... Fan, X., Strauss, M. A., Annis, J., Gunn, J. E., Hennessy, G. S., Ivezic, Z., Knapp, G. R., Lupton, R. H., Munn, J. A., Newberg, H. J., Schneider, D. P., and Yanny, B., for the SDSS Collaboration, "Spectroscopy of Quasar Candidates from Sloan Digital Sky Survey Commissioning Data", 1998, After the Dark Ages: When Galaxies Were Young (the Universe at 2 < z < 5), Eds S. Holt and E. Smith, 282. ... The Discovery of a Field Methane Dwarf from Sloan Digital Sky Survey Commissioning Data", 1999, Ap. ...

... 337, 275­292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...

Astronomical Data Analysis Software and Systems XIII ASP Conference Series, Vol. ... CARMA's monitoring system (CAM), is designed to collect monitor data periodically from a set of heterogenous systems and organize these monitor points hierarchically. ... The Array Control Computer will require a uniform stream of monitor data from all of the different types of antennas, each with its own hardware and software. ... A Block Diagram of the CARMA Software System. ...

... This oral history interview is being conducted with Gwynne Shotwell at the Headquarters of the Space Exploration Technologies Corp., or SpaceX, in Hawthorne, California for the NASA Commercial Crew & Cargo Program Office History Project. ... We agreed jointly to go in and enhance the program. ... Shotwell: The biggest challenge, I think, that we had in the execution of this was convincing NASA, every step of the way, that though we?re going to do business very differently, we?re going to get it...

... The VLTI Spectro Imager (VSI) is the proposed second-generation near-infrared multi-beam instrument for the Very Large Telescope Interferometer, featuring three band operations (J, H and K), high angular resolutions (down to 1.1 milliarcsecond) and high spectral resolutions. ... FT optical throughput The resulting FT performance at VLTI with Unit Telescopes (8 meter diameter) are presented in Figure 6, where the achievable SNR in H and K band is shown as a function of the magnitude. ...