Search

13 Mar 2012: Photon easy to detect and measure! [GeV]Tγp. 200 300 400 500 600 700. ... n=4.0 0.6 - 1.0!•MPL = 1029 200 - 100 GeV! 3/12/12 Astroparticle 23.

10 Apr 2013: Returns:. The output vircam_tfits object list. Author:. Jim Lewis, CASU. Definition at line 200 of file vircam_tfits.c.

15 Nov 1998: IBM or 100% compatible 200 MHz or better Pentium PC. Hard disk with at least 100 Mbytes of free space (a lot more if you are storing images on this disk).

14 May 2009: This involved using the One-Mile Radio Telescope of the Mullard Radio Astronomy Observatory to observe a sample of 200 bright radio sources in the 3C revised catalogue, at galactic latitudes

imreplace.upper = 200. imreplace.radius = 0. imrep. imreplace.images = "badpix". imreplace.value = 1. ... imreplace.imaginary = 0. imreplace.lower = 200. imreplace.upper = INDEF. imreplace.radius = 0.

25 Oct 2019: Your place in the cosmos. Lowestoft First Light Festival. Jun. 200.

16 Jun 2015: This involved using the One-Mile Radio Telescope of the Mullard Radio Astronomy Observatory to observe a sample of 200 bright radio sources in the 3C revised catalogue, at galactic latitudes

17 Feb 2009: Spiral structure at 200 AU implies planet at 150 AU • Same structure seen in Saturn’s rings (Charnoz et al. ... Numerical integrations of star, migrating planet, 200 planetesimals giving capture probabilities for 3:2 resonance:.

3 Sep 2007: artdata. A full-well capacity of 200,000 electrons was used for the saturation level.

23 Jan 2000: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

19 Apr 2006: This 200-AU-sized regioncoincides with the slightly tilted inner disk identified optically withthe Hubble Space Telescope5. ... The possible relationship of these components has yetto be explored, but the lower inferred temperatures of the clumpparticles

10 Apr 2013: 00334 00335 cpl_msg_info(fctid,"Doing the matching for extension %d",j); 00336 (void)ps.cat1f), 00337 vircam_tfits_get_table(ps.cat2f),200.0, 00338 &(vircam_matchxy_config.xoff),

25 Mar 2011: R is now 200 microns. This is very large on a quantum scale, but small on the scale used to test gravity in experiments – close to current limit of 100

18 Apr 2007: 200. 7. Mon. Not. R. Astron. Soc. 000, 1–6 (2006) Printed 9 April 2007 (MN LATEX style file v2.2). ... Doppler systems arepredicted here to form from 5-200 Jupiter masses of gas inthe disk, enough to make gas giant planets.

10 Nov 2017: Evidence for kinematically distinct outflows – discrete mass-loss episodes (strongly asymmetric)• Expansion velocities 40-50km/s• Kinematic age estimates for features, from distance/velocity, are 200, 400 and 900 years• Smallest

22 Mar 2024: collisional evolution. Only 6 systems with ages in the range 50 to 200 Myr were detected. ... The typical FWHM beam size of 1.′′5 (200 au) comfortably encompasses dust belts with radii up to 100 au.

18 Apr 2022: 11 174718. 11910 123109310. 638406 245. Number of detectable planets. 0 200 400. ... Sub-Neptunes Sub-Jovians0. 50. 100. 150. 200. 250. 300. 350. Det. ecta.

10 Apr 2013: fitslist[i]); 01534 val = cpl_image_get_mean_window(im,100,100,200,200); 01535 if (val > lthr && val < hthr) 01536 fitslist[m++] = fitslist[i]; 01537 else 01538 if (ditch) 01539

16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

13 Jul 2016: 0 100 200 300 400 500. UV Distance [kλ]. 100. 0. ... 100. 200. 300. Re(v. ) [m. Jy]. 0 100 200 300 400.