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J/A+AS/130/233 WATCH Solar X-Ray Burst Catalogue (Crosby+ 1998)
The WATCH Solar X-Ray Burst Catalogue Crosby N., Lund N., Vilmer N., Sunyaev R. <Astron. Astrophys. Suppl. Ser. 130, 233 (1998)> =1998A&AS..130..233C (SIMBAD/NED BibCode)
ADC_Keywords: Sun ; X-ray sources Mission_Name: GRANAT Keywords: catalogs - Sun: activity; flares; X-rays, gamma rays Description: Catalogue containing solar X-ray bursts measured by the Danish Wide Angle Telescope for Cosmic Hard X-Rays (WATCH) experiment aboard the Russian satellite GRANAT in the deca-keV energy range. Table 1 lists the periods during which solar observations with WATCH are available (WATCH ON-TIME) and where the bursts listed in the catalogue have been observed. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 40 205 On-time catalogue catalog.dat 80 1551 WATCH solar X-ray burst catalogue
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- DN Dump number 5- 12 A8 "DD/MM/YY" StartDate Start date of dump 14- 15 I2 h Starth Start time of dump 17- 18 I2 min Startm Start time of dump 20- 21 I2 s Starts Start time of dump 23- 30 A8 "DD/MM/YY" EndDate End date of dump 32- 33 I2 h End.h End time of dump 35- 36 I2 min End.m End time of dump 38- 39 I2 s End.s End time of dump
Byte-by-byte Description of file: catalog.dat
Bytes Format Units Label Explanations
1- 3 I3 --- DN dump number 5- 12 A8 "DD/MM/YY" Date Date when burst began 15- 20 I6 ct Pt Peak count rate in low-energy channel (in ct/bin) 22- 26 F5.2 s Tacc Accumulation time of bin (in s/bin) 28- 29 I2 h Tpeak.h Peak time of burst 31- 32 I2 min Tpeak.m Peak time of burst 34- 35 I2 s Tpeak.s Peak time of burst 37- 38 I2 h Tstart.h ? Start time of burst 40- 41 I2 min Tstart.m ? Start time of burst 43- 44 I2 s Tstart.s ? Start time of burst 45 A1 --- n_Tstart.h [N] N: Missing information 46- 47 I2 h Tend.h ? End time of burst 49- 50 I2 min Tend.m ? End time of burst 52- 53 I2 s Tend.s ? End time of burst 54 A1 --- n_Tend.h [N] N: Missing information 55- 58 I4 ct B Background count rate (in ct/bin) (1) 60 A1 --- H [01n] Signal in high-energy channel (2) 62 A1 --- d [d0] Dead-time effect in low-energy (3) 64 A1 --- o [o0] Overflow effect in low-energy (4) 66- 70 A5 --- AR Active region association (5) 72- 75 A4 --- GOES GOES flare identification (6) 77 I1 --- halpha [0/1] Hα association (7)
Note (1): Converted to the time accumulation of the bin. Note (2): '1' for yes, '0' for no, 'n' implies that some particle noise is observed in the high-energy channel, but not at the peak time of the burst. Note (3): 'd' for yes, '0' for no. Note (4): 'o' for yes, '0' for no. Note (5): '0' for no association. Note (6): 'N' for none, 'ng' implies that no GOES data exists. Note (7): '1' for yes, '0' for no.
Acknowledgements: Norma CROSBY References: Crosby N., 1996, Ph.D. thesis, Paris VII University, France. Crosby N., Vilmer N., Lund N., Sunyaev R., 1998A&A...334..299C Crosby N., Lund N., Vilmer N., Sunyaev R., 1998, A&AS, to be published. Lund N., 1985 in Culhane J.L., X-Ray Instrumentation in Astronomy, SPIE, 597, p.95.
(End) Patricia Bauer [CDS] 05-Jan-1998
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