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Google Keyword Rankings for : sdss central wavelengths
1
SDSS Filters - SkyServer
https://skyserver.sdss.org/dr1/en/proj/advanced/color/sdssfilters.asp
The Spectrographs ; Wavelength coverage, 3800-9200 Å, 3650-10,400 Å ; Resolution, 1500 at 3800 Å, 2500 at 9000 Å ; Pixel spacing, log-wavelength (10-4 dex) ; Units ...
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https://skyserver.sdss.org/dr1/en/proj/advanced/color/sdssfilters.asp
The Spectrographs ; Wavelength coverage, 3800-9200 Å, 3650-10,400 Å ; Resolution, 1500 at 3800 Å, 2500 at 9000 Å ; Pixel spacing, log-wavelength (10-4 dex) ; Units ...
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2
The Sloan Digital Sky Survey Photometric System - NASA/ADS
https://adsabs.harvard.edu/full/1996AJ....111.1748F
SLOAN DIGITAL SKY SURVEY 1750 Note — 1) effecttve wave length. ... Colors of main sequence stars in the SDSS photometric system. (a) — g' vs g' — r' colors, ...
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https://adsabs.harvard.edu/full/1996AJ....111.1748F
SLOAN DIGITAL SKY SURVEY 1750 Note — 1) effecttve wave length. ... Colors of main sequence stars in the SDSS photometric system. (a) — g' vs g' — r' colors, ...
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3
MSWG - Filters
https://www.cfht.hawaii.edu/Science/mswg/filters.html
The u'g'r'i'z' sloan set has been selected for MegaCam. ... Temperature: Central Wavelength (CWL) and Bandwidth (BW) are specified at 0 deg. C.
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https://www.cfht.hawaii.edu/Science/mswg/filters.html
The u'g'r'i'z' sloan set has been selected for MegaCam. ... Temperature: Central Wavelength (CWL) and Bandwidth (BW) are specified at 0 deg. C.
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4
Camera - SDSS-III
https://www.sdss3.org/instruments/camera.php
Filters. SDSS-III used the same filter system as the original SDSS. The central wavelengths of the five filters are given below: ...
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https://www.sdss3.org/instruments/camera.php
Filters. SDSS-III used the same filter system as the original SDSS. The central wavelengths of the five filters are given below: ...
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5
SDSS–2MASS–WISE 10-dimensional stellar colour locus
https://academic.oup.com/mnras/article/440/4/3430/1106956
We present the fiducial main-sequence stellar locus traced by 10 ... was provided in four filters, with central wavelengths of 3.4, 4.6, 12, and 22 μm.
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https://academic.oup.com/mnras/article/440/4/3430/1106956
We present the fiducial main-sequence stellar locus traced by 10 ... was provided in four filters, with central wavelengths of 3.4, 4.6, 12, and 22 μm.
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6
Evolution of Galactic Outflows at Revealed with SDSS, DEEP2 ...
https://iopscience.iop.org/article/10.3847/1538-4357/aa956d
based on the absorption lines of optical spectra taken from SDSS DR7, ... is the optical depth at the central wavelength ${\lambda }_{0}$ ...
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https://iopscience.iop.org/article/10.3847/1538-4357/aa956d
based on the absorption lines of optical spectra taken from SDSS DR7, ... is the optical depth at the central wavelength ${\lambda }_{0}$ ...
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7
Finder Chart: Overview - IRSA/IPAC
https://irsa.ipac.caltech.edu/onlinehelp/finderchart/finderchart/overview.html
Please note that the DSS and SDSS data do not reside at IRSA, ... +Surveys, Wavelengths, and Sky Coverage ... Band, Approximate central wavelength.
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https://irsa.ipac.caltech.edu/onlinehelp/finderchart/finderchart/overview.html
Please note that the DSS and SDSS data do not reside at IRSA, ... +Surveys, Wavelengths, and Sky Coverage ... Band, Approximate central wavelength.
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8
The Photometric Camera and the CCDs
https://www.astro.princeton.edu/PBOOK/camera/camera.htm
The photometric camera for the SDSS consists of two TDI scanning CCD arrays, one, ... All the filters except u' are easy to make and have very high central ...
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https://www.astro.princeton.edu/PBOOK/camera/camera.htm
The photometric camera for the SDSS consists of two TDI scanning CCD arrays, one, ... All the filters except u' are easy to make and have very high central ...
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9
The ugrizY JHK luminosity distributions and densities ... - arXiv
https://arxiv.org/pdf/1002.3788
of LRGs whose average properties are comparable to a real SDSS red galaxy ... central wavelengths of the emission lines are constant in time and space, ...
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https://arxiv.org/pdf/1002.3788
of LRGs whose average properties are comparable to a real SDSS red galaxy ... central wavelengths of the emission lines are constant in time and space, ...
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10
Robust automatic photometry of local galaxies from SDSS
https://www.aanda.org/articles/aa/full_html/2016/07/aa27618-15/aa27618-15.html
Therefore, within the SDSS, local galaxies can be analyzed down to a mass limit ... have a central wavelength closer to the g filter central wavelength.
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https://www.aanda.org/articles/aa/full_html/2016/07/aa27618-15/aa27618-15.html
Therefore, within the SDSS, local galaxies can be analyzed down to a mass limit ... have a central wavelength closer to the g filter central wavelength.
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11
SVO Filter Profile Service
http://svo2.cab.inta-csic.es/svo/theory/fps3/index.php?id=SLOAN/SDSS.g
SLOAN :The Sloan Digital Sky Survey ... Description (?) : SDSS g full transmission ... Reference for filter response: SDSS DR7.
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http://svo2.cab.inta-csic.es/svo/theory/fps3/index.php?id=SLOAN/SDSS.g
SLOAN :The Sloan Digital Sky Survey ... Description (?) : SDSS g full transmission ... Reference for filter response: SDSS DR7.
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12
Filters | Las Cumbres Observatory
https://lco.global/observatory/instruments/filters/
› observatory › instruments › filters
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https://lco.global/observatory/instruments/filters/
› observatory › instruments › filters
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13
Photometric system - Wikipedia
https://en.wikipedia.org/wiki/Photometric_system
› wiki › Photometric_system
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https://en.wikipedia.org/wiki/Photometric_system
› wiki › Photometric_system
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14
SDSS Filter Characteristics | Download Table - ResearchGate
https://www.researchgate.net/figure/SDSS-Filter-Characteristics_tbl1_1776148
Models suggest a synchrotron spectrum in visible wavelengths and some emission in X-ray wavelengths. Of 3.7 million objects in the Sloan Digital Sky Survey ...
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https://www.researchgate.net/figure/SDSS-Filter-Characteristics_tbl1_1776148
Models suggest a synchrotron spectrum in visible wavelengths and some emission in X-ray wavelengths. Of 3.7 million objects in the Sloan Digital Sky Survey ...
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15
vik dhillon: phy217 - instruments - photometric systems
http://www.vikdhillon.staff.shef.ac.uk/teaching/phy217/instruments/phy217_inst_photsys.html
The central wavelength of the filter bandpass is known as the effective ... UBVRI photometric system was not chosen by the Sloan Digital Sky Survey (SDSS), ...
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http://www.vikdhillon.staff.shef.ac.uk/teaching/phy217/instruments/phy217_inst_photsys.html
The central wavelength of the filter bandpass is known as the effective ... UBVRI photometric system was not chosen by the Sloan Digital Sky Survey (SDSS), ...
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16
LSST Filters versus SDSS - Data Q&A
https://community.lsst.org/t/lsst-filters-versus-sdss/2429
Hi @yorkpf, thank you for your question. You are correct that the LSST has six filters, ugrizy. These bands do not exactly match the SDSS bands. For ...
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https://community.lsst.org/t/lsst-filters-versus-sdss/2429
Hi @yorkpf, thank you for your question. You are correct that the LSST has six filters, ugrizy. These bands do not exactly match the SDSS bands. For ...
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17
r SDSS c6018 | NOIRLab Science
https://noirlab.edu/science/filters/c6018
c6018 — Filter. r SDSS c6018. February 19, 2021. Comments. Note: The central wavelength of CTIO Mosaic narrow band filters (actually all filters, ...
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https://noirlab.edu/science/filters/c6018
c6018 — Filter. r SDSS c6018. February 19, 2021. Comments. Note: The central wavelength of CTIO Mosaic narrow band filters (actually all filters, ...
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18
Flux-Calibrated Emission-Line Imaging of Extended Sources ...
https://www.jstor.org/stable/10.1086/667531
present uncertainty in setting the central wavelength of TFs (∼1 Е) is the ... out by fitting the Sloan Digital Sky Survey (SDSS) griz magnitudes of ...
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https://www.jstor.org/stable/10.1086/667531
present uncertainty in setting the central wavelength of TFs (∼1 Е) is the ... out by fitting the Sloan Digital Sky Survey (SDSS) griz magnitudes of ...
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19
6.5 UVIS Spectral Elements - HST User Documentation - HDox
https://hst-docs.stsci.edu/display/WFC3IHB/6.5+UVIS+Spectral+Elements
The F850LP filter is part of the Sloan Digital Sky Survey (SDSS) griz filter set, ... Instead, the central wavelength for each filter was determined by ...
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https://hst-docs.stsci.edu/display/WFC3IHB/6.5+UVIS+Spectral+Elements
The F850LP filter is part of the Sloan Digital Sky Survey (SDSS) griz filter set, ... Instead, the central wavelength for each filter was determined by ...
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20
HIGH-RESOLUTION H-BAND SPECTROSCOPY OF Be ...
https://repositories.lib.utexas.edu/bitstream/handle/2152/34298/highresolutionhbandspectroscopy.pdf?sequence=1
HIGH-RESOLUTION H-BAND SPECTROSCOPY OF Be STARS WITH SDSS-III/APOGEE. I. ... varies with wavelength, but the central dispersions of the blue,.
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https://repositories.lib.utexas.edu/bitstream/handle/2152/34298/highresolutionhbandspectroscopy.pdf?sequence=1
HIGH-RESOLUTION H-BAND SPECTROSCOPY OF Be STARS WITH SDSS-III/APOGEE. I. ... varies with wavelength, but the central dispersions of the blue,.
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21
Seyfert 1 composite spectrum using SDSS Legacy survey data
https://researchrepository.wvu.edu/cgi/viewcontent.cgi?article=1328&context=faculty_publications
observe the central compact source more or less directly, ... sion line shifts relative to laboratory wavelengths (Vanden. Berk et al.
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https://researchrepository.wvu.edu/cgi/viewcontent.cgi?article=1328&context=faculty_publications
observe the central compact source more or less directly, ... sion line shifts relative to laboratory wavelengths (Vanden. Berk et al.
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22
V/147 - Université de Strasbourg
http://cdsarc.u-strasbg.fr/viz-bin/ReadMe/V/147?format=html&tex=true
The SDSS Photometric Catalogue, Data Release 12 (DR12) Alam S. et al. <Astrophys. J. Suppl. Ser. ... The central wavelength and FWHM are: ...
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http://cdsarc.u-strasbg.fr/viz-bin/ReadMe/V/147?format=html&tex=true
The SDSS Photometric Catalogue, Data Release 12 (DR12) Alam S. et al. <Astrophys. J. Suppl. Ser. ... The central wavelength and FWHM are: ...
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23
MMTCam : Welcome to the MMT Observatory
https://www.mmto.org/instrument-suite/mmtcam/
It is a high-end commercial Apogee camera equipped with a SDSS filter set from ... The associated filters have central wavelengths of 355nm, 469nm, 616nm, ...
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https://www.mmto.org/instrument-suite/mmtcam/
It is a high-end commercial Apogee camera equipped with a SDSS filter set from ... The associated filters have central wavelengths of 355nm, 469nm, 616nm, ...
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24
First Light with Baader SDSS filters by S. Ziegenbalg
https://www.baader-planetarium.com/en/blog/first-light-with-baader-sdss-filters-by-s-ziegenbalg/
The three central filters used for the Sloan Digital Sky Survey (SDSS) split ... law of radiation it also emits in the same wavelengths).
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https://www.baader-planetarium.com/en/blog/first-light-with-baader-sdss-filters-by-s-ziegenbalg/
The three central filters used for the Sloan Digital Sky Survey (SDSS) split ... law of radiation it also emits in the same wavelengths).
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25
THE DATA REDUCTION PIPELINE FOR THE SDSS-IV ...
https://research-repository.st-andrews.ac.uk/bitstream/handle/10023/9512/Law_2016_Data_AJ_83.pdf?sequence=1&isAllowed=y
The wavelength calibration of the MaNGA data is accurate to 5 km s ... APO to the SDSS-IV central computing facility at the.
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https://research-repository.st-andrews.ac.uk/bitstream/handle/10023/9512/Law_2016_Data_AJ_83.pdf?sequence=1&isAllowed=y
The wavelength calibration of the MaNGA data is accurate to 5 km s ... APO to the SDSS-IV central computing facility at the.
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26
Appendix B: OBSMODE Keywords - PySynphot - Read the Docs
https://pysynphot.readthedocs.io/en/latest/appendixb.html
Each central wavelength is intended for use with a particular grating. ... The Sloan Digital Sky Survey (SDSS) ugriz filter throughputs were provided by ...
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https://pysynphot.readthedocs.io/en/latest/appendixb.html
Each central wavelength is intended for use with a particular grating. ... The Sloan Digital Sky Survey (SDSS) ugriz filter throughputs were provided by ...
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27
SDSS-IV/MaNGA: SPECTROPHOTOMETRIC CALIBRATION ...
https://www.osti.gov/pages/servlets/purl/1378987
13 Center for Cosmology and Particle Physics, Department of Physics, ... MaNGAʼs relative calibration between the wavelengths of Hα and Hβ has an rms of ...
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https://www.osti.gov/pages/servlets/purl/1378987
13 Center for Cosmology and Particle Physics, Department of Physics, ... MaNGAʼs relative calibration between the wavelengths of Hα and Hβ has an rms of ...
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28
SkyNet Filter Descriptions
https://skynetjuniorscholars.org/supplements/42/file
telescopes the SDSS filters might be listed with the word prime or as u' g' r' I' z'.) Filter. Description. Central Wavelength u. Passes ultraviolet light.
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https://skynetjuniorscholars.org/supplements/42/file
telescopes the SDSS filters might be listed with the word prime or as u' g' r' I' z'.) Filter. Description. Central Wavelength u. Passes ultraviolet light.
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29
DESDM Y1A1_FINALCUT Reduced Image Set Release
https://data.darkenergysurvey.org/aux/releasenotes/DESDMrelease.html
The g,r,i and z filters are similar to, but not identical to their SDSS ... there are some center-to-edge variations in the response of the filters to ...
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https://data.darkenergysurvey.org/aux/releasenotes/DESDMrelease.html
The g,r,i and z filters are similar to, but not identical to their SDSS ... there are some center-to-edge variations in the response of the filters to ...
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30
An empirical template library of stellar spectra for a wide range ...
https://www.arxiv-vanity.com/papers/1702.06957/
Numerous groups have used SDSS to create partial libraries of specific effective temperature regions because of the wide wavelength coverage and vast number ...
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https://www.arxiv-vanity.com/papers/1702.06957/
Numerous groups have used SDSS to create partial libraries of specific effective temperature regions because of the wide wavelength coverage and vast number ...
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31
Downloads - ALPAKA - Google Sites
https://sites.google.com/site/sdssalpaka/downloads
SDSS_HA_CENWAV_ERR: Error on Halpha central wavelength reported by SDSS (SDSS: SpecLine.waveErr). SDSS_HA_SIGMA: Width (sigma, not FWHM) of ...
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https://sites.google.com/site/sdssalpaka/downloads
SDSS_HA_CENWAV_ERR: Error on Halpha central wavelength reported by SDSS (SDSS: SpecLine.waveErr). SDSS_HA_SIGMA: Width (sigma, not FWHM) of ...
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32
SDSS - eoPortal
https://www.eoportal.org/other-space-activities/sdss
SDSS acknowledges support and resources from the Center for ... output of quasars appears when it's spread out over different wavelengths.
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https://www.eoportal.org/other-space-activities/sdss
SDSS acknowledges support and resources from the Center for ... output of quasars appears when it's spread out over different wavelengths.
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33
SN 2006oz: rise of a super-luminous supernova ... - DOI
https://doi.org/10.1051/0004-6361/201118498
We present multi-color light curves of SN 2006oz from the SDSS-II SN Survey ... out to 0.5 × FWHM from the central wavelengths of the bracketing filters).
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https://doi.org/10.1051/0004-6361/201118498
We present multi-color light curves of SN 2006oz from the SDSS-II SN Survey ... out to 0.5 × FWHM from the central wavelengths of the bracketing filters).
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34
Doppler-imaging of the planetary debris disc at the white ...
https://www.eso.org/public/archives/releases/sciencepapers/eso1544/eso1544a.pdf
SDSS J1228+1040) via the detection of double peaked emis- ... trast SDSS J084539.17+225728.0 (Gдnsicke et al. ... Central wavelength [Е].
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https://www.eso.org/public/archives/releases/sciencepapers/eso1544/eso1544a.pdf
SDSS J1228+1040) via the detection of double peaked emis- ... trast SDSS J084539.17+225728.0 (Gдnsicke et al. ... Central wavelength [Е].
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35
MaNGA - SDSS
https://www.sdss4.org/surveys/manga/
The top right compares spectra observed by two fibers at different locations in the galaxy, showing how the spectrum of the central regions differs ...
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https://www.sdss4.org/surveys/manga/
The top right compares spectra observed by two fibers at different locations in the galaxy, showing how the spectrum of the central regions differs ...
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36
Johnson/Cousins vs. SDSS Filters - what to buy to start in ...
https://www.cloudynights.com/topic/796822-johnsoncousins-vs-sdss-filters-what-to-buy-to-start-in-amateur-photometry/
r' is catching on a lot in surveys, but not broadband means not as good as. Their profiles cover large wavelength ranges so you get more photons ...
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https://www.cloudynights.com/topic/796822-johnsoncousins-vs-sdss-filters-what-to-buy-to-start-in-amateur-photometry/
r' is catching on a lot in surveys, but not broadband means not as good as. Their profiles cover large wavelength ranges so you get more photons ...
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37
the SDSS-III APOGEE Spectral Line List for H-Band ... - Typeset
https://typeset.io/pdf/the-sdss-iii-apogee-spectral-line-list-for-h-band-4zax538k07.pdf
the third stage of the Sloan Digital Sky Survey (SDSS-III;. Eisenstein et al. 2011). ... the uncertainty in the central wavelength) and log(gf), which is.
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https://typeset.io/pdf/the-sdss-iii-apogee-spectral-line-list-for-h-band-4zax538k07.pdf
the third stage of the Sloan Digital Sky Survey (SDSS-III;. Eisenstein et al. 2011). ... the uncertainty in the central wavelength) and log(gf), which is.
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38
The Black Hole Mass of the z = 2.805 Multiply Imaged Quasar ...
https://par.nsf.gov/servlets/purl/10235764
quasar SDSS J2222+2745 using the Gemini North Multi-Object Spectrograph and the Nordic Optical ... are the amplitudes, λi are the central wavelengths, and σ.
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https://par.nsf.gov/servlets/purl/10235764
quasar SDSS J2222+2745 using the Gemini North Multi-Object Spectrograph and the Nordic Optical ... are the amplitudes, λi are the central wavelengths, and σ.
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39
public release of sky-residual subtracted spectra for SDSS DR7
http://www.sdss.jhu.edu/skypca/spSpec/skydr7_v05.pdf
sky lines extend over almost half the wavelength range of the SDSS ... We briefly summarise the main steps of the procedure in Section 2, ...
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http://www.sdss.jhu.edu/skypca/spSpec/skydr7_v05.pdf
sky lines extend over almost half the wavelength range of the SDSS ... We briefly summarise the main steps of the procedure in Section 2, ...
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40
Simultaneous analysis of SDSS spectra and GALEX ...
https://hal.archives-ouvertes.fr/hal-02989953/document
SDSS main galaxy sample with photometry in both GALEX ... band can be used to estimate ∆m1.5 in other wavelengths.
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https://hal.archives-ouvertes.fr/hal-02989953/document
SDSS main galaxy sample with photometry in both GALEX ... band can be used to estimate ∆m1.5 in other wavelengths.
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41
Photometry – I. “All sky”
http://spiff.rit.edu/classes/stromgren/allsky/kilkenny.pdf
3.5 SDSS - u g r i z . ... particles is almost independent of wavelength. ... The central wavelength is the mid-point of the maximum and minimum wavelengths.
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http://spiff.rit.edu/classes/stromgren/allsky/kilkenny.pdf
3.5 SDSS - u g r i z . ... particles is almost independent of wavelength. ... The central wavelength is the mid-point of the maximum and minimum wavelengths.
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42
WIRO Prime: Available Filters
http://physics.uwyo.edu/~WIRO/obsolete/Filters.html
... the filters currently available for use at WIRO Prime. Filter Name Central Wavelength Bandwidth Notes ... SDSS u', 3540 A, 650 A, Smith: (wheel #1).
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http://physics.uwyo.edu/~WIRO/obsolete/Filters.html
... the filters currently available for use at WIRO Prime. Filter Name Central Wavelength Bandwidth Notes ... SDSS u', 3540 A, 650 A, Smith: (wheel #1).
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43
Table of UV/optical Emission Lines Observed in Galaxies
http://astronomy.nmsu.edu/drewski/tableofemissionlines.html
› drewski › tableofemissionl...
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http://astronomy.nmsu.edu/drewski/tableofemissionlines.html
› drewski › tableofemissionl...
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44
The ALFALFA-SDSS Galaxy Catalog
https://wiki.physics.wisc.edu/ObsCos/images/c/c3/Durbala_ALFALFA-SDSS_Galaxy_Catalog_AJ_2020.pdf
4 Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, ... in conjunction with observations at other wavelengths.
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https://wiki.physics.wisc.edu/ObsCos/images/c/c3/Durbala_ALFALFA-SDSS_Galaxy_Catalog_AJ_2020.pdf
4 Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, ... in conjunction with observations at other wavelengths.
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45
SDSS IV MaNGA - Spatially resolved diagnostic diagrams
https://www.repository.cam.ac.uk/bitstream/1810/256374/1/Belfiore_et_al-2016-Monthly_Notices_of_the_Royal_Astromical_Society-AM.pdf
aim of this work, MaNGA's observed wavelength range (3600 - ... 3a,c the BPT diagnostic diagrams for the SDSS main galaxy sample.
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https://www.repository.cam.ac.uk/bitstream/1810/256374/1/Belfiore_et_al-2016-Monthly_Notices_of_the_Royal_Astromical_Society-AM.pdf
aim of this work, MaNGA's observed wavelength range (3600 - ... 3a,c the BPT diagnostic diagrams for the SDSS main galaxy sample.
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46
THE BARYON OSCILLATION SPECTROSCOPIC SURVEY ...
https://oaktrust.library.tamu.edu/bitstream/handle/1969.1/181691/document-1.pdf?sequence=1&isAllowed=y
56 Center for Astrophysical Sciences, Department of Physics and Astronomy, Johns Hopkins ... survey data using the full SDSS LRG sample (Padmanabhan.
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https://oaktrust.library.tamu.edu/bitstream/handle/1969.1/181691/document-1.pdf?sequence=1&isAllowed=y
56 Center for Astrophysical Sciences, Department of Physics and Astronomy, Johns Hopkins ... survey data using the full SDSS LRG sample (Padmanabhan.
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47
The Data Reduction Pipeline for the SDSS-IV MaNGA IFU ...
https://uknowledge.uky.edu/cgi/viewcontent.cgi?article=1420&context=physastron_facpub
The wavelength calibration of the MaNGA data is accurate to 5 km s ... APO to the SDSS-IV central computing facility at the.
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https://uknowledge.uky.edu/cgi/viewcontent.cgi?article=1420&context=physastron_facpub
The wavelength calibration of the MaNGA data is accurate to 5 km s ... APO to the SDSS-IV central computing facility at the.
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48
Panchromatic properties of 99 000 galaxies detected by SDSS ...
https://academiccommons.columbia.edu/doi/10.7916/D8J1016F
Notably, we find that SDSS 'main' galaxies detected by GALEX include ... fraction at other wavelengths and optical properties such as flux, ...
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https://academiccommons.columbia.edu/doi/10.7916/D8J1016F
Notably, we find that SDSS 'main' galaxies detected by GALEX include ... fraction at other wavelengths and optical properties such as flux, ...
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49
Introduction to SDSS - Astro Data Science
https://astrodatascience.net/introduction-to-sdss/
The Sloan Digital Sky Survey (SDSS) is one of the greatest ... The center wavelengths of these filters are presented in table below.
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https://astrodatascience.net/introduction-to-sdss/
The Sloan Digital Sky Survey (SDSS) is one of the greatest ... The center wavelengths of these filters are presented in table below.
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50
Baader SLOAN/SDSS Filters – Photometric
https://alpineastro.com/products/baader-sloan-sdss-filters-photometric
Description Baader SLOAN-ugriz' Bandpass Filter Set, suitable from f/15 to f/1.8 SLOAN/SDSS (ugriz') photometric filters with transmission according to ...
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https://alpineastro.com/products/baader-sloan-sdss-filters-photometric
Description Baader SLOAN-ugriz' Bandpass Filter Set, suitable from f/15 to f/1.8 SLOAN/SDSS (ugriz') photometric filters with transmission according to ...
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51
astro1.pdf - UC Berkeley Statistics
https://www.stat.berkeley.edu/~mmahoney/pubs/astro1.pdf
The main goals of this paper are to identify the informative wavelength regions in an ... wavelength range of spectra in most nearby SDSS galaxies,.
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https://www.stat.berkeley.edu/~mmahoney/pubs/astro1.pdf
The main goals of this paper are to identify the informative wavelength regions in an ... wavelength range of spectra in most nearby SDSS galaxies,.
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52
Galaxy and Mass Assembly (GAMA): survey diagnostics and ...
https://researchportal.port.ac.uk/portal/files/1518353/971.full.pdf
the Sloan Digital Sky Survey (SDSS; York et al. 2000). Each ... the 580V and 385R gratings with central wavelengths of 4800 and.
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https://researchportal.port.ac.uk/portal/files/1518353/971.full.pdf
the Sloan Digital Sky Survey (SDSS; York et al. 2000). Each ... the 580V and 385R gratings with central wavelengths of 4800 and.
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53
Transmission data for the CTIO Mosaic SDSS z Filter (c6020)
https://www.darkskiesawareness.org/kpno/mosaic/filters/c6020.html
Note: The central wavelength of CTIO Mosaic narrow band filters (actually all filters, but is very significant for narrow band filters) is ...
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https://www.darkskiesawareness.org/kpno/mosaic/filters/c6020.html
Note: The central wavelength of CTIO Mosaic narrow band filters (actually all filters, but is very significant for narrow band filters) is ...
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54
Low-cost BVRI Filters for CMOS/CCD Photometry
https://britastro.org/vss/low_cost_BVRI_filters.pdf
around 300 nm can define the short-wavelength edge of the passband. ... The central wavelengths and FWHM for the DIY filters used with a CMOS sensor are ...
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https://britastro.org/vss/low_cost_BVRI_filters.pdf
around 300 nm can define the short-wavelength edge of the passband. ... The central wavelengths and FWHM for the DIY filters used with a CMOS sensor are ...
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55
Panchromatic properties of 99 000 galaxies detected by SDSS ...
https://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2006.10675.x
Notably, we find that SDSS 'main' galaxies detected by GALEX include ... SDSS and surveys at other wavelengths have already been published.
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https://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2006.10675.x
Notably, we find that SDSS 'main' galaxies detected by GALEX include ... SDSS and surveys at other wavelengths have already been published.
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56
Vacuum and air wavelengths in spectroscopy
https://astronomy.stackexchange.com/questions/44999/vacuum-and-air-wavelengths-in-spectroscopy
Spectral wavelengths usually are defined as vacuum wavelength. The index of refraction of the medium influences the wavelength, and as such 'in vacuum' ...
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https://astronomy.stackexchange.com/questions/44999/vacuum-and-air-wavelengths-in-spectroscopy
Spectral wavelengths usually are defined as vacuum wavelength. The index of refraction of the medium influences the wavelength, and as such 'in vacuum' ...
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57
Panchromatic properties of 99 000 galaxies ... - NYU Scholars
https://nyuscholars.nyu.edu/en/publications/panchromatic-properties-of-99-000-galaxies-detected-by-sdss-and-s
For example, ∼2/3 of SDSS 'main' galaxies classified as active galactic nucleus ... of this diagram induced by requiring detections at other wavelengths.
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https://nyuscholars.nyu.edu/en/publications/panchromatic-properties-of-99-000-galaxies-detected-by-sdss-and-s
For example, ∼2/3 of SDSS 'main' galaxies classified as active galactic nucleus ... of this diagram induced by requiring detections at other wavelengths.
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58
Baader SLOAN/SDSS y´ Filter 1.25" - photometric
https://www.teleskop-express.de/shop/product_info.php/language/en/info/p14128_Baader-SLOAN-SDSS-y-acute--Filter-1-25----photometrisch.html
CMOS optimized filters from Baader-Planetarium ; CWL (central wavelength): SLOAN yŽ ; Coating (antireflection coating): Reflex-Blocker™ hard-coated, plano-optical ...
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https://www.teleskop-express.de/shop/product_info.php/language/en/info/p14128_Baader-SLOAN-SDSS-y-acute--Filter-1-25----photometrisch.html
CMOS optimized filters from Baader-Planetarium ; CWL (central wavelength): SLOAN yŽ ; Coating (antireflection coating): Reflex-Blocker™ hard-coated, plano-optical ...
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59
SN 2006oz: rise of a super-luminous supernova observed by ...
http://lss.fnal.gov/archive/2012/pub/fermilab-pub-12-933-a.pdf
We present multi-color light curves of SN 2006oz from the SDSS-II SN Survey that cover its ... to 0.5 × FWHM from the central wavelengths of the bracketing.
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http://lss.fnal.gov/archive/2012/pub/fermilab-pub-12-933-a.pdf
We present multi-color light curves of SN 2006oz from the SDSS-II SN Survey that cover its ... to 0.5 × FWHM from the central wavelengths of the bracketing.
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60
SDSS-IV MaNGA - OA@INAF
https://openaccess.inaf.it/bitstream/20.500.12386/31301/2/2011.04675.pdf
The SDSS-IV Mapping Nearby Galaxies at APO (MaNGA) program has been operating ... a 1σ width 40 km s−1 and central wavelength shifted by.
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https://openaccess.inaf.it/bitstream/20.500.12386/31301/2/2011.04675.pdf
The SDSS-IV Mapping Nearby Galaxies at APO (MaNGA) program has been operating ... a 1σ width 40 km s−1 and central wavelength shifted by.
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61
Photometric Redshifts and Properties of Galaxies from the ...
https://www.imprs-astro.mpg.de/sites/default/files/greisel.pdf
I also generate model spectra for red galaxies from the SDSS-III located at ... consists of five filters, u, g, r, i, z, with central wavelengths of 3551, ...
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https://www.imprs-astro.mpg.de/sites/default/files/greisel.pdf
I also generate model spectra for red galaxies from the SDSS-III located at ... consists of five filters, u, g, r, i, z, with central wavelengths of 3551, ...
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62
Magnitudes from spectra and the pivot wavelength
https://www.astro.ljmu.ac.uk/~ikb/research/mags-fluxes/
2 code, I determined the pivot wavelengths for the following filters. filter, pivot wavelength (Å), filter, pivot wavelength (Å). SDSS u, 3557, Bessell ...
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https://www.astro.ljmu.ac.uk/~ikb/research/mags-fluxes/
2 code, I determined the pivot wavelengths for the following filters. filter, pivot wavelength (Å), filter, pivot wavelength (Å). SDSS u, 3557, Bessell ...
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63
A Supernova Hits a Cosmic Speed Bump - Sky & Telescope
https://skyandtelescope.org/astronomy-news/supernova-cosmic-speed-bump/
SDSS / Caltech / Keck / CC BY 4.0 ... While the u-band emission faltered, all other wavelengths grew as expected, and this relative ...
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https://skyandtelescope.org/astronomy-news/supernova-cosmic-speed-bump/
SDSS / Caltech / Keck / CC BY 4.0 ... While the u-band emission faltered, all other wavelengths grew as expected, and this relative ...
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64
Hubble Archives - Universe Today
https://www.universetoday.com/category/hubble/
... supernova (SN 2016adj) located in the central dust lane of Centaurus A, ... The galaxies are named SDSS J115331 and LEDA 2073461, ...
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https://www.universetoday.com/category/hubble/
... supernova (SN 2016adj) located in the central dust lane of Centaurus A, ... The galaxies are named SDSS J115331 and LEDA 2073461, ...
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65
Quasars at All Cosmic Epochs - Page 27 - Google Books Result
https://books.google.com/books?id=zEdxDwAAQBAJ&pg=PA27&lpg=PA27&dq=sdss+central+wavelengths&source=bl&ots=Oj3Z0_tm9g&sig=ACfU3U3yAAeqZhQ3lH3DR0LtCHpO8zgS-A&hl=en&sa=X&ved=2ahUKEwiA1-_3n8L7AhWoMlkFHXAICbYQ6AF6BQiDAhAD
Absorption of radiation and source confusion are still the main issues affecting ... TABLE 1 |Data sources for the selection of multi-wavelength SED points.
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https://books.google.com/books?id=zEdxDwAAQBAJ&pg=PA27&lpg=PA27&dq=sdss+central+wavelengths&source=bl&ots=Oj3Z0_tm9g&sig=ACfU3U3yAAeqZhQ3lH3DR0LtCHpO8zgS-A&hl=en&sa=X&ved=2ahUKEwiA1-_3n8L7AhWoMlkFHXAICbYQ6AF6BQiDAhAD
Absorption of radiation and source confusion are still the main issues affecting ... TABLE 1 |Data sources for the selection of multi-wavelength SED points.
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66
Nasa sky calendar - kkcircuits.us
https://kkcircuits.us/nasa-sky-calendar.htm
Sigma VI Zero indicates the best-fitting, central (nominal) orbit and the further ... Join meteor experts from NASA's Marshall Space Flight Center for live ...
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https://kkcircuits.us/nasa-sky-calendar.htm
Sigma VI Zero indicates the best-fitting, central (nominal) orbit and the further ... Join meteor experts from NASA's Marshall Space Flight Center for live ...
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67
Statistics, Data Mining, and Machine Learning in Astronomy: ...
https://books.google.com/books?id=h2eYDwAAQBAJ&pg=PA305&lpg=PA305&dq=sdss+central+wavelengths&source=bl&ots=KfayGDNxdm&sig=ACfU3U30GQ0SFbq5WV5bZGSCwi00OTsVPQ&hl=en&sa=X&ved=2ahUKEwiA1-_3n8L7AhWoMlkFHXAICbYQ6AF6BQiCAhAD
For example, in the case of the SDSS spectra, a galaxy spectrum can be assumed ... The central panel of figure 7.7 shows the results of NMF applied to the ...
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https://books.google.com/books?id=h2eYDwAAQBAJ&pg=PA305&lpg=PA305&dq=sdss+central+wavelengths&source=bl&ots=KfayGDNxdm&sig=ACfU3U30GQ0SFbq5WV5bZGSCwi00OTsVPQ&hl=en&sa=X&ved=2ahUKEwiA1-_3n8L7AhWoMlkFHXAICbYQ6AF6BQiCAhAD
For example, in the case of the SDSS spectra, a galaxy spectrum can be assumed ... The central panel of figure 7.7 shows the results of NMF applied to the ...
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