J/A+A/456/977       XMM observations of NGC 2516 stars       (Marino+, 2006)

X-ray variability of NGC 2516 stars in the XMM-Newton observations. Marino A., Micela G., Pillitteri I., Peres G. <Astron. Astrophys., 456, 977-983 (2006)> =2006A&A...456..977M 2006A&A...456..977M
ADC_Keywords: Clusters, open ; Stars, late-type ; X-ray sources ; Photometry, UBVRI Keywords: X-ray: stars - stars: activity - stars: early-type - stars: late-type - stars: coronae - galaxy: open clusters and associations: individual: NGC 2516 Abstract: We present the characteristics of the X-ray variability of stars in the cluster NGC 2516 as derived from XMM-Newton/EPIC/pn data. The X-ray variations on short (hours), medium (months), and long (years) time scales have been explored. We detected 303 distinct X-ray sources by analysing six EPIC/pn observations; 194 of them are members of the cluster. Stars of all spectral types, from the early-types to the late-M dwarfs, were detected. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 07 58 06 -60 45.0 NGC 2516 = C 0757-607 ------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 44 6 XMM-Newton/EPIC/pn observations of NGC 2516 table2.dat 77 474 X-ray and optical properties of NGC 2516 members in the XMM-Newton/EPIC/pn observations having more than 25 counts. -------------------------------------------------------------------------------- See also: J/A+A/312/818 : NGC 2516 X-ray sources (Dachs+, 1996) J/A+A/375/863 : Photometry in NGC 2516 (Jeffries+, 2001) J/AJ/123/290 : UBVI CCD photometry of NGC 2516 (Sung+, 2002) J/ApJ/588/1009 : Chandra X-ray observations of NGC 2516 (Damiani+, 2003) J/ApJ/606/466 : X-ray variability in NGC 2516 (Wolk+, 2004) J/A+A/450/993 : XMM survey of NGC 2516 (Pillitteri+, 2006) J/MNRAS/367/781 : XMM observations of NGC 2547 (Jeffries+, 2006) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Obs Observation code 3- 12 I010 --- ObsId XMM Observation identification number 14- 16 I3 --- Orbit Orbit number 18- 21 F4.1 ks FTime Filtered time 23- 32 A10 "YYYY/MM/DD" ObsDate Start date 34- 36 I3 --- NX-ray Number of X-ray source 38- 40 I3 --- Ndetect Number of detected members 42- 44 I3 --- Nopt Number of optical members -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- JTH JTH number (Cl* NGC 2516 JTH NNNNN in Simbad) 7 A1 --- Obs [a-f] Observation code, in table1.dat 9- 10 I2 h RAh Right ascension (J2000) 12- 13 I2 min RAm Right ascension (J2000) 15- 19 F5.2 s RAs Right ascension (J2000) 21 A1 --- DE- Declination sign (J2000) 22- 23 I2 deg DEd Declination (J2000) 25- 26 I2 arcmin DEm Declination (J2000) 28- 31 F4.1 arcsec DEs Declination (J2000) 33- 38 F6.3 mag Vmag V magnitude 40- 45 F6.3 mag B-V ? B-V colour index 47- 51 F5.3 mag V-I ? V-I colour index 53- 59 F7.1 s ExpTime Exposure time 61- 66 F6.3 ct/ks CRate Count Rate (0.2-2keV) 68- 72 F5.3 ct/ks e_CRate rms uncertainty on CRate 74- 75 A2 --- l_K-S [≥] Limit on K-S probability 76-77 I2 % K-S ? Result of the Kolmogorov-Smirnov membership probability test -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 07-Apr-2007
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line