Next: Adding plot classes Up: Plotting Previous: Plotting Contents . Plot variables are identified by a sequence number in , and are defined in terms of data variables in set_plotdata (and the corresponding function set_ploterr . ... The following additional information needs to be entered for each plot variable. Each plot variable's ID is entered in set_plotlabels for the index label it requires so that it is displayed together with the name in the plots. ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Equatorial coronal hole (top left), polar CH (top right), quiet Sun (bottom left) and quiet Sun with TCHs (bottom right) with the positions of all the corresponding identified brightening pixels over-plotted. ... We found that in comparison to the quiet Sun, the boundaries of coronal holes are abundant with brightening events including areas inside the coronal holes where closed magnetic field structures are present. ...

Radio data are displayed in the following format: . After the title with name of cluster under examination and with line about kind of data under one, e.g. Radio data [ optical data ] [ radio source identifications ] [ radio spectra (1.0 or 1.1) ] . ... The first line contains the number of radio sources associated with the cluster (these are just those sources with entries in sections 'Radio galaxy', 'Radio source' and 'Radio spectrum' below). ... Radio sources in cluster: 2 # . ...

Next: References Up: No Title Previous: Observational data and reduction . ... A minor loss of information is due to the overestimation of the scattered light in the region of and to the broad emission lines and . On the diagrams are shown the blue-shifted absorption lines and the interstellar diffusion bands. ... In Table 1 are given only emission lines. Questionable features and the lines that fell within the gaps are not included in it, question-marks are for unreliable identification. ...

... General Catalog of Variable Stars (GCVS database, Version 2012 Feb.) ... The cross-identification tables of the General Catalogue of Variable Stars (GCVS) contain all GCVS (including extragalactic variables from vol.V), NSV (New catalogue of Suspected Variable stars) and Supplement to the NSV stars as well as stars from the name-lists of variable stars nos. 67 - 80; it also makes it possible to find out identifications between the GCVS and the NSV catalogue. ... I-III) names are included. ...

OPTICAL IDENTIFICATIONS OF INTEGRAL / RXTE SOURCES WITH 1.5-METER OPTICAL TELESCOPE RTT150 I.Bikmaev (1,2), M.Revnivtsev (3,4) , R.Burenin (3) R.Sunyaev (3,4) , N.Sakhibullin (1,2) (1) Kazan State University, Kremlevskaya Str., ... 1, D-85741, Garching bei MЭnchen , Germany (3 (4) ABSTRACT We present the first results of our project on optical identifications of INTEGRAL / RXTE hard X-ray sources by using scientific instrumentations of the 1.5meter joint Russian-Turkish optical telescope RTT150. ...

Name: GRSLCT Purpose: select active output device Category: GRAPHICS File: pgplot.src Author: T.J. Pearson Use: see description below. Description: SUBROUTINE GRSLCT (IDENT) GRPCKG: Check that IDENT is a valid plot identifier, and select the corresponding plot as the current plot. All subsequent plotting will be directed to this device until the assignment is changed by another call to GRSLCT. ... Updates: Oct 16, 1998: JPT automatically extracted from source. ...

Proposal Identification No.: ... Section IV - RFI Considerations 2 Frequency Ranges Planned 300 - 350 Section V - Observing List Target List 00:31:06.0 01:02:12.7 02:39:32.8 03:12:48.7 03:18:01.9 03:38:16.7 03:41:51.7 04:31:33.5 05:16:47.9 05:26:38.1 06 ... 07:11:38 06:12:48 10:13:29 15:48:36 01:31:12 06:32:31 12:12:43 35:55:47 36:52:56 12:13:13 26:05:07 07:02:53 07:07:24 Fermi2FGL 2FGL 2FGL 2FGL 2FGL 2FGL 2FGL 2FGL 2FGL 2FGL 2FGL 2FGL ...

Chapter 2: Header Keyword Definitions . ... T/F- Was the observation an association? ... Looking at the ASN_MTYP and EXPNAME keywords for each extension of the n48o06020_jif.fits file, we see... n48o06020_jif.fits [1], ASN_MTYP = EXP-TARG EXPNAME = N48O06G9J n48o06020_jif.fits [2], ASN_MTYP = EXP-TARG EXPNAME = N48O06GAJ n48o06020_jif.fits [3], ASN_MTYP = EXP-BCK1 EXPNAME = N48O06GBJ n48o06020_jif.fits [4], ASN_MTYP = EXP-BCK1 EXPNAME = N48O06GCJ n48o06020_jif.fits [5], ...

... Tonight's Sky . ... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . ... Moon . ... The Magazine . ... Observing . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... More UFOs identified . ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter....

Peremennye Zvezdy", . ... Coordinates (J2000): . ... They were discovered by Hoffmeister (1964) from Sonneberg plates as S 8283 and S 8284, respectively. ... However, no star patterns resembling Hoffmeister's finding charts were found for these stars by Skiff (1999) who had successfully identified all the other stars from Hoffmeister (1964). ... a: A 5'x5' DSS finding chart for EV Cep, with the chart for S 8283 Cep from Hoffmeister (1964) inserted; b: same for EW Cep and S 8284 Cep (insert). ...

DIS-III Spectra Other information . ... LOW Blue . ... MED Blue . ... HIGH Blue . ... Lines / mm . ... 5.03е /pix . 2.43е /pix . 2.26е /pix . 1.23е /pix . 0.84е /pix . 0.62е /pix . ... 7.0 е /pix . 3.05е /pix . 3.15е /pix . ... 1.17е /pix . ... Spacial scale for Blue gratings are: 0.42 arc-sec/pixel . ... 300 lines/mm . Low Blue . ... Med Blue . ... 0.9 " slit . ... unidentified . ... Offset Directions for DIS Using Various Interfaces as viewed by the Slit Camera . ...

Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...

FLAMES multiobject spectroscopy of low mass stars in the "twin" young clusters Ori andOri 1,2 1 3 G.G. Sacco , R. Pallavicini , S. Randich , 1 3 E. Franciosini , F. Palla 1 INAF Osservatorio Astronomico di Palermo, Italy 2DSFA UniversitЮ di Palermo, Italy 3 INAF ­Osservatorio Astrofisico di Arcetri, Italy ABSTRACT Using FLAMES on VLT/UT2, we obtained spectra of 147 lowmass candidate members of the two young (~5 Myr) and coeval clusters Ori and Ori. ... Results: In Ori we identified 65 members. ...

... are preliminary IAU-style names for ChaMP objects. Finalization of names awaits the final systematization of optical coordinates and source identification. ... The yellow regions highlight atmospheric telluric bands at ~6900A and ~7600A. The optical ID, X-ray ID, classification, and redshift are given at the top of each plot, and a series of lines are shown that are often found in sources of that given classification. ... HS limit? ... g' band magnitude; calibrated SExtractor Kron mag or limit . ...

Next: Analysis Tools for Nebular Emission Lines . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... The direct image is used to locate objects of interest, to find the position of the appropriate spectra in the grism image, to determine the optimal extraction technique to use, and to calibrate the wavelength range of the extracted spectra. ... Figure 1: The NICMOSlook User Interface . ...

Catalogue of eclipsing variables (CEV) is the world's principal database of eclipsing binary systems with available classification. CEV contains identifications, classifications, photometry, periods, eclipses data, spectral types, references and notes for 7179 systems. Format of the current CEV . CEV main table (~1.0MB) . ... List of systems, erroneously classified as eclipsing binaries in GCVS (they are not included in the CEV main table) Download all files as a single archive (~0.6MB) . ...

On the problem of using of the ICRF radio coordinates reference system Lipovka A.A. (1), Lipovka N.M. (1) Center of research for physics, Sonora State University e-mail: nila_lip@mail.ru Bibliography 1. ... Columns 8, 9 are corrections to right ascension and declination, which should be added to coordinates of ICRF2 radio sources, to obtain coordinates of optical objects, with which these radio sources are identified. ... Lipovka .. ... Fig 3 Fig 3 ...

... LOGIC OF THE MASTER SIGNAL . ... SELECTION OF EVENTS BASED ON THE DRIFT CHAMBERS DATA . ... CYGAM, unlike the traditional telescopes, does not have a special energy detector and can not measure energy of each registered photon. ... The physical processes responsible for the high energy gamma-ray emission can not result in narrow lines or sharp irregularities in the energy spectra of compact sources for revelation of which good energy resolution is needed. ... CYGAM (PDF, 450 Kb) . ...

... Recognition of Anomalous Events S. Monai 1,2 and F.Pasian 2 1 Osservatorio Astronomico di Brera Merate, Italy 2 Osservatorio Astronomico di Trieste, Italy Abstract. We present an original algorithm for the recognition of anomalous events in a CCD frame (i.e., cosmic hits, bad pixels etc.) ... Raw images, as read from a CCD, are often a#ected by some events which are revealed by anomalous pixel values, i.e., single saturated pixels or pixels at zero intensity (also named hot or bad pixels). ...