. Next: Auto-baselining Up: Basic Processing Previous: Time average separate scans . To make a baseline fit, you must first create a mask of channels to use in the baseline fit. ASAP> msk = scans.create_mask([100,400],[600,900]) ASAP> scans.poly_baseline(msk, 1) . This will fit a first order polynomial to the selected channels and subtract this polynomial from the full spectra. Subsections . Auto-baselining . Malte Marquarding 2005-11-30

The purpose of these tools is to provide a control mechanism for flagging an LRP as baselined in ASSIST.. ... Viewgraph on Desired Baselining Procedure. Outline of New Baseline Tool Requirements (Investigated and documented by Tony Roman) . ... Bill W.?) which detail what notifications need to be sent to the LRPG account when a calendar is baselined. ... Below is a viewgraph (same author as previous viewgraphs?) detailing what notification needs to be sent to the PCs when the LRP is baselined. ...

... Science . ... Science Users Information > Science Publications > Science Announcements > Release of ALMA Long Baseline Campaign Science Verification Data . ... Observing with ESO Telescopes . ... A new installment of ALMA Science Verification (SV) data is available. This release contains several new datasets corresponding to four targets observed as part of the 2014 ALMA Long Baseline Campaign in order to demonstrate the long baseline (~10 km), high angular resolution, capability of ALMA. ...

OptInt PmWiki . MROI Delay Line SW / . Edit Page | Page History | ... MROI Delay Line Design Contract . ... MROI DL Production SW Contract . ... Software Design Documentation . ... MROI . ... MROI DL Design Contract Private Material . ... Baseline Solution Software . ... May be best to implement within a framework which is an embryonic form of the MROI offline software framework - but we need to design the framework! ISS Supervisor able to launch specific offline data analysis tasks . ...

Next: Submitting a Telescope Proposal Up: Astronomer's Guide to the Previous: Pulsars . Arecibo presently supports VLBI for up to a maximum of 4% of its astronomy observing time. ... Arecibo is equipped with a a VLBA4 recording system, compatible with the HSA, EVN and Global networks, and the 305-m telescope is available for scheduling with any of them. ... From 2004, Arecibo has used a VLBA4 Data-Acquisition Rack, together with a Mark-5A disk-based VLBI recording system. ...

... 50 Weirdest Objects . ... Observing springtime deep-sky objects with a large telescope . ... What is the baseline for determining the magnitude scale of celestial objects? Why do brighter objects have negative numbers? ... He called the brightest 1st magnitude and the faintest 6th magnitude. ... Also, to assign a magnitude to the brightest planets, the Moon, and especially the Sun, scientists would have to work with negative numbers. Get instant access to subscriber content on Astronomy.com! ...

Find Similar Abstracts (with default settings below ) . ... Translate Abstract . ... Bispectrum speckle interferometry and future long-baseline interferometry of the carbon star IRC+10216 . ... 2003SPIE.4838.1055B We present near-infrared (JHK) bispectrum speckle-interferometry monitoring of IRC+10216 obtained with the SAO 6m telescope. The present speckle observations covering baselines up to 6m provide important complementary informations for future long-baseline interferometry. ...

Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...