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J/MNRAS/376/960 X-ray emission from the Sombrero galaxy (NGC 4594) (Li+, 2007)
Chandra and XMM-Newton detection of large-scale diffuse X-ray emission from the Sombrero galaxy. Li Z., Wang Q.D., Hameed S. <Mon. Not. R. Astron. Soc., 376, 960-976 (2007)> =2007MNRAS.376..960L
ADC_Keywords: Galaxies, nearby ; X-ray sources Keywords: galaxies: general - galaxies: individual: Sombrero, NGC 4594 - galaxies: spiral - X-rays: general Abstract: We present an X-ray study of the massive edge-on Sa galaxy, Sombrero (M 104; NGC 4594), based on XMM-Newton and Chandra observations. A list of 62 XMM-Newton and 175 Chandra discrete X-ray sources is provided, the majority of which are associated with the galaxy. Spectral analysis is carried out for relatively bright individual sources and for an accumulated source spectrum. Description: The Chandra ACIS-S observation of Sombrero (Obs. ID. 1586) was taken on 2001 May 31 with an exposure of 18.8ks. The XMM-Newton EPIC observation of Sombrero (Obs. ID 0084030101) was taken on 2001 December 28, with the thin filter and with a total exposure of 43ks. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 63 175 Chandra source list table3.dat 64 62 XMM-Newton source list table4.dat 49 8 Matching results with 2MASS
See also: J/ApJ/599/1067 : X-ray sources in M104 (Di Stefano+, 2003) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [LWH2007] [1/175] Source designation, [LWH2007] Chandra NNN in Simbad 5- 23 A19 --- CXOU CXOU name (JHHMMSS.ss-DDMMSS.s) 25- 27 F3.1 arcsec e_Pos Position uncertainty (1σ) calculated from the maximum likelihood centroiding 29- 34 F6.2 ct/ks CR On-axis source broad-band count rate (1) 36- 39 F4.2 ct/ks e_CR rms uncertainty on CR 41- 45 F5.2 --- HR ?=- Harness ratio, HR=(H-S2)/(H+S2) (2) 47- 50 F4.2 --- e_HR ?=- rms uncertainty on HR 52- 56 F5.2 --- HR1 ?=- Harness ratio 1, HR1=(S2-S1)/S (2) 58- 61 F4.2 --- e_HR1 ?=- rms uncertainty on HR1 63 A1 --- Band [BSH] band in which a source is detected with the most accurate position that is adopted in Position uncertainty (e_Pos)
Note (1): The sum of the exposure-corrected CRs in the four bands. Note (2): Definition of the bands: S1=0.3-0.7keV, S2=0.7-1.5keV, H1=1.5-3keV and H2=3-7keV. In addition, S=S1+S2, H=H1+H2 and B=S+H. The hardness ratios defined as HR=(H-S2)/(H+S2), and HR1=(S2-S1)/S, listed only for values with uncertainties less than 0.2.
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [LWH2007] [1/62] Source designation, [LWH2007] XMM NNN in Simbad 5- 23 A19 --- XMMU XMMU name (JHHMMSS.ss-DDMMSS.s) 25- 27 F3.1 arcsec e_Pos Position uncertainty (1σ) calculated from the maximum likelihood centroiding 29- 34 F6.2 ct/ks CR On-axis source broad-band count rate (1) 36- 40 F5.2 ct/ks e_CR rms uncertainty on CR 42- 46 F5.2 --- HR ?=- Harness ratio, HR=(H-S2)/(H+S2) (2) 48- 51 F4.2 --- e_HR ?=- rms uncertainty on HR 53- 57 F5.2 --- HR1 ?=- Harness ratio1, HR1=(S2-S1)/S (2) 59- 62 F4.2 --- e_HR1 ?=- rms uncertainty on HR1 64 A1 --- Band [BSH] band in which a source is detected with the most accurate position that is adopted in Position uncertainty (e_Pos)
Note (1): The sum of the exposure-corrected CRs in the four bands. Note (2): Definition of the bands: S1=0.5-1keV, S2=1-2keV, H1=2-4.5keV and H2=4.5-7.5keV. In addition, S=S1+S2, H=H1+H2 and B=S+H. The hardness ratios defined as HR=(H-S2)/(H+S2), and HR1=(S2-S1)/S, listed only for values with uncertainties less than 0.2.
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 2 A2 --- List [XA XP] XA for table2, XP for table3 3 A1 --- --- [-] 4- 6 I3 --- [LWH2007] Source designation 8- 26 A19 --- Name Name (JHHMMSS.ss+DDMMSS.s) 28- 30 F3.1 arcsec Dox Distance between X-ray and optical position 32- 34 F3.1 arcsec e_Dox rms uncertainty on Dox 36- 39 F4.1 mag Jmag J magnitude 41- 44 F4.1 mag Hmag H magnitude 46- 49 F4.1 mag Kmag K magnitude
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 28-Sep-2007
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