Search Results for 'redshift'

redshift published presentations and documents on DocSlides.

SDSS-II SN survey:
SDSS-II SN survey:
by lindy-dunigan
Constraining Dark Energy with intermediate-. reds...
Watching Galaxies Form Near the Beginning of Time
Watching Galaxies Form Near the Beginning of Time
by alida-meadow
The Cosmic Time Machine. Astronomical telescopes ...
Cosmology,   lect.
Cosmology, lect.
by messide
5. Curved Cosmos. & . Observational Cosmology....
Ambulance analogy First the pitch became higher, then lower.
Ambulance analogy First the pitch became higher, then lower.
by sherrill-nordquist
Originally discovered by the Austrian mathematici...
HI Stacking:
HI Stacking:
by liane-varnes
Past, Present and Future. HI Pathfinder Workshop....
Redshift
Redshift
by faustina-dinatale
Lesson Objectives. To understand toast Doppler pr...
Why would you want accurate quasar redshifts?
Why would you want accurate quasar redshifts?
by liane-varnes
Paul Hewett (. IoA. , Cambridge). James Allen (U....
GRAVITATIONAL REDSHIFTS
GRAVITATIONAL REDSHIFTS
by sherrill-nordquist
versus convective . blueshifts. , and wavelength...
Cluster views of the high redshift universe
Cluster views of the high redshift universe
by tatiana-dople
Leonidas . Moustakas. , JPL/Caltech. CLASH London...
Gravitational
Gravitational
by myesha-ticknor
Redshift. in Clusters of Galaxies. Marton Trencse...
Tailoring
Tailoring
by faustina-dinatale
Strong . L. ensing . C. osmographic . O. bservati...
Gravitational Lensing
Gravitational Lensing
by cheryl-pisano
and. Quasars . “A man should look for what is, ...
Big Bang
Big Bang
by pamella-moone
vs. Creation. Christopher W. Ashcraft M.S., M.E...
Radio faint GRB afterglows
Radio faint GRB afterglows
by marina-yarberry
Sydney Institute for Astronomy (. SIfA. )/ CAASTR...
GRBs as cosmological probes
GRBs as cosmological probes
by lois-ondreau
Thomas Krühler (DARK). Thanks to J. . Fynbo. , D...
Inefficient on the Redshift side of things
Inefficient on the Redshift side of things
by aaron
Only works with STRING and NUMBER types Decide wh...
Tracing HI gas within dust-reddened quasars with
Tracing HI gas within dust-reddened quasars with
by liane-varnes
ASKAP. Marcin Glowacki. Supervisors: Elaine Sadle...
The Cosmos & the Bible
The Cosmos & the Bible
by ellena-manuel
Looking at Modern Cosmologies. Robert C. Newman. ...
Spatially Resolving the Kinematics of the
Spatially Resolving the Kinematics of the
by tatyana-admore
. Quasar Broad Line Region . using . Spectro. -...
The KMOS Redshift One Spectroscopic Survey (KROSS):
The KMOS Redshift One Spectroscopic Survey (KROSS):
by kittie-lecroy
The Evolution of the Tully-Fisher Relation Since ...
The HI gas content of galaxies
The HI gas content of galaxies
by yoshiko-marsland
around Abell 370, . a galaxy cluster at z = 0.37....
Dalefest
Dalefest
by mitsue-stanley
!. Donna Kubik. Rolfsenfest. . CIRM 2013. Interd...
The Build-up of Quasars
The Build-up of Quasars
by ellena-manuel
Gordon Richards. Drexel University. With thanks t...
Non-parametric Determination of Luminosity Evolutions, Corr
Non-parametric Determination of Luminosity Evolutions, Corr
by ellena-manuel
Jack . Singal. University of Richmond. Stat. . Ch...
ESO Recent Results on
ESO Recent Results on
by giovanna-bartolotta
Reionization. . Chris . Carilli (NRAO). LANL Cos...
Z-Spec results
Z-Spec results
by jane-oiler
April 2008. 7.9 hours. half . t. ~0.5, half . t...
X- Spec:
X- Spec:
by myesha-ticknor
Multi-Object Survey . Spectroscopy with . CCAT. M...
SF  timescale   from  [ alpha
SF timescale from [ alpha
by ceila
/Fe]. SNII . release. . most. . alpha. –. ele...
Detection of H-alpha emission from
Detection of H-alpha emission from
by myesha-ticknor
z. >3.5 galaxies with. AKARI-FUHYU NIR spectro...
Magnitudes and Redshifts of S
Magnitudes and Redshifts of S
by briana-ranney
1 From upernovae , their Light - Curves, and Ang...
Summary of Previous Day
Summary of Previous Day
by cheryl-pisano
Science. is limited to observing nature and expl...
Hawking radiation, infinite redshifts, and black hole analo
Hawking radiation, infinite redshifts, and black hole analo
by test
Ted Jacobson. University of Maryland. Gravity and...
X-Spec: a Multi-Object Wideband Spectrograph for CCAT:
X-Spec: a Multi-Object Wideband Spectrograph for CCAT:
by conchita-marotz
Concept and Technology Development. © . 2013. CC...
The Universe This is a spiral galaxy with other galaxies in the background. The universe is “ever
The Universe This is a spiral galaxy with other galaxies in the background. The universe is “ever
by sherrill-nordquist
The universe is a big place, perhaps the biggest....
Timeline  Cosmology
Timeline Cosmology
by conchita-marotz
2nd Millennium BCE. BC. . . Mesopotamian ...
The Universe This is a spiral galaxy with other galaxies in the background. The universe is “ever
The Universe This is a spiral galaxy with other galaxies in the background. The universe is “ever
by conchita-marotz
The universe is a big place, perhaps the biggest....
1 Cosmology with  Supernovae:
1 Cosmology with Supernovae:
by pasty-toler
Lecture 1. Josh . Frieman. I Jayme . Tiomno. Sch...
Thomas Prevenslik QED Radiations
Thomas Prevenslik QED Radiations
by hondasnoopy
Hong Kong and Berlin. Dust and . the Origin of the...
The Slit-Less Spectroscopic Survey of Galaxies (SPICY) with
The Slit-Less Spectroscopic Survey of Galaxies (SPICY) with
by collectmcdonalds
AKARI/IRC – perspective to SPICA. T. . Wada, . Y...