lamost 补充星系样本和lamost-sdss星系对样本
DESCRIPTION
LAMOST 星系巡天计划 North Galactic Cap South Galactic Cap Complementary galaxy sample South Galactic Cap Main galaxy sample Emission line galaxy Two complete fields(Wu Hong)TRANSCRIPT
![Page 1: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/1.jpg)
LAMOST 补充星系样本和LAMOST-SDSS星系对样本
沈世银上海天文台
![Page 2: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/2.jpg)
LAMOST 星系巡天计划 North Galactic Cap
Complementary galaxy sample
South Galactic Cap Main galaxy sample Emission line galaxy
Two complete fields(Wu Hong)
![Page 3: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/3.jpg)
Complementary galaxy sample
SDSS main sample galaxies r<17.77 Spectroscopic completeness
>90% ~7% missed due to fiber
collision effect Input catalog of LAMOST
68,722 objects Biased towards (small scale)
high density environment, e.g. galaxy pair, triplet/quartlet, compact group
![Page 4: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/4.jpg)
Galaxy pair sample in SDSS are strongly biased towards large separation and low redshift
![Page 5: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/5.jpg)
Current status
Complementary galaxy with LAMOST spectra
DR2 (2011-2014): 3456 Why very small fraction?
Lower priority than QSO targets Few Medium plates
Low S/N
Y3 (2014-2015): 2620
![Page 6: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/6.jpg)
Redshift measurements In DR2, 3456 complementary galaxies have
LAMOST spectra Only 1951 have redshifts measured by LAMOST 1-
D pipeline We developed a new PCA-redshift
measurement code 2796 with redshift measured, increased about
25%
![Page 7: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/7.jpg)
Early science: new galaxy pairs
How to define a galaxy pair?
Non-trivial
P<100kpc dV<500km/s
Galaxy pairs are one of the key ingredients to study the galaxy merging and galaxy interaction.
![Page 8: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/8.jpg)
Galaxy pair sample (Shen et al., 2015) 1,102 galaxy pairs (P<100kpc, dV<500km/s)
Visual inspection
![Page 9: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/9.jpg)
Multiple flag Pair definition: dV<500km/s, Rp<100kpc Physical pair ?
interaction
Multiple system: triplet, group,cluster One of the member within another pair Not complete
Redshift dependent A triplet system with M =-20,-21,-22 mag would be
identified as a triplet, a pair and a single galaxy in the SDSS MG sample (r<17.77) at redshift z=0.05,0.1,0.15 respectively.
![Page 10: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/10.jpg)
Overlap flag Visual inspection
Very close pair (image overlap each other) Photometry not accurate Color bias
Interesting objects Example: an isolated triplet (Feng et al. 2015) See http://
cluster.shao.ac.cn/wiki/index.php/Interesting_object_in_LEGAS_DR1
http://cluster.shao.ac.cn/wiki/index.php/Interesting_object_in_LEGAS_DR2
![Page 11: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/11.jpg)
Discovery of an isolated galaxy triplet (Feng et al. 2015)
Chain-like structureFormed in early time
Early type galaxies with Halpha emissionrecent star formation
![Page 12: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/12.jpg)
![Page 13: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/13.jpg)
Other applications and future Supply the galaxy pair sample Supply redshifts to the galaxy group catalog of
Yang et al. Small-scale galaxy cross-correlation function
(Guo Hong)
Future How much can we finish the spectral survey of the
complementary galaxies? After three years (6000 of 6,8000), only two years left.
LAMOST spectral survey 2? (after 2017)
![Page 14: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/14.jpg)
Two complete fields Ra = 37.8, Dec = 3.4 Ra = 21.5, Dec = −2.20
r<18.1 mag ~5000 galaxies, 25000 point sources 28 plates observed from 2012-2014
Yang et al. in preparation
![Page 15: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/15.jpg)
South Galactic Cap
Main goal of the galaxy survey in design Winter season, good weather
Footprint Dec>-10 & b<-30, 3700 sq deg
Input catalog Main sample galaxies (r<18) ~660 k Blue galaxies (18<r<18.8) ~200 k
Science motivation Large galaxy spectroscopic sample in SGC,
deeper than SDSS main sample galaxies Probe the faint (higher z) star forming galaxies
![Page 16: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/16.jpg)
Current status Only 35,000 (<5%) objects observed in past
four years
![Page 17: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/17.jpg)
We can not finish the galaxy survey in SGC as we designed in 5 years (2012-2017)
![Page 18: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/18.jpg)
How is the spectra quality?
![Page 19: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/19.jpg)
Reasons for the small number of galaxies being observed Fiber assignment
Galaxy PRI < QSO QSO candidates outnumbers galaxy
Will be changed Small number of M plates in EG area
Could not be greatly improved because of requirement of successful rate of spectroscopy Weather condition Other survey (Galactic Anti Center , M31)
![Page 20: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/20.jpg)
Possible Collaboration: TAIPAN Measure redshifts for 500,000 galaxies(r~17) and peculiar
velocities for 50,000 galaxies in the nearby universe on the UKST over a 3.5-year period (2016-2019)
Scientific goal Hubble constant Bulk flow Velocity power spectrum Redshift space distortions Galaxy evolution
LAMOST: extend the Taipan survey into the non-SDSS areas of the northern hemisphere? Spectra quality?
![Page 21: LAMOST 补充星系样本和LAMOST-SDSS星系对样本](https://reader033.vdocuments.net/reader033/viewer/2022061502/5a4d1ad37f8b9ab059971efa/html5/thumbnails/21.jpg)
summary There are only about 50,000 galaxies that had
been observed by LAMOST in its first three years ~6000 SDSS missed main sample galaxies
Useful for new galaxy pair identification ~5000 galaxies in two small complete fields ~35000 galaxies in South Galactic Cap Other ~4000 bright galaxies (replicated
observation) The spectra quality is barely acceptable(S/N
~10) for galaxies brighter than r<17 mag Redshift measurement Stellar population?