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J/A+A/418/841       XMM-Newton observations of N11 in the LMC   (Naze+, 2004)

XMM-Newton observations of the giant H II region N11 in the LMC. Naze Y., Antokhin I.I., Rauw G., Chu Y.-H., Gosset E., Vreux J.-M. <Astron. Astrophys. 418, 841 (2004)> =2004A&A...418..841N (SIMBAD/NED BibCode)
ADC_Keywords: Magellanic Clouds ; H II regions ; Photometry, ultraviolet Keywords: ISM: individual objects: LMC N11 - Magellanic Clouds - Galaxies: star clusters - ultraviolet: stars - X-rays: general Description: Using the XMM-Newton observatory, we have observed the giant H II region N11 of the LMC. The field includes three OB associations LH9, LH9, and LH13. Our XMM observations included parallel observations with the OM camera that provided us with unique UV and optical photometry of more than 6000 sources. In this paper we present the photometrical data for these sources as well as their cross-identifications with several catalogues. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 175 6250 OM photometry and identifications
See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) I/271 : The Guide Star Catalog, Version 2.2 (GSC2.2) (STScI, 2001) I/284 : The USNO-B1.0 Catalog (Monet+ 2003) J/AJ/103/1205 : Stellar Content of LH 9 and 10 in the LMC (Parker+ 1992) J/A+A/405/111 : LMC Survey of Young Stellar Systems (Gouliermis+, 2003) J/AJ/121/891 : UBV photometry of LMC OB associations (Parker+, 2001) Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 4 I4 --- OM Sequential number in OM observation 8- 15 F8.3 pix Xpos X coordinate (1) 17- 24 F8.3 pix Ypos Y coordinate (1) 26- 27 I2 h RAh Right ascension (J2000.0) 29- 30 I2 min RAm Right ascension (J2000.0) 32- 36 F5.2 s RAs Right ascension (J2000.0) 38 A1 --- DE- Declination sign (J2000.0) 39- 40 I2 deg DEd Declination (J2000.0) 42- 43 I2 arcmin DEm Declination (J2000.0) 45- 48 F4.1 arcsec DEs Declination (J2000.0) 51- 56 F6.3 mag Vmag ? V magnitude 59- 63 F5.3 mag e_Vmag ? V magnitude error 66- 71 F6.3 mag UVW1 ? UVW1 (245-320nm) magnitude 74- 78 F5.3 mag e_UVW1 ? UVW1 magnitude error 81- 86 F6.3 mag UVM2 ? UVM2 (205-245nm) magnitude 89- 93 F5.3 mag e_UVM2 ? UVM2 magnitude error 96-111 A16 --- 2MASS ? 2MASS identification (II/246) 113-118 F6.3 arcsec D(OM-2MASS) ? Distance between the OM and 2MASS sources 121-133 A13 --- GSC ? GSC-2.2.1 identification (I/271) 135-140 F6.3 arcsec D(OM-GSC) ? Distance between the OM and GSC sources 143-155 A13 --- USNO ? USNO-B1.0 identification (I/284) 157-162 F6.3 arcsec D(OM-USNO) ? Distance between the OM and USNO sources 165-168 I4 --- PGMW ? PGMW identification (J/AJ/103/1205) 170-175 F6.3 arcsec D(OM-PGMW) ? Distance between the OM and PGMW sources
Note (1): The observations were obtained in the so-called "Rudi-5" mode when the data from 5 separate windows covering adjacent parts of the OM CCD are collected and then transmitted to the ground. During the following processing, the windows are combined to form a virtual CCD of the size 1024/1024 pixels covering the whole field of view of the OM. X and Y are the coordinates on this virtual CCD. Pixel size is approximately 1 arcsec. Orientation on the sky plane is arbitrary.
Acknowledgements: Yael Naze
(End) Yael Naze & Igor I. Antokhin [IAG, Liege, Belgium] 09-Mar-2004
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

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