... RPFITS Files: Our working directory in Narrabri is /DATA/KAPUTAR_2/LVHIS ; for each observed galaxy a directory exists with subdirectories for the arrays, including data reduction scripts, notes,and results. ... Session 1: EW352 array, 22 x 12-h done. 2005, Jan 25 to 30 (B. Koribalski; 5 x 12-h); . ... 2006, Jan 28 (K. Kern; 1 x 12-h); . ... 2006, Jun 14-18 (B. Koribalski, A. Lopez-Sanchez, J. van Eymeren, 4 x 12-h), done. ... 2006, Nov 7/8 (B. Koribalski, E. Kirby; 2 x 12-h; remote) done. ...

... Science . ... Science Users Information > Science Publications > Science Announcements > Completion of Atacama Compact Array . ... ALMA . ... Instrumentation Development . ... Observing with ESO Telescopes . ... Data Handling and Products . ... The last 7-metre antenna forming the Atacama Compact Array (ACA) has been delivered to the ALMA high site. ... The ACA has been named the Morita Array after Professor Koh-ichiro Morita, who died in 2012 and was closely associated with the development of ALMA....

... 9.03.1999 . ... Credit: European Southern Observatory Explanation: The Very Large Telescope (VLT) Interferometric Array will be able to act as individual telescopes or as one huge telescope. ... Each VLT telescope by itself is now one of the largest optical telescopes in the world, joining the new cadre of large telescopes with mirrors greater than 8-meters in diameter. ... Publications with keywords: interferometry - VLT - telescope . Publications with words: interferometry - VLT - telescope . ...

... March 9, 1999 . The VLT Interferometric Array . ... Explanation: The Very Large Telescope (VLT) Interferometric Array will be able to act as individual telescopes or as one huge telescope. ... Over the next few years, the VLT telescopes will explore the universe in unprecedented detail, searching for everything from ordinary planets orbiting nearby stars to extraordinary explosions in the distant universe . Tomorrow's picture: First Light for VLT Kueyen . ... About APOD > . ...

... 739C As one part of a program to detect complete samples of active extragalactic objects, the 3.36x10^-3 sr field centered on alpha=12h04min, delta=+11deg30' (1950.0) was mapped with the Very Large Array at 1411MHz. Sixty-seven maps cover this field so that no point is more than 15arcmin from the nearest map center. ... The rms map noise is 0.030 + 0.001 mJy, and the resulting source list is complete to a map peak flux density S_p = 0.2 mJy within 25 arcmin of the field center. ...

... Proposal Type: General Category: Observation Category: Time Requested this semester: Hours Next Semester: Hours already used for this pro ject: Additional Hours required to complete pro ject: Minimum Useful Time: Expected Data Storage: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 18 0 0 0 1.5 hours less than 100 GB Expanding the NANOGrav Pulsar Timing Array Direct detection of gravitational waves (GW) is a ma jor goal in experimental physics and will open an entirely new astronomical spectrum...

... Posts tagged ?incompleteness? ... Comment . ... The notions of missing data are overall different between two communities. ... Astronomers?I?m not sure how they think but my impression so far is that a missing value in one attribute/variable from a object/observation/informant, all other attributes related to that object become useless because that object is not considered in scientific data analysis or model evaluation process. ... 2 Comments . ... Entries RSS . ... Entries (RSS) and Comments (RSS)...

... March 02 2001 09:00 (Moscow time) . The operations scheduled on OC "Mir" for March 1-2 are complete. During communication sessions the OC "Mir" onboard systems were checked out and the "Progress M1-5" facilities were used to perform orbit radio monitoring. ... The onboard systems performed norminally.  ... The OC "Mir" onboard systems will be checked out and orbit monitoring is scheduled for 2-3 March. ...