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J/MNRAS/357/645     LMC far-UV HST observations              (Almoznino+, 2005)

The deepest Hubble Space Telescope far-ultraviolet observations in the Large Magellanic Cloud. Almoznino E., Brosch N., Shara M., Zurek D. <Mon. Not. R. Astron. Soc., 357, 645-655 (2005)> =2005MNRAS.357..645A
ADC_Keywords: Magellanic Clouds ; Ultraviolet ; Photometry, CCD Keywords: stars: formation - galaxies: individual: Large Magellanic Cloud - galaxies: irregular - galaxies: stellar content Abstract: We present a new analysis of the deepest pure-ultraviolet (UV) observations with the highest angular resolution ever performed. A set of 12 exposures with the Hubble Space Telescope (HST) WFPC2 and F160BW filter obtained in parallel observing mode, which cover ∼12arcmin2 in the Large Magellanic Cloud (LMC), north of the bar and in the 'general field' region of the LMC, contain stars with far-UV monochromatic magnitudes as faint as 22mag. The 198 detected UV sources represent an accumulated exposure of 2x104s and reveal stars as faint as mUV≃20mag. We combine these observations with deep UBVI charge-coupled device (CCD) imaging of the same region reaching as faint as V≃26mag, and reselect probable optical counterparts for the UV sources. After a two-stage search-and-analysis process, we detect robust counterparts for 129 stars. These are mostly upper main-sequence stars, from early B to early A spectral classes, with several F stars. We point out the lack of blue supergiants, which could have been easily detected in our survey. We measure a foreground extinction E(B-V)≃0.08mag by Galactic dust and a surface density of star formation rate twice the average Galactic value. These observations indicate that relatively recent star formation took place even off the bar of the LMC. Description: New optical observations of a small fraction of the LMC, including the area studied with the HST, were performed by MS using the CTIO 4-m Victor Blanco Telescope with the Mosaic II CCD imager. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 275 129 FUV (160nm) stars in the HST LMC field
See also: J/AJ/117/206 : LMC far-ultraviolet imaging (Brosch+, 1999) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [BSM99] UV source number, from Brosch et al., 1999, Cat. J/AJ/117/206 4 A1 --- m_[BSM99] Multiplicity (for source #37) (1) 5- 6 I2 --- nObs Number of observations 8- 9 I2 h RAh HST right ascension (J2000.0) 10 A1 --- --- [:] 11- 12 I2 min RAm HST right ascension (J2000.0) 13 A1 --- --- [:] 14- 18 F5.2 s RAs HST right ascension (J2000.0) 20 A1 --- DE- HST declination sign (J2000.0) 21- 22 I2 deg DEd HST declination (J2000.0) 23 A1 --- --- [:] 24- 25 I2 arcmin DEm HST declination sign (J2000.0) 26 A1 --- --- [:] 27- 31 F5.2 arcsec DEs HST declination sign (J2000.0) 33- 34 I2 h RACh Corrected right ascension (J2000.0) 35 A1 --- --- [:] 36- 37 I2 min RACm Corrected right ascension (J2000.0) 38 A1 --- --- [:] 39- 44 F6.3 s RACs Corrected right ascension (J2000.0) 48 A1 --- DEC- Corrected declination sign (J2000.0) 49- 50 I2 deg DECd Corrected declination (J2000.0) 51 A1 --- --- [:] 52- 53 I2 arcmin DECm Corrected declination sign (J2000.0) 54 A1 --- --- [:] 55- 59 F5.2 arcsec DECs Corrected declination sign (J2000.0) 61- 65 F5.2 mag UVmag Far UV (F160BW, 160nm) magnitude 67- 70 F4.2 mag e_UVmag rms uncertainty on UVmag 72- 77 I6 --- [ABS2005] LMC optical counterpart number 79- 86 F8.3 pix Xpos X position 88- 94 F7.3 pix Ypos Y position 96- 97 I2 h RAOh CCD right ascension (J2000.0) 98 A1 --- --- [:] 99-100 I2 min RAOm CCD right ascension (J2000.0) 101 A1 --- --- [:] 102-106 F5.2 s RAOs CCD right ascension (J2000.0) 108 A1 --- DEO- CCD declination sign (J2000.0) 109-110 I2 deg DEOd CCD declination (J2000.0) 111 A1 --- --- [:] 112-113 I2 arcmin DEOm CCD declination sign (J2000.0) 114 A1 --- --- [:] 115-119 F5.2 arcsec DEOs CCD declination sign (J2000.0) 121-126 F6.3 mag Imag I magnitude 128-132 F5.3 mag e_Imag rms uncertainty on Imag 134 I1 --- o_Imag [3] Number of observations in I band 136-141 F6.3 mag Vmag V magnitude 143-147 F5.3 mag e_Vmag rms uncertainty on Vmag 149 I1 --- o_Vmag [3] Number of observations in V band 151-156 F6.3 mag Bmag B magnitude 158-162 F5.3 mag e_Bmag rms uncertainty on Bmag 164 I1 --- o_Bmag [3] Number of observations in B band 166-171 F6.3 mag Umag U magnitude 173-177 F5.3 mag e_Umag rms uncertainty on Umag 179 I1 --- o_Umag [3] Number of observations in U band 181-186 F6.3 mag V-I V-I colour index 188-192 F5.3 mag e_V-I rms uncertainty on V-I 194-199 F6.3 mag B-V B-V colour index 201-205 F5.3 mag e_B-V rms uncertainty on B-V 207-212 F6.3 mag U-B U-B colour index 214-218 F5.3 mag e_U-B rms uncertainty on U-B 220-225 F6.3 mag U-V U-V colour index 227-231 F5.3 mag e_U-V rms uncertainty on U-V 233-236 F4.2 arcsec Dist Distance between UV and optical source 238-243 F6.3 mag UV-I UV-I colour index 245-249 F5.3 mag e_UV-I rms uncertainty on UV-I 251-256 F6.3 mag UV-U UV-U colour index 258-262 F5.3 mag e_UV-U rms uncertainty on UV-U 264-269 F6.3 mag UV-V UV-V colour index 271-275 F5.3 mag e_UV-V rms uncertainty on UV-V
Note (1): in the original table, the source #37 appeared twice. The correct suffix was added at CDS in May 2007, according to the original list of Brosch et al. (1999AJ....117..206B)
History: * 07-Feb-2006: From electronic version of the journal * 31-May-2007: Suffix added in table2 for source #37
(End) Patricia Vannier [CDS] 07-Feb-2006
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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