45 research outputs found
1861-08-17 John H. Quimby requests payment of bill of Captain S.M. Fuller
https://digitalmaine.com/cw_me_4th_regiment_corr/1066/thumbnail.jp
1861-07-18 John H. Quimby requests payment of invoice
https://digitalmaine.com/cw_me_4th_regiment_corr/1057/thumbnail.jp
1861-07-25 John H. Quimby requests payment of bill submitted to Captain Silas Fuller
https://digitalmaine.com/cw_me_4th_regiment_corr/1058/thumbnail.jp
The Sloan Digital Sky Survey-II Supernova Survey: Search Algorithm and Follow-up Observations
The Sloan Digital Sky Survey-II Supernova Survey has identified a large
number of new transient sources in a 300 sq. deg. region along the celestial
equator during its first two seasons of a three-season campaign. Multi-band
(ugriz) light curves were measured for most of the sources, which include solar
system objects, Galactic variable stars, active galactic nuclei, supernovae
(SNe), and other astronomical transients. The imaging survey is augmented by an
extensive spectroscopic follow-up program to identify SNe, measure their
redshifts, and study the physical conditions of the explosions and their
environment through spectroscopic diagnostics. During the survey, light curves
are rapidly evaluated to provide an initial photometric type of the SNe, and a
selected sample of sources are targeted for spectroscopic observations. In the
first two seasons, 476 sources were selected for spectroscopic observations, of
which 403 were identified as SNe. For the Type Ia SNe, the main driver for the
Survey, our photometric typing and targeting efficiency is 90%. Only 6% of the
photometric SN Ia candidates were spectroscopically classified as non-SN Ia
instead, and the remaining 4% resulted in low signal-to-noise, unclassified
spectra. This paper describes the search algorithm and the software, and the
real-time processing of the SDSS imaging data. We also present the details of
the supernova candidate selection procedures and strategies for follow-up
spectroscopic and imaging observations of the discovered sources.Comment: Accepted for publication in The Astronomical Journal (66 pages, 13
figures); typos correcte
The Fast, Luminous Ultraviolet Transient AT2018cow: Extreme Supernova, or Disruption of a Star by an Intermediate-Mass Black Hole?
Wide-field optical surveys have begun to uncover large samples of fast
(t_rise < 5d), luminous (M_peak < -18), blue transients. While commonly
attributed to the breakout of a supernova shock into a dense wind, the great
distances to the transients of this class found so far have hampered detailed
investigation of their properties. We present photometry and spectroscopy from
a comprehensive worldwide campaign to observe AT2018cow (ATLAS18qqn), the first
fast-luminous optical transient to be found in real time at low redshift. Our
first spectra (<2 days after discovery) are entirely featureless. A very broad
absorption feature suggestive of near-relativistic velocities develops between
3-8 days, then disappears. Broad emission features of H and He develop after
>10 days. The spectrum remains extremely hot throughout its evolution, and the
photospheric radius contracts with time (receding below R<10^14 cm after 1
month). This behaviour does not match that of any known supernova, although a
relativistic jet within a fallback supernova could explain some of the observed
features. Alternatively, the transient could originate from the disruption of a
star by an intermediate-mass black hole, although this would require
long-lasting emission of highly super-Eddington thermal radiation. In either
case, AT2018cow suggests that the population of fast luminous transients
represents a new class of astrophysical event. Intensive follow-up of this
event in its late phases, and of any future events found at comparable
distance, will be essential to better constrain their origins.Comment: Corrected Figure 8 / Table 4 to use final fits. Includes
machine-readable photometry table (hopefully for real this time
1861-08-17 John H. Quimby requests payment of bill of Captain S.M. Fuller
https://digitalmaine.com/cw_me_4th_regiment_corr/1066/thumbnail.jp
1861-07-25 John H. Quimby requests payment of bill submitted to Captain Silas Fuller
https://digitalmaine.com/cw_me_4th_regiment_corr/1058/thumbnail.jp
1861-07-18 John H. Quimby requests payment of invoice
https://digitalmaine.com/cw_me_4th_regiment_corr/1057/thumbnail.jp
1863-02-16 John H. Quimby recommends Sergeant Russell H. White for promotion
https://digitalmaine.com/chamberlain_corr/1322/thumbnail.jp
Richard Schindler Collection 1938-1980
The collection contains Richard Schindler's article "Principles of a New Therapy with High Speed Electrons," accompanied by correspondence
concerning the article and Schindler's related research.Physician, born 1891 in Strassburg. Emigrated from Germany to the United States in 1935.The original inventory is available in the folderProcessed for digitizationSent for digitizationReturned from digitizationLinked to online manifestationdigitize