Ground based γ-ray burst follow-up efforts: The first three years of the BATSE/COMPTEL/NMSU γ-ray burst rapid response network

1996 ◽  
Author(s):  
B. J. McNamara ◽  
T. E. Harrison ◽  
J. Ryan ◽  
R. M. Kippen ◽  
G. J. Fishman ◽  
...  
1996 ◽  
Vol 103 ◽  
pp. 173 ◽  
Author(s):  
Bernard J. McNamara ◽  
Thomas E. Harrison ◽  
J. Ryan ◽  
R. M. Kippen ◽  
M. McConnell ◽  
...  

2013 ◽  
Vol 9 (S296) ◽  
pp. 77-85
Author(s):  
Keiichi Maeda ◽  
Melina C. Bersten ◽  
Takashi J. Moriya ◽  
Gaston Folatelli ◽  
Ken'ichi Nomoto

AbstractWe review emission processes within the supernova (SN) ejecta. Examples of the application of the theory to observational data are presented. The emission processes and thermal condition within the SN ejecta change as a function of time, and multi-epoch observations are important to obtain comprehensive views. Through the analyses, we can constrain the progenitor radius, compositions as a function of depth, ejecta properties, explosion asymmetry and so on. Multi-frequency follow-up is also important, including radio synchrotron emissions and the inverse Compton effect, γ-ray emissions from radioactive decay of newly synthesized materials. The optical data are essential to make the best use of the multi-frequency data.


1995 ◽  
Vol 231 (1-2) ◽  
pp. 251-254 ◽  
Author(s):  
B. J. McNamara ◽  
T. E. Harrison ◽  
J. Ryan ◽  
R. M. Kippen ◽  
K. Bennett ◽  
...  

Author(s):  
JOHANNE RENAUD ◽  
DAVID A. BRENT ◽  
MARIANNE BAUGHER ◽  
BORIS BIRMAHER ◽  
DAVID J. KOLKO ◽  
...  

Resuscitation ◽  
2010 ◽  
Vol 81 (1) ◽  
pp. 31-35 ◽  
Author(s):  
Paolo Calzavacca ◽  
Elisa Licari ◽  
Augustine Tee ◽  
Moritoki Egi ◽  
Andrew Downey ◽  
...  

2012 ◽  
Vol 10 (H16) ◽  
pp. 138-138
Author(s):  
Shinsuke Abe

AbstractThe physical nature such as orbital distribution of asteroids is fundamental to understanding how our solar system has been evolved. The connection between Near-Earth Objects (NEOs) and Earth impactors such as meteorites and fireballs are still under debate, since there is no meteorite orbit whose parent NEO was identified. The orbital distribution of NEOs has been investigated by comprehensive sky surveys including Pan-STARRS (The Panoramic Survey Telescope And Rapid Response System). Here we focus on the Phaethon-Gemind complex detected by Pan-STARRS PS1 Prototype Telescope and our follow-up lightcurve observations.


2017 ◽  
Vol 98 (8) ◽  
pp. 1646-1651.e1 ◽  
Author(s):  
James M. Bjork ◽  
Thomas K. Burroughs ◽  
Laura M. Franke ◽  
Treven C. Pickett ◽  
Sade E. Johns ◽  
...  

2004 ◽  
Vol 13 (7) ◽  
pp. 549-553 ◽  
Author(s):  
Edward Chow ◽  
Kin-Wah Fung ◽  
Nicole Bradley ◽  
Lori Davis ◽  
Lori Holden ◽  
...  
Keyword(s):  

2021 ◽  
Vol 80 (Suppl 1) ◽  
pp. 960.1-960
Author(s):  
S. Garcia Perez ◽  
J. L. Modesto Dos Santos ◽  
J. Mendizabal ◽  
M. López I Gómez ◽  
G. Sada ◽  
...  

Background:The Remitting Seronegative Symmetrical Synovitis with Pitting Edema Syndrome (RS3PE) is a rare rheumatological disease, considered a benign process.Objectives:This study aims to describe its clinical features and serological markers, and also to analyze its possible association with neoplasms.Methods:An observational retrospective study was performed to assess demographic and clinical characteristics of patients diagnosed from RS3PE at a reference hospital amongst the Rheumatology and Internal Medicine departments, from 2010 to 2021.Results:Twenty-seven patients were included, with a mean age of 82.74 y.o. (IC95% 80.45-85.04; range 66 to 93), and a 51.85% proportion of males. Only 22.22% were from rural areas.All patients presented bilateral hand edema although some associated feet edema (40.74%) or morning stiffness (70.37%). Blood tests demonstrated anemia in 44.44% of patients. Inflammatory markers were elevated, such as C-Reactive Protein (29.23 mg/L, IC95% 18.17-40.29), erythrocyte-sedimentation rate (33.74 mm/hour, IC95% 24.22-43.26) and fibrinogen (531.6 mg/dL, IC95% 482.91-580.30). Only a few patients presented any autoimmune serological marker such as antinuclear antibodies (18.18%) or rheumatoid factor (8.70%).X-ray screening was realized to 22 patients. 14 showed of osteoarthritis radiologic presentation, 4 had radiological findings of chondrocalcinosis and one of them presented both. Only one patient had bone erosion.Malignancy screening was performed at diagnosis in only 29.63% of patients (all negative). During follow-up only two tumors were detected (mean accumulated follow-up: 40.37 months, IC95% 26.70-54.04; range 1 to 122) and there were adenocarcinoma primary neoplasms.All but one patient received low-dose corticosteroids, with a good and rapid response in all cases. Three patients received treatment with methotrexate (2) or leflunomide (1).Conclusion:RS3PE must be contemplated in elderly patients presenting with bilateral hand pitting edema and articular symptoms. No specific biomarkers have been described, but inflammatory reaction is often found in the absence of rheumatoid arthritis biomarkers. Rapid response to corticosteroids is prevalent. Only two neoplasms were detected during follow-up.References:[1]Paira S, Graf C, Roverano S, Rossini J. Remitting seronegative symmetrical synovitis with pitting oedema: a study of 12 cases. Clin Rheumatol. 2002 May;21(2):146-9. doi: 10.1007/pl00011218. PMID: 12086166.[2]Cobeta García JC, Martínez Burgui J. RS3PE syndrome or benign edematous polysynovitis in the elderly. Study of 8 cases. Rev Clin Esp. 1999 Dec;199(12):785-9. Spanish. PMID: 10687410.[3]Moreno Obregón F, Del Castillo Madrigal M, Díaz Narváez F, Pérez Delgado FJ. RS3PE syndrome with positive rheumatoid factor. Reumatol Clin. 2019 Nov-Dec;15(6):e168-e169. English, Spanish. doi: 10.1016/j.reuma.2017.11.009. Epub 2017 Dec 15. PMID: 29254743Disclosure of Interests:None declared


Author(s):  
G E Anderson ◽  
M E Bell ◽  
J Stevens ◽  
M D Aksulu ◽  
J C A Miller-Jones ◽  
...  

Abstract We introduce the Australia Telescope Compact Array (ATCA) rapid-response mode by presenting the first successful trigger on the short-duration gamma-ray burst (GRB) 181123B. Early-time radio observations of short GRBs may provide vital insights into the radio afterglow properties of Advanced LIGO- and Virgo-detected gravitational wave events, which will in turn inform follow-up strategies to search for counterparts within their large positional uncertainties. The ATCA was on target within 12.6 hr post-burst, when the source had risen above the horizon. While no radio afterglow was detected during the 8.3 hr observation, we obtained force-fitted flux densities of 7 ± 12 and 15 ± 11μJy at 5.5 and 9 GHz, respectively. Afterglow modelling of GRB 181123B showed that the addition of the ATCA force-fitted radio flux densities to the Swift X-ray Telescope detections provided more stringent constraints on the fraction of thermal energy in the electrons (log $\epsilon _e = -0.75^{+0.39}_{-0.40}$ rather than log $\epsilon _e = -1.13^{+0.82}_{-1.2}$ derived without the inclusion of the ATCA values), which is consistent with the range of typical εe derived from GRB afterglow modelling. This allowed us to predict that the forward shock may have peaked in the radio band ∼10 days post-burst, producing detectable radio emission ≳ 3 − 4 days post-burst. Overall, we demonstrate the potential for extremely rapid radio follow-up of transients and the importance of triggered radio observations for constraining GRB blast wave properties, regardless of whether there is a detection, via the inclusion of force-fitted radio flux densities in afterglow modelling efforts.


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