/ftp/cats/J/A+A/530



Subdirectories represent pages of A+A vol. 530

drwxr-xr-x 318 cats archive 8192 Apr 22 10:18 [Up] -rw-r--r-- 1 cats archive 47 Apr 28 2011 .message drwxr-xr-x 4 cats archive 4096 Feb 17 17:05 A108 drwxr-xr-x 9 cats archive 4096 Dec 15 09:38 A115 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A118 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A120 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A138 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A146 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A147 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A15 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A150 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A151 drwxr-xr-x 5 cats archive 4096 Dec 15 09:38 A18 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A2 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A21 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A28 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A31 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A33 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A42 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A5 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A50 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A54 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A58 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A72 drwxr-xr-x 3 cats archive 4096 Dec 15 09:38 A86 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A90 drwxr-xr-x 2 cats archive 4096 Dec 15 09:38 A93 -rw-r--r-- 1 cats archive 13377 Feb 1 2013 ReadMe
Beginning of ReadMe : File: NrecxLrec Unix Z Explanation J/A+A/530/A108/ReadMe: 144x80 18b 0b VLT-FLAMES Tarantula Survey (Evans+, 2011) J/A+A/530/A108/table5.dat: 930x154 146b 46b Observational information for the VLT-FLAMES Tarantula J/A+A/530/A108/table6.dat: 918x58 107b 32b Near-IR photometry from the InfraRed Survey Facility J/A+A/530/A108 =====>: 1992x1544 271b 78b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A115/ReadMe: 220x80 28b 0b Rotating massive MS stars evolutionary models (Brott+, 2011) J/A+A/530/A115/evol/*: 663x. 965646b 0b J/A+A/530/A115/iso/*: 528x. 3819816b 0b J/A+A/530/A115/isochron.dat: 528x3 38b 0b List of isochrones files J/A+A/530/A115/models.dat: 663x33 45b 0b List of models files J/A+A/530/A115 =====>: 2602x80 9 4785573b 0b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A118/ReadMe: 59x80 8b 0b G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011) J/A+A/530/A118/maps/*: 4x. 750b 0b J/A+A/530/A118/table1.dat: 2x71 2b 0b List of stars J/A+A/530/A118 =====>: 65x80 2 760b 0b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A120/ReadMe: 168x80 23b 0b Mid-infrared diameter of W Hydrae (Zhao-Geisler+, 2011) J/A+A/530/A120/data.dat: 71x1133 159b 46b Calibrated visibilities of W Hya J/A+A/530/A120/table1.dat: 83x46 9b 4b Observation log J/A+A/530/A120 =====>: 322x1131 191b 50b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A138/ReadMe: 194x80 23b 0b Geneva-Copenhagen survey re-analysis (Casagrande+, 2011) J/A+A/530/A138/catalog.dat: 16682x62 14403b 3856b *Stellar parameters J/A+A/530/A138 =====>: 16876x4412 14426b 3856b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A146/ReadMe: 116x80 15b 0b eps Aur eclipse spectral and photometric analysis (Chadima+, 2011) J/A+A/530/A146/table1a.dat: 105x13 29b 11b eps Aur CI,EW,RV of various spectral lines J/A+A/530/A146/table1b.dat: 201x13 54b 17b eps Aur CI,EW,RV of various spectral lines J/A+A/530/A146/table1c.dat: 47x74 8b 4b eps Aur CI,EW,RV of various spectral lines J/A+A/530/A146/table2a.dat: 204x68 29b 9b U,B,V photometry of eps Aur (Hvar Observatory) J/A+A/530/A146/table2b.dat: 198x68 28b 8b U,B,V photometry of HR 1644 (Hvar Observatory) J/A+A/530/A146 =====>: 871x1332 163b 49b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A147/ReadMe: 117x80 15b 0b Megamaser detection in Seyfert galaxies (Ramolla+, 2011) J/A+A/530/A147/refs.dat: 71x46 7b 4b References J/A+A/530/A147/table1.dat: 163x49 14b 7b Off-sample sources appended after l 133 J/A+A/530/A147/table3.dat: 163x75 26b 8b Measured fluxes and literature values J/A+A/530/A147 =====>: 514x80 8 62b 19b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A15/ReadMe: 88x80 11b 0b Abundances of 94 stars (Nissen+, 2011) J/A+A/530/A15/table1.dat: 53x75 9b 4b Data based on VLT/UVES spectra J/A+A/530/A15/table2.dat: 47x75 8b 4b Data based on NOT/FIES spectra J/A+A/530/A15/table3f.dat: 9212x46 847b 99b Equivalent widths from NOT/FIES spectra J/A+A/530/A15/table3u.dat: 10388x4 955b 111b Equivalent widths from VLT/UVES spectra J/A+A/530/A15 =====>: 19788x80 1830b 218b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A150/ReadMe: 199x80 24b 0b lambda Ori young open clusters XMM obs. (Franciosini+, 2011) J/A+A/530/A150/table1.dat: 58x98 13b 5b X-ray and optical properties of sources identified J/A+A/530/A150/table2.dat: 24x78 5b 3b X-ray sources identified with possible new J/A+A/530/A150/tablea1.dat: 169x10 30b 10b X-ray sources detected in the lambda Ori cluster J/A+A/530/A150/tablea2.dat: 78x122 20b 7b 3sigma upper limits and optical properties of J/A+A/530/A150 =====>: 528x1221 92b 25b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A151/ReadMe: 64x80 8b 0b V light curve of WR 123 (Chene+, 2011) J/A+A/530/A151/fig1.dat: 142x31 10b 4b Light curve of WR 123 obtained at Bell J/A+A/530/A151 =====>: 206x80 2 18b 4b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A18/ReadMe: 173x80 22b 0b Nebular NII lines effective recombination coeff. (Fang+, 2011) J/A+A/530/A18/table3.dat: 217x122 54b 0b Case B effective recombination coefficients for J/A+A/530/A18/table4.dat: 217x122 54b 0b Case B effective recombination coefficients for J/A+A/530/A18/table5.dat: 217x122 54b 0b Case B effective recombination coefficients for J/A+A/530/A18/table6.dat: 217x122 54b 0b Case B effective recombination coefficients for J/A+A/530/A18/table7.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table8.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table9.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table10.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table11.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table12.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table13.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table14.dat: 55x129 15b 0b Fit parameters and maximum errors delta for J/A+A/530/A18/table15.dat: 26x70 5b 0b Comparison of our direct recombination J/A+A/530/A18 =====>: 1507x129 363b 0b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A2/ReadMe: 126x80 15b 0b New hot subdwarf stars (Oreiro+, 2011) J/A+A/530/A2/table3.dat: 15x114 5b 3b List of candidates in the Kepler field-of-view J/A+A/530/A2/table7.dat: 73x60 9b 5b List of the 73 candidates in and around the J/A+A/530/A2 =====>: 214x114 29b 8b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A21/ReadMe: 170x80 21b 0b Spectral properties of 438 GRBs (Nava+, 2011) J/A+A/530/A21/table2.dat: 345x103 72b 26b Spectral parameters of the time-averaged spectra of J/A+A/530/A21/table3.dat: 114x66 16b 7b *Spectral parameters of the time-averaged spectra of J/A+A/530/A21/table4.dat: 234x115 55b 20b Spectral parameters of the peak spectra of 235 J/A+A/530/A21/table5.dat: 228x107 50b 13b Spectral parameters of the Fermi/GBM GRBs collected J/A+A/530/A21 =====>: 1091x115 214b 66b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A28/ReadMe: 137x80 17b 0b MUCHFUSS project (Geier+, 2011) J/A+A/530/A28/refs.dat: 36x132 5b 3b References J/A+A/530/A28/table2.dat: 69x46 8b 4b Priority targets for follow-up J/A+A/530/A28/table3.dat: 17x88 4b 3b Priority targets for follow-up (HRV subsample) J/A+A/530/A28/table4.dat: 52x88 11b 5b Priority targets for follow-up (RRV subsample) J/A+A/530/A28/tablea1.dat: 89x80 16b 6b Orbital parameters of all known hot subdwarf J/A+A/530/A28 =====>: 400x132 61b 21b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A31/ReadMe: 149x80 18b 0b Stellar parameters from 10 Galactic GC fields (Lane+, 2011) J/A+A/530/A31/table1.dat: 28244x12 6732b 2157b Parameters from the RAVE pipeline for all fields J/A+A/530/A31/table2.dat: 8788x118 2044b 598b Parameters from the KISS pipeline for fields J/A+A/530/A31/table3.dat: 20563x14 5945b 1808b Parameters from the KISS pipeline for fields J/A+A/530/A31 =====>: 57744x147 14739b 4563b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A33/ReadMe: 127x80 15b 0b S/Zn method for silicon depletion in DLA systems (Vladilo+, 2011) J/A+A/530/A33/refs.dat: 56x103 6b 3b References J/A+A/530/A33/table4.dat: 35x81 7b 4b The Zn+S sample of DLA systems selected as J/A+A/530/A33/table5.dat: 47x81 9b 4b The Z sample: DLA systems with measurements of J/A+A/530/A33/table6.dat: 29x81 6b 3b The S sample: DLA systems with measurements of J/A+A/530/A33/table8.dat: 378x71 55b 15b Evolutionary tracks of the reference model of J/A+A/530/A33 =====>: 672x103 98b 29b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A42/ReadMe: 112x80 13b 0b X-ray properties of AGN in XBS (Corral+, 2011) J/A+A/530/A42/table2.dat: 305x92 52b 16b Summary of XMM-Newton observations used J/A+A/530/A42/table3.dat: 305x95 57b 19b Power law fit results J/A+A/530/A42 =====>: 722x95 122b 35b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A5/ReadMe: 88x80 11b 0b WASP-4b Ks-band detection of thermal emission (Caceres+, 2011) J/A+A/530/A5/table1.dat: 24071x31 1506b 325b Secondary eclipse light curve J/A+A/530/A5 =====>: 24159x80 1517b 325b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A50/ReadMe: 101x80 13b 0b Principal Component Analysis of QSO UV spectra (Paris+, 2011) J/A+A/530/A50/proj.dat: 10x89 3b 0b Projection matrix J/A+A/530/A50/xi.dat: 1962x106 412b 113b Principal Components over the full wavelength J/A+A/530/A50/zeta.dat: 1569x106 329b 92b Principal Components redwards to Ly-alpha emission J/A+A/530/A50 =====>: 3642x106 757b 205b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A54/ReadMe: 75x80 10b 0b Bulge K giant abundances (Gonzalez+, 2011) J/A+A/530/A54/table4.dat: 650x49 65b 17b Abundances of 650 bulge red giant branch stars J/A+A/530/A54 =====>: 725x80 75b 17b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A58/ReadMe: 97x80 12b 0b Stars in early-type dwarf galaxies JKVI phot. (Crnojevic+, 2011) J/A+A/530/A58/table3.dat: 228x99 46b 15b AGB candidates list J/A+A/530/A58 =====>: 325x99 58b 15b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A72/ReadMe: 116x80 15b 0b Fermi sources with massive YSO associations (Munar-Adrover+, 2011) J/A+A/530/A72/table3.dat: 22x135 7b 3b Positional coincidence of Fermi sources with J/A+A/530/A72/table4.dat: 2x113 2b 0b Positional coincidence of Fermi sources with J/A+A/530/A72/table5.dat: 5x114 3b 0b Positional coincidence of Fermi sources with J/A+A/530/A72/table6.dat: 113x140 33b 10b Positional coincidence of Fermi sources with J/A+A/530/A72 =====>: 258x140 60b 13b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A86/ReadMe: 143x80 18b 0b Hubble Legacy Archive ACS grism data (Kuemmel+, 2011) J/A+A/530/A86/tablea1.dat: 15x38 3b 0b List of failed associations J/A+A/530/A86/tablea2.dat: 54x96 11b 5b Objects with determined redshifts J/A+A/530/A86/tablea3.dat: 440x112 98b 19b The associations included in this release J/A+A/530/A86 =====>: 652x112 130b 24b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A90/ReadMe: 187x80 23b 0b Optically bright post-AGB population of LMC (van Aarle+, 2011) J/A+A/530/A90/cat_pagb.dat: 1407x6 1664b 293b Post-AGB candidates J/A+A/530/A90/cat_sg.dat: 286x486 274b 58b Discarded possible supergiants J/A+A/530/A90/cat_spec.dat: 89x606 107b 23b Discarded objects with a spectral type J/A+A/530/A90/cat_yso.dat: 6823x48 6491b 1021b Discarded possible YSOs J/A+A/530/A90 =====>: 8792x606 8559b 1395b Total File: NrecxLrec Unix Z Explanation J/A+A/530/A93/ReadMe: 226x80 28b 0b de Houtman, Kepler and Halley star catalogs (Verbunt+ 2011) J/A+A/530/A93/aliter.dat: 20x82 5b 3b Variants on Secunda Classis (Kepler (1627) J/A+A/530/A93/classis.dat: 434x82 72b 25b Secunda Classis and Tertia Classis Kepler (1627) J/A+A/530/A93/halley.dat: 341x139 74b 0b Star catalogue of Halley (1679) J/A+A/530/A93/houtman.dat: 304x70 44b 17b Star Catalogue of de Houtman (1603) J/A+A/530/A93 =====>: 1325x139 223b 45b Total

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