List of Amateurs Discoverers of SNe. The following list shows amateurs who have discovered or co-discovered a supernova . ... For each discoverer we indicate the number of supernovae found, the number of co-discoveries (i.e., shared with other observers), the method used (V=visual, P=photographic and C=ccd), the first and last years of his discoveries and country of origin. ... DISCOVERER NAME . No.SNe . ... U.S.A. Evans . ... 1996-01 . ... Japan . ... Italy . ... 1994-98 . ... 2001 . ...

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• APOD: 2015 May 31 - Supernova 1994D and the Unexpected Universe
• APOD: April 11, 1996 - Unexpected X-rays from Comet Hyakutake
• APOD: 2006 March 6 - Unexpected Comet Pojmanski Now Visible

... Unexpected X-rays from Comet Hyakutake . ... 11.04.1996 . ... Credit: C. Lisse, M. Mumma (NASA/GSFC), K. Dennerl, J. Schmidt, and J. Englhauser (MPE) Explanation: The first X-rays ever detected from a comet were discovered from Comet Hyakutake with the ROSAT satellite on March 27th. ... Information: The Scale of the Universe Debate in April 1996 . ... March . ... Publications with keywords: comet - comet Hyakutake . Publications with words: comet - comet Hyakutake . ... Comet Holmes Over Hungary . ...

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• Астронет > Unexpected X-rays from Comet Hyakutake
• Unexpected Comet Pojmanski Now Visible
• An Unexpected Flare from the Crab Nebula

Proposal Identification No.: ... 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: Regular Pulsars Galactic 27 9 0 1 hour 100-500 GB Further Follow-up of Interesting Pulsars Discovered in the Arecibo 327 MHz Drift Scan Survey ABSTRACT: We propose to use 36 hours of Arecibo ...

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• http://www.naic.edu/vscience/schedule/2013Spring/StovalltagP2790.pdf
• http://www.naic.edu/vscience/schedule/2013Fall/BarrtagP2817.pdf
• http://www.naic.edu/vscience/schedule/2013Fall/StovalltagP2825.pdf

Supernova 2000cl in NGC 3318 This page is devoted to information on Supernova 2000cl in NGC 3318 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the Supernova links web page. ... Robin Chassagne's Supernova in NGC 3318 web page in French [ Translate ] . ... Robin Chassagne image . ... and Lidman image . ... vsnet-alert 4896 ] SN 2000cl in NGC 3318 . ...

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• Supernova 1999dq in NGC 976
• Supernova 1999ev in NGC 4274
• Supernova 2002bx in IC 2461

Detected Supernovae . The search have produced till now the detections of 4 SNe. ... This result highlights the power of infrared monitoring in detecting Obscured SNe and indicates that optical surveys are probably missing a significant fraction of SNe, especially in obscured systems such as starburst galaxies. ... In Fig. we show the archival SOFI image of NGC3256 (left) and the first image obtained in 2001 (right) where SN2001db has been detected. ...

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• APOD: 2000 March 12 - Supernova 1994D and the Unexpected Universe
• APOD: December 30, 1998 - Supernova 1994D and the Unexpected Universe
• K-band Arcetri Obscured Supernova Search - What is the KAOSS Projrect?

Next: Observations and reduction Up: The discovery of SN1998bv Previous: The discovery of SN1998bv . ... Since the life cycle of massive stars is very short (<30Myr), one can expect to observe more or less frequent SNe in galaxies where current intensive star formation takes place. ... 1998). ... The supernova SN 1998bv was discovered on April 6, 1998 in the galaxy HS 1035+4758 selected as an ELG candidate in the HSS. ... Figure 1: DSS image of the galaxy HS 1035+4758. ...

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• Radio survey for new compact HII regions
• Conclusions

... Search . ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Visual Supernova Searching with the 40 inch Telescope at Siding Spring Observatory . ... It has been questioned whether automatic and visual searches can be compared in this way since the automatic searches have a fixed list of targets, while visual observers are likely to be biased in observing a galaxy with a known supernova. ...

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• Discovery Observations: The Fornax Spectroscopic Survey
• VSOP Observing Schedule
• First discoveries from the H survey

... WFIRST . ... Missions . ... Science . ... The design reference mission described in the Final Report of the WFIRST-AFTA Science Definition Team has two instruments to execute the mission science program : . ... The WFI will have 6 imaging filters, a grism (for redshift measurements in support of BAO science), and an Integral Field Unit (IFU) for spectroscopic characterization of supernovae. ... A three-tiered WFI supernova survey, with both imaging and IFU spectroscopy, taking a total of 0.6 years. ...

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• Future Calibrations, Calibration by Observers, and Calibration Outsourcing
• Observing with Linear Ramp Filters
• Proposing Overview

... Observing . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... First galaxies were born much earlier than expected . ... Using the amplifying power of a cosmic gravitational lens, astronomers have discovered a distant galaxy whose stars were born unexpectedly early in cosmic history. ... However, the newly discovered galaxy has dramatically different features from other distant galaxies that have been observed, which generally shine brightly with only young stars...

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• The Very Large Array finds unexpected т??stormт?? at galaxyт??s core |
• A much expected journey: How Pluto became a giant among the dwarfs |
• Bob Berman's strange universe: Expect a surprise | Astronomy.com

... INSTRUMENT: SurveyCam FILTERS: Stromgren uvby, 2" square COMMENTS: remote observations are expected BRIEF SCIENCE JUSTIFICATION: Last decade numerous faint structures at the periphery of regular galaxies, as arcs, tails, or streams, have been discovered (see e.g. Martinez-Delgado et al., ... The broad-band photometry is used for observing the faint structures, but it does not allow to break the age-metallicity degeneracy efficiently. ... The standard Stromgren set is available at APO. ... 2014). ...

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• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_feb2015/AS01.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2014/AS01.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_jan2016/AS01.html

... Images obtained using the Faulkes Telescope South, operated by Las Cumbres Observatory. ... The Faulkes Telescope Project and Las Cumbres Observatory Global Telescope Network had kindly given us the opportunity to use these telescopes and the observatory had booked us four sessions of controlling the telescope in order for us to make some observations on NEOs. ... Just before our first observing session on Friday, we were given a tour of the observatory building and its telescopes, by John McFarland...

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• Armagh Observatory
• Leonid Meteors
• Leonids 2006

Next: Conclusion Up: No Title Previous: The Transmission Gratings . ... The potential of Chandra is illustrated in Figure which shows the official "first-light" image. ... Figure: The official CXO first light image - the supernova remnant CasA. Perhaps the neutron star - black hole connection and the utility of CXO are best illustrated by an early observation of the Crab Nebula and pulsar taken as part of the HETG calibration. ... Figure shows the zeroth-order image of the Crab Nebula. ...

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• Supernova Explosions
• Discussion and conclusions
• Spatial distribution of X-ray binaries at the Galactic center after the

... ESO . ... Galaxies . ... Now, however, Dante Minniti and Albert Zijlstra [1] , working at the ESO 3.5-metre New Technology Telescope (NTT), have found a large halo of old and metal-poor stars around one of the dwarf galaxies in the Local Group. ... This does not necessarily imply that all dwarf galaxies must likewise lack halos: it is also possible that the halos of the Magellanic Clouds were stripped away when they came too close to the Milky Way sometime in the past. ... A Dwarf Galaxy With A Halo...

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• Unexpected Changes of Bright Spots on Ceres Discovered | ESO
• ESO - I see unexpected boxy emission-like features in my REDL spectra - where
• Aleksandar Cikota

... Our recent observations with the Hubble Space Telescope (August 29, 2014) led to revealing a highly isolated dwarf spheroidal galaxy KKs 3 situated at a distance of 2.12 0.07 Mpc from the Milky Way. The dSph galaxy locates on the southern sky (RA=02 h 24 m 44.4 s , Dec.= ... Over the last decade, about 30 dSph galaxies have been discovered inside the Local Group through systematic search in the vicinity of M31 and more that a dozen dSphs were discovered in the nearby group around M81. ...

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• Metagalaxy sector, archive 2007

M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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• ESO Press Release 06/96, 16 February 1996
• Astro-2 and the UIT Experiment

... Timeline . ... 16H. Schwabe, 1843 . 16a. Schwabe paper . ... The weather throughout this year was so extremely favorable that I have been able to observe the Sun clearly on 312 days; however, I counted only 34 groups of sunspots.. From my earlier observations, which I have reported every year in this journal, it appears that there is a certain periodicity in the appearance of sunspots and this theory seems more and more probable from the results of this year.. ... Year . ... 149 . ... 1843 . ...

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• The Scale of the Solar System
• Main results of the experimental and theoretical research completed in 2010
• The Sun -- History

... Timeline . ... 16H. Schwabe, 1843 . 16a. Schwabe paper . ... The weather throughout this year was so extremely favorable that I have been able to observe the Sun clearly on 312 days; however, I counted only 34 groups of sunspots.. From my earlier observations, which I have reported every year in this journal, it appears that there is a certain periodicity in the appearance of sunspots and this theory seems more and more probable from the results of this year.. ... Year . ... 149 . ... 1843 . ...

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• First X-Rays From a Comet Discovered
• The Sun -- History
• Other Solar Systems

... Home Observing Charles Dana Discovery Center, Central Park . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Charles Dana Discovery Center . ... 6:30тАУ8:00 p.m. The Charles Dana Discovery Center is just inside Central Park, near 110th Street between Lenox and Fifth avenues ( map ). ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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• Lecture Series 2010-2011 ? ?Top Ten Discoveries of the Phoenix Misson to Mars?
• Amateur Astronomers Association of New York ? Amateur Astronomers Association
• Observing Out-Of-Town ? Amateur Astronomers Association of New York

Astronotes Armagh Planetarium's Stellar Blog! ... Sun . ... There could be an eighth planet to discover! ... The orbits of the planets could be predicted perfectly- apart from Mercuryт??s. Planetary orbits are not circles, but ellipses and Mercuryт??s orbit was the least circular (or most т??eccentricт??) known. ... Vulcan, according to Le Verrier, orbited the Sun every 19.7 days at an average distance of 21 million km (0.14 au), a little over a third of Mercury?s average distance from the Sun. ...

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• Supernova spotted by Irish astronomer | Astronotes
• Neptune: discovered one year ago | Astronotes
• Supernova in the Cigar Galaxy | Astronotes

RadioAstron AO-1 prop osal Submission dead line: February 8, 23:59 UT. ... Team contact name and e-mail address: Ivan Petrov (e-mail: Ivan.Peterov@gmail.com ) Total observing time request: 100 hrs Number of independent observing segments and typical range of pro jected baselines required: 20 (3-30 Earth diameters) Specific dates and time intervals requested : If your experiment requires specific dates and UT ranges, please, indicate them: February 1, 2014: 08:00-16:00 UT -- M87 imaging ...

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• http://www.asc.rssi.ru/RadioAstron/ao-2/radioastron_ao2_proposal_template.pdf
• Contingency Plans