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 |
by | ZHENG 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 |
by | HUANG 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 |
by | LI 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. |
Origin | of 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 |
by | LUO 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/> |
Origin | of the Acronym: A = Assigned by the author(s) |