added feedback materials

This commit is contained in:
caes 2017-04-20 10:18:16 -04:00
parent 4e4a71ed99
commit 0be46082fc
20 changed files with 88 additions and 0 deletions

View File

@ -673,3 +673,80 @@ url = {http://www.engineeringtoolbox.com/air-density-specific-weight-d_600.html}
@ARTICLE{1997A&A...326..924M,
author = {{Matsakis}, D.~N. and {Taylor}, J.~H. and {Eubanks}, T.~M.},
title = "{A statistic for describing pulsar and clock stabilities.}",
journal = {\aap},
keywords = {TIME, PULSARS:GENERAL, PULSARS: INDIVIDUAL: PSR B1937+21, PSR B1855+09},
year = 1997,
month = oct,
volume = 326,
pages = {924-928},
adsurl = {http://adsabs.harvard.edu/abs/1997A%26A...326..924M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@INPROCEEDINGS{2000dhst.conf...65M,
author = {{Mignani}, R.~P. and {Caraveo}, P.~A. and {de Luca}, A.},
title = "{HST As a Powerful Astrometric Tool for Pulsar Astronomy}",
booktitle = {A Decade of HST Science : Poster Papers},
year = 2000,
eprint = {astro-ph/0009033},
editor = {{Livio}, M. and {Noll}, K. and {Stiavelli}, M.},
pages = {65},
adsurl = {http://adsabs.harvard.edu/abs/2000dhst.conf...65M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2001ApJ...546.1159K,
author = {{Kaaret}, P. and {Marshall}, H.~L. and {Aldcroft}, T.~L. and
{Graessle}, D.~E. and {Karovska}, M. and {Murray}, S.~S. and
{Rots}, A.~H. and {Schulz}, N.~S. and {Seward}, F.~D.},
title = "{Chandra Observations of the Young Pulsar PSR B0540-69}",
journal = {\apj},
eprint = {astro-ph/0008388},
keywords = {Stars: Pulsars: General, Stars: Pulsars: Individual: Alphanumeric: PSR 0540-69, Stars: Neutron, ISM: Supernova Remnants, X-Rays: Stars},
year = 2001,
month = jan,
volume = 546,
pages = {1159-1167},
doi = {10.1086/318287},
adsurl = {http://adsabs.harvard.edu/abs/2001ApJ...546.1159K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2010MNRAS.409..619K,
author = {{Keith}, M.~J. and {Jameson}, A. and {van Straten}, W. and {Bailes}, M. and
{Johnston}, S. and {Kramer}, M. and {Possenti}, A. and {Bates}, S.~D. and
{Bhat}, N.~D.~R. and {Burgay}, M. and {Burke-Spolaor}, S. and
{D'Amico}, N. and {Levin}, L. and {McMahon}, P.~L. and {Milia}, S. and
{Stappers}, B.~W.},
title = "{The High Time Resolution Universe Pulsar Survey - I. System configuration and initial discoveries}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1006.5744},
primaryClass = "astro-ph.HE",
keywords = {pulsars: general},
year = 2010,
month = dec,
volume = 409,
pages = {619-627},
doi = {10.1111/j.1365-2966.2010.17325.x},
adsurl = {http://adsabs.harvard.edu/abs/2010MNRAS.409..619K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

View File

@ -0,0 +1 @@
,caes,aquileia,20.04.2017 01:26,file:///mnt/sdd_500GB/home/caes/.config/libreoffice/4;

Binary file not shown.

After

Width:  |  Height:  |  Size: 1.9 MiB

Binary file not shown.

After

Width:  |  Height:  |  Size: 1.5 MiB

Binary file not shown.

After

Width:  |  Height:  |  Size: 768 KiB

Binary file not shown.

After

Width:  |  Height:  |  Size: 413 KiB

Binary file not shown.

After

Width:  |  Height:  |  Size: 485 KiB

Binary file not shown.

Binary file not shown.

After

Width:  |  Height:  |  Size: 44 KiB

Binary file not shown.

Binary file not shown.

After

Width:  |  Height:  |  Size: 196 KiB

Binary file not shown.

After

Width:  |  Height:  |  Size: 432 KiB

Binary file not shown.

After

Width:  |  Height:  |  Size: 39 KiB

Binary file not shown.

Binary file not shown.

Binary file not shown.

View File

@ -0,0 +1,10 @@
Quasars and the Birth & Evolution of Galaxies
It was on February 5, 1963 (just 8 days before my birth) that astronomer
Maarten Schmidt ran through the hallways of Caltech announcing that
he had discovered the high redshift nature of quasars, then known only
as mysterious points of light recently identified in radio surveys. In
the interim period our understanding of their place in the universe has
gone from that of isolated, ultraluminous freaks of nature to crucial
links in the birth and evolution of massive galaxies. I will present an
overview of these very recent and dramatic developments.