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J/ApJS/163/306 Chandra study of the Cep B star-forming region (Getman+, 2006)
Chandra study of the Cepheus B star-forming region: stellar populations and the initial mass function. Getman K.V., Feigelson E.D., Townsley L., Broos P., Garmire G., Tsujimoto M. <Astrophys. J. Suppl. Ser., 163, 306-334 (2006)> =2006ApJS..163..306G
ADC_Keywords: X-ray sources ; Interstellar medium ; Molecular clouds ; Stars, pre-main sequence Keywords: ISM: individual (Cepheus molecular cloud) - open clusters and associations: individual (Cepheus OB3) - stars: formation - stars: luminosity function, mass function - stars: pre-main-sequence - X-rays: stars Abstract: The Cepheus B (Cep B) molecular cloud and a portion of the nearby Cep OB3b OB association, one of the most active regions of star formation within 1kpc, have been observed with the ACIS detector on board the Chandra X-Ray Observatory. We detect 431 X-ray sources, of which 89% are confidently identified as clustered premain-sequence (PMS) stars. Description: The observation of Cep B and Cep OB3b was obtained on 2003 March 11.51-11.88 with the ACIS camera on board Chandra. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 101 431 Basic source properties table2.dat 88 431 2MASS counterparts table3.dat 82 431 X-ray spectroscopy and luminosities
See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) J/MNRAS/341/805 : UBVI CCD photometry of Cep OB3b (Pozzo+, 2003) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [GFT2006] CepB source number 5- 22 A18 --- CXOCepB The IAU designation (HHMMSS.ss+DDMMSS.s) 24- 33 F10.6 deg RAdeg Right ascension in decimal degrees (J2000) 35- 43 F9.6 deg DEdeg Declination in decimal degrees (J2000) 45- 50 F6.2 arcmin OAxis The off-axis angle 52- 57 F6.1 ct NetF Net total band (0.5-8.0keV) counts (1) 59- 62 F4.1 ct e_NetF Error in NetF 64- 67 F4.1 ct BkgF Background total band (0.5-8.0keV) counts extracted 69- 74 F6.1 ct NetH Net hard band (2.0-8.0keV) counts (1) 76- 79 F4.2 --- PSF Point spread fraction in extracted area at fiducial energy 1.5keV 81- 84 F4.1 --- Sig Source significance (in sigma) 86- 89 A4 --- Anom Source anomalies (2) 91 A1 --- Var Source variability from K-S test (3) 93- 96 F4.1 ks Exp Effective exposure time 98-101 F4.2 keV MedE Median energy in total band corrected for background
Note (1): In extracted area. Note (2): Source anomalies, defined as follows: g... = fractional time when source is on a detector (FRACEXPO) is <0.9 .e.. = source on field edge ..p. = source piled up ...s = source on readout streak Note (3): Source variability, defined as follows: a = no evidence for variability b = possibly variable c = definitely variable . = no test is performed for sources with <4 counts, or sources in chip gaps or on field edges
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [GFT2006] CepB source number 5- 22 A18 --- CXOCepB The IAU designation (HHMMSS.ss+DDMMSS.s) 24- 39 A16 --- 2MASS The 2MASS source identification 41- 44 F4.2 arcsec Offset ? Chandra-2MASS source positional offset 46- 50 F5.2 mag Jmag ? 2MASS J band brightness 52- 56 F5.2 mag Hmag ? 2MASS H band brightness 58- 62 F5.2 mag Ksmag ? 2MASS Ks band brightness 64- 66 A3 --- q_2MASS 2MASS photometric quality flag (1) 68- 70 A3 --- f_2MASS 2MASS contamination and confusion flag (2) 72- 76 F5.2 mag Av ? Visual absorption (3) 78- 82 F5.2 solMass Mass ? Stellar mass (3) 84- 88 F5.2 [solLum] Lbol ? Stellar bolometric luminosity (3)
Note (1): This is the phqual flag provided in the 2MASS All-Sky Data Release where the three characters refer to the JHK bands, defined as follows: A = very high significance detection (>10 SNR); B = high significance detection (>7 SNR); C = moderate significance detection (>5 SNR); D = low significance detection; E = point spread fitting poor; F = reliable photometric errors not available; U = upper limit on magnitude (source not detected); X = source is detected but no valid brightness estimate is available. Note (2): This is the ccflg provided in the 2MASS All-Sky Data Release where the three characters refer to the JHK bands, defined as: 0 = source unaffected by artifacts; b = bandmerge confusion (possible multiple source); c = photometric confusion from nearby star; d = diffraction spike confusion from nearby star; p = persistence contamination from nearby star; s = electronic stripe from nearby star. Note (3): From the 2MASS color-magnitude diagram.
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [GFT2006] CepB source number 5- 22 A18 --- CXOCepB The IAU designation (HHMMSS.ss+DDMMSS.s) 24- 28 F5.2 [cm-2] log(NH) Log of the Hydrogen column density 30- 34 F5.2 keV kT Plasma energy 36- 40 F5.2 [10-7W] Lh Log of observed hard band (2.0-8.0keV) luminosity (1) 42- 45 F4.2 [10-7W] e_Lh Error in Lh from simulations (1) 47- 51 F5.2 [10-7W] Lhc Log of estimated hard band luminosity corrected for absorption (1) 53- 56 F4.2 [10-7W] e_Lhc Error in Lhc from simulations (1) 58- 62 F5.2 [10-7W] Lt Log of observed total band (0.5-8.0keV) luminosity (1) 64- 67 F4.2 [10-7W] e_Lt Error in Lt from simulations (1) 69- 73 F5.2 [10-7W] Ltc Log of estimated total band luminosity corrected for absorption (1) 75- 78 F4.2 [10-7W] e_Ltc Error in Ltc from simulations (1) 80- 82 A3 --- MMDFl Source flag (2)
Note (1): In units of erg/s. Note (2): Three-part flag giving details on spectroscopy method, source membership, and stars with K-disks, defined as follows: b-- = spectral results from spectral fits of 174 relatively "bright" sources with >20 net counts. w-- = spectral results from NH_IR-MedE interpolation for 212 "weak" sources with known NH_IR. v-- = spectral results from fits of ungrouped spectra for 45 "weak" sources with unknown NH_IR. -e- = possible members of the embedded cluster. -l- = possible members of the lightly absorbed cluster. -o- = other possible members, found in the molecular cloud, not related to the embedded cluster. -a- = AGN candidates. -f- = field star candidates. --d = possible K-disk stars. --0 = stars with no K-disk.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 31-Jul-2007
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