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14 Apr 2014: 4990.24 0.9262011 0.03116661. 4990.28 0.9371514 0.03115548. 4990.32 0.9425622 0.03101928. Note that this example has only three columns. ... 2. H I 0.56100 0.0004240 24.5479 0.00 0.00E00! 3. statistics for whole fit:.

5 Mar 2014: the original Vega one based on ESO std fields observed each night APASSZPT= 24.147 / APASS ZP (mags) for default extinction APASSZRR= 0.012 / APASS ZP error (mags) APASSNUM= 104 / Number ... of APASS standards used NIGHTZPT= 24.155 / Average APASS ZP

23 Jul 2014: 1 -2.4 3.8 4.84 18.4#2 3.7 4.2 4.87 20.5#3 -9.0 4.2 5.80 24.4#4 49.1

10 Feb 2014: IRS pick-up camera at 16 and 22 µm and the MIPS 24 µm photometry to establish the absolute. ... and 22 µm and MIPS 24 µm broadband fluxes (listed in Table 3).

8 Apr 2014: This was interpreted as a transition from a dust-‐producing planetesimal belt to a region dominated by submicron-‐sized grains blown out by radiation pressure (9,24). ... The dashed line is an axisymmetric model for the parent body distribution

31 Jul 2014: 16 and MIPS 24 µm photometry (Farihi et al. 2008; Reach et al.2005). ... µMIPS 24 mµIRAC 8 m. Figure 1. Reduced infrared images of G29-38 taken with both Spitzer and Herschel.

11 Mar 2014: which at 50AU from the Sun corresponds to σv/vk = 0.056,0.13, 0.27, 0.55, and 1.24.

21 Jan 2014: Argon lamps were used for wave-length calibration. 24 images were taken with 1 second exposures.

22 Aug 2014: 4-35µm), three MIPS(24-160µm), and two SCUBA (450-850µm) bands. ... 2014). However, plotting their tempera-tures shows a probable correlation, with all Sun-like starshav-ing warm components<220K, but 15 out of 24 A-type starshaving warm components>220K

21 Jan 2014: The expected December 2010 source position of α = 22h 48m 4.7s,δ = 24 22m 9.9s is at the centre of the images, and the PACS pointing accuracy for these ... Figure 3 shows the limits on the fractional luminosity of adisc around TW PsA given these