Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati LAMOST JHHMMSS.ss+DDMMSS.s$
.

Details on Acronym:   LAMOST
  
LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope)
Write:<<LAMOST -HVSN>>
N: 4
Object:HV*  (SIMBAD class: HighVel* = High Velocity Star)
Stat:is completely incorporated in Simbad
Note:N=4 hypervelocity stars (HVS) discovered from the LAMOST surveys.
Ref:=2014ApJ...785L..23Z
byZHENG Z. , CARLIN J.L., BEERS T.C., DENG L., GRILLMAIR C.J., GUHATHAKURTA P., LEPINE S., NEWBERG H.J., YANNY B., ZHANG H., LIU C., JIN G., ZHANG Y.
 Astrophys. J., 785L, 23 (2014)
  The first hypervelocity star from the LAMOST survey.
o<LAMOST-HVSN> (No. HVS1).
Ref:=2017ApJ...847L...9H
byHUANG Y. , LIU X.-W., ZHANG H.-W., CHEN B.-Q., XIANG M.-S., WANG C., YUAN H.-B., TIAN Z.-J., LI Y.-B., WANG B.
 Astrophys. J., 847L, 9-9 (2017)
  Discovery of two new hypervelocity stars from the LAMOST spectroscopic surveys.
o<LAMOST-HVSN> (Nos HVS2-HVS3) added.
Ref:=2018AJ....156...87L
byLI Y.-B. , LUO A.-L., ZHAO G., LU Y.-J., ZHANG X.-S., ZHANG F.-P., DU B., ZUO F., ZHANG L., HUANG Y., XIANG M.-S., ZHAO J.-K., ZHAO Y.-H., HAN Z.-W.
 Astron. J., 156, 87-87 (2018)
  A new hyper-runaway star discovered from LAMOST and Gaia: ejected almost in the Galactic rotation direction.
o<LAMOST-HVSN> (No. HVS4) added.
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   LAMOST
  
LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope)
Write:<<LAMOST JHHMMSS.ss+DDMMSS.ss>>
<<LAMOST JHHMMSS.ss+DDMMSS.s>>
<<LAMOST JHHMMSS.ss+DDMMSS>>
N: ?
Object:?  (SIMBAD class: Optical = Optical Source)
Note:The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), is a special quasi-meridian reflecting Schmidt telescope located in Xinglong Station of national Astronomical Observatory, China (spectral range: 370-900nm).
LAMOST survey contains two main parts: the LAMOST ExtraGAlactic Survey (LEGAS), and the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) survey of Milky Way stellar structure.
For more information, visit: http://www.lamost.org/public/?locale=en
Only the reference to the first data release is given here.
Ref:=2015RAA....15.1095L
byLUO A.-L. , ZHAO Y.-H., ZHAO G., DENG L.-C., LIU X.-W., JING Y.-P., WANG G., ZHANG H.-T., SHI J.-R., CUI X.-Q., CHU Y.-Q., LI G.-P., BAI Z.-R., WU Y., CAI Y., CAO S.-Y., CAO Z.-H., CARLIN J.L., CHEN H.-Y., CHEN J.-J., CHEN K.-X., CHEN L., CHEN X.-L., CHEN X.-Y., CHEN Y., CHRISTLIEB N., CHU J.-R., CUI C.-Z., DONG Y.-Q., DU B., FAN D.-W., FENG L., FU J.-N., GAO P., GONG X.-F., GU B.-Z., GUO Y.-X., HAN Z.-W., HE B.-L., HOU J.-L., HOU Y.-H., HOU W., HU H.-Z., HU N.-S., HU Z.-W., HUO Z.-Y., JIA L., JIANG F.-H., JIANG X., JIANG Z.-B., JIN G., KONG X., KONG X., LEI Y.-J., LI A.-H., LI C.-H., LI G.-W., LI H.-N., LI J., LI Q., LI S., LI S.-S., LI X.-N., LI Y., LI Y.-B., LI Y.-P., LIANG Y., LIN C.-C., LIU C., LIU G.-R., LIU G.-Q., LIU Z.-G., LU W.-Z., LUO Y., MAO Y.-D., NEWBERG H., NI J.-J., QI Z.-X., QI Y.-J., SHEN S.-Y., SHI H.-M., SONG J., SONG Y.-H., SU D.-Q., SU H.-J., TANG Z.-H., TAO Q.-S., TIAN Y., WANG D., WANG D.-Q., WANG F.-F., WANG G.-M., WANG H., WANG H.-C., WANG J., WANG J.-N., WANG J.-L., WANG J.-P., WANG J.-X., WANG L., WANG M.-X., WANG S.-G., WANG S.-Q., WANG X., WANG Y.-N., WANG Y., WANG Y.-F., WANG Y.-F., WEI P., WEI M.-Z., WU H., WU K.-F., WU X.-B., WU Y.-Z., XING X.-Z., XU L.-Z., XU X.-Q., XU Y., YAN T.-S., YANG D.-H., YANG H.-F., YANG H.-Q., YANG M., YAO Z.-Q., YU Y., YUAN H., YUAN H.-B., YUAN H.-L., YUAN W.-M., ZHAI C., ZHANG E.-P., ZHANG H.-W., ZHANG J.-N., ZHANG L.-P., ZHANG W., ZHANG Y., ZHANG Y.-X., ZHANG Z.-C., ZHAO M., ZHOU F., ZHOU X., ZHU J., ZHU Y.-T., ZOU S.-C., ZUO F.
 RAA, 15, 1095-1124 (2015)
  The first data release (DR1) of the LAMOST regular survey.
=E=Catalogue in electronic form as <V/146/>
=E=Catalogue in electronic form as <V/149/>
=E=Catalogue in electronic form as <V/153/>
Originof the Acronym: A = Assigned by the author(s)