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1. Clear Sky Chart ? Amateur Astronomers Association of New York
... Home Observing Clear Sky Chart . ... Lecture Series 2014-2015 . ... AAA Fall Astronomy Class: Astronomy Basics тАУ October-November 2015 . ... Clear Sky Chart . This Month's Sky . ... This MonthтАЩs Sky тАУ April 2015 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...
[ Сохраненная копия ]  Ссылки http://www.aaa.org/observing/clear-sky-chart/ -- 96.1 Кб -- 10.04.2016
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2. The XTE Data Finder (XDF)
... Table of Contents - Index - PS reprint - PDF reprint . ... All RXTE telemetry will be archived in a hierarchical database consisting entirely of FITS Binary Tables. We describe an interactive tool, the XTE Data Finder (XDF). ... Our basic design contains a three level hierarchy: Master Index, Subsystem Index, and Data Table. ... The Master Index acts as an observation catalog with references to Subsystem Indices, while the latter contain configuration information and references to the Data Tables. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/rotsa.html -- 9.2 Кб -- 23.06.1998
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3. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... Min . ... 2MASS J16480306-6715178 . ... The variable star catalogued as ASAS 164802 6715.2 by Pojmanski (2002) was found to display two types of eclipsing variability by Pilecki and Szczygiel (2007). ... The comparison stars (identified in the finding chart) used were: . ... The data for Star A and B has been obtained using Comp Star 2 between HJD 2455709.956 and 2455710.089 and between 2455718.005 and 2455718.096. All other data was obtained using Comp Star 1. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1253592 -- 12.3 Кб -- 30.12.2011
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4. Remnant Molecular Clouds in the Ori OB 1 Association
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Remnant Molecular Clouds in the Ori OB 1 Association . ... A list is presented of about 80 objects of these remnant clouds in the Ori OB 1 association. ... We suspect that retarded star formation in remnant clouds can explain the presence of so-called dispersed T Tau stars in the peripheries of OB associations. ... ISM: molecular clouds - ISM:globules - HII regions - OB associations . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/ogura/paper/index.html -- 51.5 Кб -- 08.04.2016
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5. A CS and NH3 Survey
... 205Anglada+ 0) and NH3(1,1) observations towards 172 different star forming regions (99 observed in both molecules) associated with H2O maser emission. We make a comparative study between the physical parameters obtained from the CS and NH3 spectra, and their relationship with the H2O maser emission. ... We find that both the CS and the NH3 lines are significantly wider in regions with H2O masers than in other regions. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/H2O_masers.html -- 2.8 Кб -- 18.03.2015
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6. Whatcom Association Of Celestial Observers, Waco, AstroGuide Listing
The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Whatcom Association of Celestial Observers is a community based society dedicated to preserving the arts and skills of amateur astronomy. ... Listed Since January 29, 1999 . ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/astroguide/ag532.html -- 12.4 Кб -- 09.04.2016
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7. SN 1989B Light Curve Analysis.
SN 1989B Light Curve Analysis. ... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... The observations were inserted against the V magnitude templete of BL, CCD photometric data, (Wells et. al, (1994) and a color trend (B-V) histogram of the mean type Ia SN (BL)(nutemp.gif). Key Words: Amateur Observations, Supernova, Magnitude Estimates, 1989B . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/analysis.htm -- 5.1 Кб -- 02.02.2012
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8. HST Observer Monthly
... HST . ... Missions . ... Data . ... Future Missions and . ... Missions Office . ... HST Peer Review Process . ... HST Overview . Overview . ... Servicing Missions . ... Cycle 24 Announcement . ... Retrieving HST Data . ... While long-duration gamma-ray bursts (LGRBs) result from the collapse of massive stars, the progenitors of short-duration gamma-ray bursts (SGRBs) are still unknown. Although SGRBs are widely thought to result from the in-spiral of compact binaries, this is a conjecture. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/observermonthly/2012/apr2 -- 15.5 Кб -- 10.04.2016
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9. http://hea-www.harvard.edu/~slane/psr/ps/asca2.ps
ROSAT OBSERVATIONS OF PSR 0355+54 and PSR 1642--03 1 Patrick Slane Harvard­Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA 02138 USA ABSTRACT PSR 0355+54 and PSR 1642--03 are both radio pulsars whose X­ray behavior was left unresolved by Einstein observations. 1;2 In each case, faint emission was detected near the sources, but appeared to be concentrated 1--2 arcmin from the known pulsar positions. ... Seward, F. D., & Wang, Z­R 1988, ApJ, 332, 199 3. ... 1993, ApJ, 413, L27 7. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~slane/psr/ps/asca2.ps -- 59.7 Кб -- 31.01.2011
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10. Abstract
Close binary systems of the RS CVn and Algol type are characterized by a highly variable radio emission, from typical flux densities of a few mJy during low-activity (quiescent) periods, up to 1 Jy during strong flares. The origin of this radio emission is attributed to the gyrosynchrotron mechanism. Several observations of these stars have shown an evolution of the radio spectrum during both the rising and decay phases of flares. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~francio/tesi/abstract.html -- 3.2 Кб -- 23.05.1997
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11. SN1989B in M66
... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... 10 (IAUC # 4742) 2/25 13.3 16 j 2/27 13.5(*) 18 lc 2/28 13.8 19 p 3/1 13.2 20 w 3/2 13.5 21 a 3/4 13.8 23 p 3/6 13.3 25 c 3/7 13.3 26 c 3/8 14.1 27 m 3/8 13.3 27 r 3/9 13.4 28 c 3/9 14.1 28 m 3/10 13.6 29 j 3/10 14.0 29 a 3/11 13.6 30 c 3/11 13.5 30 r 3/11 13.7 30 s 3/13 [13.69 CCD Mag.] ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/snimages/sn1989b.html -- 9.7 Кб -- 22.12.2007
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/SNIMAGES/sn1989b.html -- 9.7 Кб -- 10.04.2016
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12. http://www.naic.edu/vscience/schedule/tpfiles/TaylortagP1770tp.ps
Proposal Identi cation No.: P1770 Date Received: 2003-Feb-03 14:04:19 Technical Page Proposal Type: Regular General Category: Pulsars Observation Category: Galactic Total Time Requested: 57 Hours Proposal Title: Relativistic Measurements of Binary Pulsar B1913+16 ABSTRACT: The binary pulsar B1913+16 continues to be an excellent laboratory for the study of relativistic gravitation. ... This proposal requires Iridium RFI protection at 1612 MHz between 10pm and 6am EST. ...
[ Текст ]  Ссылки http://www.naic.edu/vscience/schedule/tpfiles/TaylortagP1770tp.ps -- 99.1 Кб -- 19.04.2004
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13. NICMOS Observes the Galactic Center
Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node25.html -- 12.9 Кб -- 12.06.2006
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14. Sub-mm and radio observations of water maser sources
... I have undertaken a limited survey of water maser sources in the sub-mm continuum. ... Source selection . ... We have defined such a sample using the Arcetri catalogues of Comoretto et al. (1990) and Brand et al. (1994) , and have observed 44 of these sources in continuum (and in some cases at also), using the 15-m JCMT . ... 1994) . ... This source is interesting in that it is one of only two sources in the sample where the water maser is not associated with the sub-mm dust emission. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/jenness/jenness.html -- 18.3 Кб -- 08.12.2003
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15. Marina Rejkuba's Web Site
... Research . ... Ljubljana Univ., ... Zagreb Univ., ... Asiago Observatory, Italy . ... ESO, Germany . ... I am an associate astronomer at the European Southern Observatory (ESO). I divide my work between the scientific research and management of the ESO's User Support Department (USD), which is in charge of providing support to observers who use ESO's Paranal Observatory facilities . ... A final standard disclaimer: the opinions expressed in this site do not reflect in any way the opinions of ESO. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~mrejkuba/ -- 6.5 Кб -- 16.05.2015
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16. Abstract 204
In the literature, there is an ambiguity pertaining to the existance of a far-IR excess in RS CVn systems. ... We found 72 acceptable detections in the 12mu band, and 40 in the 25mu band (50% more than the IRAS Point Source Catalog). ... Furthermore, at the higher wavelength bands the IRAS angular resolution drops from 0.5 arcmin at 12mu to 2 arcmin at 100mu and the background becomes very complex so one cannot be certain about the origin of the observed flux. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract197.html -- 2.9 Кб -- 16.08.1996
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17. Observers
Observation data to which modern planetary ephemerides can be adjusted . Date is time of signal emission!, as contrasted to American radar ranging . where date is time of signal reception. Frequensy is 769.42875 MHz 1962-1986 . ... Coordinates of stations in Eupatoria, Crimea . ... station 8 . ... Observational Data to which DE/LE ephemerides are adjusted http://ssd.jpl.nasa.gov/?eph_data . This page is supplied by Elena Pitjeva; please send commentaries to: evp@quasar.ipa.nw.ru . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LEA/ENG/rrr.html -- 4.7 Кб -- 09.04.2016
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18. http://zebu.uoregon.edu/~uochep/talks/talks03/lscv2.pdf
Astrophysical implications of external triggers, GRB030329 in particular External Triggers subgroup · · GRB astrophysics is still very uncertain Associated GW emission: even more uncertain Interpret our observations in the simplest terms Easy to re-cast in terms of specific models Provides some astrophysical context which is readily interpretable Probable: The GRB field will need GW observations to fully understand GRB progenitor astrophysics Nov 10, 2003 Frey 1 Short and Long GRBs.. ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/talks/talks03/lscv2.pdf -- 207.1 Кб -- 12.10.2004
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19. The Sun -- History
Large sunspots were occasionally seen far in the past without any instruments, when the sun was dimmed by thick haze, but not much was remembered of those observations. ... Sunspot Cycle (1850 - 1975) . One who was greatly influenced by Schwabe's discovery was an English gentleman of independent means, Richard Christopher Carrington , who devoted himself to the study of sunspots. ... Carrington had seen a flare, of the rare variety that is visible in white light (only about 50 are known). ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/whsun.html -- 8.0 Кб -- 15.03.1999
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20. Observers Instructions for filling out the ARCSAT nightlog
... The schedule assigned id (example: AS05) for your observing program. ... Use the time you started using the telescope including when you started taking calibrations. The time you opened for on sky observations can be entered later in the activity log. UTC End Time: . ... Focus Log: . ... The focus position can be obtained under the Telescope column of the System Status in ACP or from the run log. ... When all fields are filled out press this button to email the log to the ARCSAT and community. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObservingAids/nightlogInstructions.html -- 5.9 Кб -- 16.05.2014
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