_method: Konus-Wind Det: t_trigger: 14:49:45. The data are all in Photon Counting (PC) mode. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. it> B. (2005a, 2006). inaf. Holland1,2,3, Boris Sbarufatti4, Rongfeng Shens, Patricia Schady6, Jay R. Embed figure. P. Page, Silvia Zane, Alice A. Lien (GSFC/UMBC) and B. Burst Advocate for this burst is B. 9 ks exposure. Sbarufatti (INAF-OAB/PSU), P. inaf. it> V. (GCN Circ. 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. Melandri (INAF-OAB), D. UT on 2009 Apr17 (Sbarufatti et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. A. 8462) at 17:46:11. TITLE: GCN CIRCULAR NUMBER: 7195 SUBJECT: GRB080120: Swift XRT position DATE: 08/01/20 23:24:55 GMT FROM: Boris Sbarufatti at INAF-IASF-Pa B. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Siegel (PSU) report on behalf of the Swift-XRT team: We have analysed 15 ks of XRT data for GRB 150317A (Siegel et. , GCN Circ. Sbarufatti (INAF-IASF PA) report on behalf of the Swift-XRT team: The Swift-XRT observed GRB 080603B (trigger 313087, Mangano et al. D'Elia (ASDC), A. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. it> D. De Pasquale (MSSL) report on behalf of the Swift Team. Evans (U. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. We use the 80cm telescope of CHanging Event Survey at the YaoAn observation station(101. News; Events; Alumni; Faculty and Staff Directory; Utility Menu. 9 ks to T+391. Sbarufatti (PSU), K. it> B. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. edu> B. Holland 1,2,3, Boris Sbarufatti 4, Rongfeng Shen 5, Patricia Schady 6, Jay R. Boris Sbarufatti at PSU <[email protected] Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. it> B. . M. The refined position for the afterglow, obtained using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue (see. Breeveld, Samantha R. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Bicocca & INAF-OAB) A. The peak count rate was ~1,000 counts/sec (15-350 keV), at 0 sec after the trigger. Boris Sbarufatti at INAF-IASF-Pa <[email protected] hours after the trigger. Page (U. Our earliest-time LRIS images do not cover the position of the X-ray source reported by Sbarufatti et al. McCauley (PSU), J. Y. Palmer (LANL), M. 7 ks after the BAT trigger. My main interests are space science, observatory and satellite operations and high energy astrophysics. Sbarufatti (INAF-OAB/IASFPA), V. Evans (U. Baumgartner (GSFC/UMBC) The Swift-XRT began observing GRB 080506 (trigger=311159, Baumgartner et al. The data comprise 288 s in Windowed Timing (WT) mode (the first. Table 1 - uploaded by Boris Sbarufatti. Dive into the research topics where Boris Sbarufatti is active. Leicester), K. Y. R. Sbarufatti (INAF-OAB/IASFPA), J. directly from the image (Sbarufatti et al. B. 10968 ), from 96 s to 25. Copy reference. P. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. inaf. it> B. from publication: European. 3 ks of XRT data for GRB 110915A (Holland et al. sbarufatti@brera. We analyzed 3. D'Avanzo (INAF-OAB), J. it> B. GCN Circ. Margutti (INAF/OAB) and M. We consider a sample of 49 BL Lac objects from an ongoing spectroscopic program at the ESO VLT (B. 3 ks after the BAT trigger. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the. GCN Circ. Mangano (INAF/IASF Pa) report on behalf of the Swift XRT team Swift XRT began observations of GRB 080710 (Sbarufatti et al.