We analyzed 3. Leicester) report on behalf of the Swift XRT team. Boris Sbarufatti; Stefano Ciprini; Jari Kotilainen [. Holland (GSFC/USRA), H. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. Sbarufatti (INAF OAB/INAF IASF-PA) and W. Barthelmy (GSFC), P. it> B. 6 ks in Photon Counting mode. Lien (GSFC/UMBC) and S. 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 Elia (ASDC), A. sbarufatti@brera. , Kotilainen, J. P. 9603) on 2009 July 2 at 14:15 UT, 3. 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. Breeveld and Samantha R. 2006) it remains one of the f ew bright sour ces. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. sbarufatti AT brera. Sbarufatti (PSU), A. it). 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. ] Renato Falomo; We present results of an ongoing program at the ESO VLT for spectroscopy of BL Lac objects lacking a firm redshift estimate. 28341. Boris Sbarufatti at INAF-OAB/IASFPA <boris. View publication. Astronomy & Astrophysics; Research output: Contribution to journal › Article › peer-review. D'Avanzo (INAF-OAB), A. it> Sbarufatti B. Sbarufatti (PSU), P. A. Osborne (U. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Palmer (LANL) report on behalf of the Swift-XRT team: We have analysed 6. A. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. Using t he imaging redshift method by Sbarufatti et al. Content may be subject to copyright. GCN Circ. Siegel (PSU) report on behalf of the Swift team: Examination of the full BAT data set for Swift trigger 629693 (Siegel et al. it> B. 15029), from 53 s to 35. Stephen T. B. (GCN 12067). 10998), from 48 s to 39. 2005 Sbarufatti et al. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The observation is in PC mode and consists of 1. Boris Sbarufatti at PSU <bxs60@psu. 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. ESO VLT optical spectroscopy of BL Lac objects. it> B. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. GCN Circ. Sbarufatti (PSU), K. The data comprise 24 s in Windowed Timing (WT) mode with the. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Pagani (U. A. Swift-XRT performed further observations on the afterglow candidate announced in Sbarufatti et al. La Parola (INAF-IASF PA) and W. { "subject": "GRB 200901A: Swift-XRT refined Analysis", "bibcode": "2020GCN. A. 10968 ), from 96 s to 25. Embed figure. inaf. (GCN 12067). Sbarufatti (INAF OAB/INAF IASF-PA) , V. A. 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. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. C. Moretti (INAF-OAB) report, on behalf of the Swift-XRT team We have analysed the first three orbits of Swift XRT data for GRB070621 (Sbarufatti et al. Sbarufatti, V. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. B. The observation is in PC mode and consists of 1. Sbarufatti T able 1: Roma-BZCA T blazars detected in the BA T surve y . inaf. sbarufatti@brera. Here’s how you knowDOI: 10. Y. Boris Sbarufatti at INAF-OAB/IASFPA <boris. L. The K-band luminosity functions of super star clusters in luminous infrared galaxies, their slopes, and the effects of blending #5. 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. Please contact the BA by email if you require additional information regarding Swift followup of this burst. sbarufatti@brera. Here’s how you knowDOI: 10. Holland (GSFC/USRA), H. , GCN Circ. Stroh (PSU), D. it> B. inaf. Due to an observing constraint, Swift will not slew until T0+40. D. 7687). . 7197) and by Schady & Sbarufatti (GCN Circ. Sbarufatti (boris. 10979), from 82 s to [email protected]. Cummings (GSFC/UMBC), N. E. 0 ks after the BAT trigger. , GCN circ. inaf. Mangano (INAF IASF-Pa), C. V. it> B. Sbarufatti (PSU), A. 13 UT on 2023-08-21, is due to misidentification of a known source during a Star Tracker Loss-of-Lock. Barthelmy (GSFC), P. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. Burrows (PSU), J. Burrows (PSU), J. 4 ks, with a 1. it> B. Proceedings of ScienceACCEPT & CONTINUE. Sbarufatti. Boris Sbarufatti at INAF-OAB/IASFPA <boris. D. R. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. (Sbarufatti et al. 2002) and the possible host galaxy of GRB 090417B. Sbarufatti (PSU), A. Mangano, V. inaf. Swift did not slew. Burst Advocate for this burst is. , GCN circ. At the present day, spectroscopic follow up of unclassified blazars have been mainly performed with 4 m or 8 m class telescopes (e. Melandri (INAF-OAB), T. The XRT began observing GRB 080405 (Cummings et al. Sbarufatti, R. from publication: European. In extremely urgent cases, after trying the Burst Advocate, you can contact the. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. A. There will be no XRT or UVOT data until this time. Siegel (PSU) report on behalf of the Swift team. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. , GCN Circ. This distribution has a mean value of. N. Krimm (GSFC/USRA), M. GCN Circ. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. Sbarufatti (boris. edu> B. The data are entirely in. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. 29529). Leicester) and M. The data comprise 24 s in Windowed Timing (WT) mode with the. Cummings (GSFC/UMBC), N. g. it>. Sbarufatti (1) and 18 other authors. Copy caption. Crossref. Pascoli, I-06123 Perugia, Italy 2. inaf. B. Boris Sbarufatti Osservatorio astronomico di Brera: Milano, Lombardia, IT 2011-10-01 to 2017-07-31 | Post-Doc Employment Show more detail Source : Boris. Mangano (INAF-IASFPA) and J. 17429. Mangano (INAF/IASF Pa) report on behalf of the Swift XRT team Swift XRT began observations of GRB 080710 (Sbarufatti et al. sbarufatti@brera. afterglows. 2 ks of XRT data for GRB 130725B (Swenson et al. 4 ks after the BAT trigger. inaf. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. email. Sbarufatti (PSU) report on behalf of. 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. Boris Sbarufatti at INAF-IASF-Pa <[email protected]. GCN [email protected]@brera. H. Baumgartner (GSFC/UMBC) The Swift-XRT began observing GRB 080506 (trigger=311159, Baumgartner et al. Kennea (PSU), [email protected] peak count rate was ~7000 counts/sec (15-350 keV), at ~2 sec after the trigger. 7 ks after the BAT trigger. , 2003, Ap&SS, 285, 367. GCN Circ. , Mangano V. 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. Burst Advocate for this burst is. C. edu) Subjects: X-ray, Neutron Star, Transient. inaf. 9905). Beardmore (U. Boris Sbarufatti at INAF-IASF-Pa <[email protected], the position is marginally consistent with the known X. 1 ks. Sbarufatti at this conference). 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. Description of the variables in the GRBweb catalogue. We secured medium resolution optical and near-infrared spectra of 4 bright BL Lac objects of unknown redshift using the. GCN Circ. These topic labels come from the works of this person. it> B. The peak count rate was ~1,000 counts/sec (15-350 keV), at 0 sec after the trigger. Lien (GSFC/UMBC), A. Lien. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. T. Boris Sbarufatti at INAF-OAB <boris. inaf. De Pasquale (MSSL) report on behalf of the Swift Team. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. Monthly Notices of the Royal Astronomical Society 525:3 (2023) 3626-3632. de Pasquale (INAF-IASFPA), A. Mangano (INAF IASF-PA), B. R. sbarufatti@uninsubria. La Parola (INAF-IASF Pa), T. 29529). Beardmore (U. sbarufatti AT brera. A. Moretti (INAF-OAB) report, on behalf of the Swift-XRT team We have analysed the first three orbits of Swift XRT data for GRB070621 (Sbarufatti et al. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. Boris. GCN Circ. The peak count rate was ~1,000 counts/sec (15-350 keV), at 0 sec after the trigger. Dr. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 05:00 UT on 2011 April 11. Sbarufatti over 6 years ago. Boris Sbarufatti INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Via Ugo La Malfa 153, I-90146 Palermo, Italy E-mail: sbarufatti@ifc. inaf. Please contact the BA by email if you require additional information regarding Swift followup of this burst. inaf. 10968 ), from 96 s to 25. N. The lightcurve is quite complex. The best position for the X-ray afterglow is the XRT. it> B. Sbarufatti, V. Mangano (INAF IASF-PA), B. D'Avanzo (INAF-OAB), V. it> B. Y. inaf. inaf. 2591 [astro-ph. , GCN Circ. , GCN Circ. Maselli (INAF-IASFPA), A. Leicester), J. it> B. Oates, Alberto J. La Parola (INAF-IASF PA) and W. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Gehrels (GSFC), S. Name Institution Dr. 41 ± 0. 2009) and identified it as an SDSS galaxy (Strauss et al. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et [email protected]@inaf. Sbarufatti, V. 8462) at 17:46:11. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. 0 ks after the BAT trigger. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Maselli (INAF-IASFPA) and P. 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. Table 1 - uploaded by Boris Sbarufatti. Page (U. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester), A. Evans ([email protected] ks of XRT data for GRB 110106B (Sbarufatti et al. inaf. Melandri (INAF-OAB), K. inaf. GRB 090417B was an unusually long burst with a T 90 duration of at least 2130 s and a multi-peaked light curve at energies of 15-150 keV. Lien (GSFC/UMBC) and B. it> B. B. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (INAF-OAB/PSU), L. D. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Maselli (INAF-IASFPA), A. L. Palmer (LANL), M. The source has faded with respect to the initial. A. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. 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. 0 ks after the BAT trigger. Sbarufatti (INAF-OAB/IASFPA), S. 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. inaf. [email protected] ks of exposure we don t detect. 2 ks exposure time. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 2 ks of XRT data for GRB 130518B (Cummings GCN Circ. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the. 3 ks after the BAT trigger. 7687). Roma-BZCA T blazars in the P alermo BA T Survey B. A. Guidorzi (Univ. Y. Fariborz Besarati (born 23 August 1966) is a Swedish former wrestler who competed in the 1992 Summer Olympics and in the 1996 Summer Olympics. Sbarufatti, V. T. 3 ks of XRT data for GRB 110915A (Holland et al. Leicester) and P. , GCN Circ. Find Boris Sbarufatti's email address, contact information, LinkedIn, Twitter, other social media and more. Mangano (PSU), M. 6466 ) with total exposure time of 3. GCN Circ. A. 11947) has not faded. 12335), from 82 s to 7. new redshifts, by B. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. 11440), from 126. M. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. An official website of the United States government. News; Events; Alumni; Faculty and Staff Directory2 dark and has been convincingly associated with a bright star-forming galaxy at a redshift of 0. sbarufatti@brera. 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. Leicester), A. Evans (U. 6 ks in. Raised by her mother, Sara and her. Beardmore (U Leicester), J. Boris Sbarufatti at PSU <[email protected] Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. 6 ks to 14. Perley, W. Sbarufatti, V. 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. News; Events; Alumni; Faculty and Staff Directory; Utility Menu. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Y. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. Sbarufatti (INAF-OAB/PSU) and C. 11944), from 2. La Parola, B. GCN Circ. GCN Circ. GCN Circ. Table 2 - uploaded by Boris Sbarufatti. Sbarufatti (INAF-OAB/PSU), L. GCN Circ. 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. De Pasquale (MSSL) report on behalf of the Swift Team. The data comprise 288 s in Windowed Timing (WT) mode (the first.