J/MNRAS/512/1091ivo://CDS.VizieR/J/MNRAS/512/1091doi:10.26093/cds/vizier/bg-g0-123CDSScicluna P.Kemper F.Mcdonald I.Srinivasan S.Trejo A.,Wallstrom S.H.J.Wouterloot J.G.A.Cami J.Greaves J.He J.Hoai D.T.,Kim H.Jones O.C.Shinnaga H.Clark C.J.R.Dharmawardena T.,Holland W.Imai H.Van Loon J.T.Menten K.M.Wesson R.Chawner H.,Feng S.Goldman S.Liu F.C.Macisaac H.Tang J.Zeegers S.Amada K.,Antoniou V.Bemis A.Boyer M.L.Chapman S.Chen X.Cho S.-H.Cui L.,Dell'agli F.Friberg P.Fukaya S.Gomez H.Gong Y.Hadjara M.,Haswell C.Hirano N.Hony S.Izumiura H.Jeste M.Jiang X.,Kaminski T.Keaveney N.Kim J.Kraemer K.E.Kuan Y.-J.Lagadec E.,Lee C.F.Li D.Liu S.-Y.Liu T.De Looze I.Lykou F.Maraston C.,Marshall J.P.Matsuura M.Min C.Otsuka M.Oyadomari M.Parsons H.,Patel N.A.Peeters E.Pham T.A.Qiu J.Randall S.Rau G.Redman M.P.,Richards A.M.S.Serjeant S.Shi C.Sloan G.C.Smith M.W.L.Suh K.-W.,Toala J.A.Uttenthaler S.Ventura P.Wang B.Yamamura I.Yang T.,Yun Y.Zhang F.Zhang Y.Zhao G.Zhu M.Zijlstra A.A.2026-08-03T07:31:19Z2025-03-27T15:09:43ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmilky-way-galaxystellar-mass-lossinterstellar-mediuminfrared-astronomymillimeter-astronomysubmillimeter-astronomyphotometrystellar-distancestellar-spectral-typesastrometryThe Nearby Evolved Stars Survey (NESS) is a volume-complete sample of ~850 Galactic evolved stars within 3 kpc at (sub-)mm wavelengths, observed in the CO J = (2-1) and (3-2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to Gaia EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of 4.7 * 10^-5^ M_{sun}_ yr^-1^ from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 {mu}m spectral indices are consistent with the blackbody Rayleigh-Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.2022MNRAS.512.1091Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/512/1091CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/112/557 : Classification of IRAS Sources (Kwok+ 1997)J/A+A/532/A54 : GRAMS carbon-star model grid (Srinivasan+, 2011)J/MNRAS/471/770 : Parameters and IR excesses of Gaia DR1 stars (McDonald+,2017)J/ApJ/877/49 : DUSTiNGS. V. 3.6 and 4.5um light curves (Goldman+, 2019)II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)J/AJ/156/112 : Near-infrared Mira period-luminosity relations in M33J/ApJ/857/67 : HST obs. of Mira candidates in NGC 4258 (Huang+, 2018)J/A+A/556/A38 : Period-mass-loss rate relation of Miras (Uttenthaler, 2013)I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)I/337 : Gaia DR1 (Gaia Collaboration, 2016)I/345 : Gaia DR2 (Gaia Collaboration, 2018)J/A+A/606/A67 : Circumstellar envelopes CO photodissociationJ/ApJ/851/152 : DUSTiNGS. IV. AGB spectral types with HST (Boyer+, 2017)J/ApJ/800/51 : DUSTiNGS II. Metal-poor dusty AGB stars (Boyer+, 2015)J/AJ/142/103 : Cool evolved stars in SAGE-SMC and SAGE-LMC (Boyer+, 2011)J/A+A/622/A120 : Mass loss from Miras with and without Tc (Uttenthaler, 2019)https://evolvedstars.space/catalogue/ : current NESS cataloguehttps://nida.esac.esa.int/nida-cl-web/?ACTION=OBSERVATION : ISO data archivehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/512/1091https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/512/1091http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/512/1091https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/512/1091https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/512/1091http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/512/1091GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/512/1091/table1 (Physical properties of our NESS sources sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/512/1091/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/512/1091/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/512/1091/table1?GETtext/xml+votable180.050000true1.7198133343.083987780.0055555555555555566/15 676 846 883 889 959 1015 1079 1238 1345 1350 1399 1482 1490 1493 1619 1634 1727 1784 1889 1892 1977 1986 2018 2031 2040 2203 2282 2428 2500 2528 2694 2732 2902 2937 2994 3209 3221 3256 3262 3265 3272 3359 3394 3438 3446 3459 3462 3469 3491 3628 3640 3666 3765-3766 3801 3951 4290 4306 4355 4365 4614 4972 5273 5489 5574 5647 5718 6007 6219 6251 6444 6714 6803 6919 7119 7152 7545 7619 7673 7919 8162 8430 8475 8492 8532 8603 8611 8678 8926 9074 9137 9142 9258 9589 9620 9750 9813 9939 9968 10107 10137 10167 10609 10696 10960 11017 11097 11165 11188 11519 11544 11597 11747 11866 11928 12137 12300 12333 12382 12544 12703 12829 12877 12882 12964 12974 12988 13023 13051 13080 13088 13110 13113 13385 13392 13454 13463 13579 13615 13623 13666 13677 13683 13711 13783 13803 13813 13845 13861 13968 14027 14048 14161 14175 14196 14259 14301-14302 14319 14336 14355 14371 14391 14396 14399 14428 14443 14454 14457 14490 14508 14550 14619 14623-14624 14632 14644 14659 14689 14692-14693 14729 14736 14738 14811 14834 14846 14878 14894 14968 15044 15105 15122 15135 15396 15401 15415 15430 15449 15475 15620 15624 15629 15640-15641 15650 15663 15674 15681 15741 15877 15939 16019 16132 16147 16175 16224 16232-16233 16452 16783 16807 16812 17192 17223 17271 17502 17716 17763 18256 18364 18634 18691 18917 18998 19103 19186 19279 19284 19293 19490 19629 19761 20022 20212 20600 20626 20699 20715 20761 20764 20824 20843 21050 21215 21224 21241 21255 21326 21376 21447 21457 21494 21710 21777 21854 21977 22023 22051 22144 22156 22161 22170 22233 22241 22271 22333 22434 22556 22806 22855 22860 22881 22941 23095 23327 23423 23471 23606 23611 23694 23876 23996 24151 24164 24389 24443 24448 24501 24554 24563 24605 24611 24800 25228 25246 25489 25543-25544 26070 26180 26319 26327 26345 26654 27788 28028 28685-28687 28692 28711 28731 28773-28774 28779 28796 28800 28803 28807 28812 28819 28821 28825-28827 28829-28830 28846-28847 28851 28868 28872 28880 28890-28891 28908 28912-28913 28917 28920 28922 28927 28981 28996 28998 29000 29043 29072 29091-29092 29096 29100 29108 29115-29116 29123 29136 29207 29222 29237 29286 29318 29438 29474 29504 29508 29513 29528 29539 29545 29550 29556 29597 29626 29690 29701 29705 29817 29841 29855 29859 29877 29886 29963 30011 30034-30035 30069 30087 30123 30189 30218 30220 30222 30234 30243-30245 30247 30256 30260-30262 30265 30269 30318 30322 30341 30345 30397 30445 30479 30481 30491 30567 30602-30603 30606 30614 30624 30634 30644 30664 30687 30958 31231 31292 31366 31629 31828 31837 31866 31938 32015 32062 32081 32123 32142 32189 32254 32259 32271 32322 32331 32519 32626 32661 32784 32790 32799 32878 32891 33094 33140 33233 33249 33349 33581 33589 33624 33689 33739 33919 34158 34240 34279 34312 34356 34576 34792 35069 35118 35506 35641 36028 36222 36233 36317 36320 36655 36765 36954 36980 36986 37121 37139 37174 37193 37210-37211 37244 37247 37306-37307 37327 37335 37337-37338 37342-37343 37357 37369 37371 37374 37400 37405 37540 37617 37663 37675 37680 37688 37706 37747 37752 37759-37760 37844 37865 37894 37899 37927-37928 37938 37940 37987 38002 38016 38024 38044 38051 38059 38066 38073 38096 38130 38149 38210 38230 38455 38505-38506 38540 38560 38562 38660 38701 39089 39165 39233 39317 39324 39342 39355 39371 39395 39504 39631 39637 39714 39724 39789 39899 39905 40009 40094 40150 40235 40246 40466 40566 40686 40795 40878 41022 41045 41061 41118 41198 41204 41206 41245 41270 41284 41310 41392 41397 41473 41530 41580 41586 41593-41594 41607 41614 41624 41633 41653 41670 41673 41676-41677 41679 41683 41687 41690-41691 41704 41710 41742 41754 41763 41786 41791 41795 41801 41807 41811 41815 41822 41824 41827 41835 41849 41856 41877 41920 41937 41945 41974 41996 42046 42057 42077 42081 42126 42138 42150 42154 42165 42168 42195 42197 42201 42205-42208 42212 42214 42218 42225-42226 42229 42272 42283 42285 42290 42332 42337 42362 42370 42377-42379 42382 42388 42391-42392 42394-42396 42398 42404 42410 42418 42435-42436 42438-42439 42442 42444 42446 42454 42461-42462 42467 42479 42483 42486 42489 42492 42496 42498-42500 42504 42507 42513 42519 42527 42530 42561-42562 42584 42687 42702 42730 42774 42818 42833 42840 42850 42895 43028 43032-43033 43046 43052-43053 43132 43141 43258 43309 43328 43480 43494 43566 43572 43609 43726 43797 43842 43861 43890 44018 44067 44198 44248 44417 44546 44748 44857 45075 45131 45285 45291 45343 45450 45700 45771 45782 45790 45809 45824 46138 46160 46313 46318 46321 46330 46387 46768 46795 46932 46938 47185 47217 47248 47303 47332 47342 47374 47376 47414 47484 47508 47637 47664 47677 47736-47737 47822 47828 47963 47967 48006 48038 48097 48133 48301 48330 48604 48650 48700 48753 48903 48918 49123https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/512/1091?format=asciiInfraredMillimeterdefaultJ/MNRAS/512/1091/table1Physical properties of our NESS sources sampleIRASIRAS PSC identifier (IRASPSC)meta.id;meta.maincharprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSimbadNameSimbad column added by the CDSmeta.idcharnullabletable3Indicates SCUBA-2 obs data in table3meta.ref.urlcharSIMBADSIMBAD main identifier (ID_SIM)meta.idchar2MASS2MASS PSC designation (TMASS_Designation)meta.id.crosscharTierNESS sample tier (sample) (1)src.samplecharMap[0/1] Whether source was mapped, yes for 46 sources (mapping) (2)meta.codeintDDistance estimate to source (DIST_BEST)kpcpos.distancedoublee_D? Uncertainty in distance estimate (EDIST_BEST)kpcstat.errordoublenullablen_D[M H G L] Source of distance estimate (DIST_BEST_TYPE) (3)meta.notecharISO? Infrared Space Observatory ISO identifier (ISO_TDT)meta.id;phys.veloc;instr.obstyintnullableLRSSpectroscopic IRAS LRS classification from Kwok et al. (1997ApJS..112..557K, Cat. J/ApJS/112/557) (LRS_class)src.spTypecharSWSSpectroscopic ISO SWS classification from Kraemer et al. (2002ApJS..140..389K) (SWS_class)src.spTypecharChem[O S C]? Chemical type from spectrum (spec_chemtype) (4)src.spTypechardM/dtGRAMS best-fit dust-production rate DPR (GRAMS_DPR) (5)solMass/yrphys.mass.loss;meta.modelleddoublee_dM/dtUncertainty in GRAMS best-fit DPR (GRAMS_eDPR)solMass/yrstat.errordoubleChemGram[o c] GRAMS best-fit chemical type (GRAMS_chemtype) (6)src.spTypecharFtot450GRAMS star+dust flux prediction at 450 um (GRAMS_ftot_450)Jyphot.flux.density;em.mm.400-750GHz;meta.modelleddoubleFtot850GRAMS star+dust flux prediction at 850 um (GRAMS_ftot_850)Jyphot.flux.density;em.mm.200-400GHz;meta.modelleddoubleRAJ2000Right ascension from simbad (J2000) (RA_SIM)degpos.eq.ra;meta.mainDEJ2000Declination from simbad (J2000) (DEC_SIM)degpos.eq.dec;meta.mainRAIdegRight ascension from IRAS (J2000) (RA_IRAS)degpos.eq.raDEIdegDeclination from IRAS (J2000) (DEC_IRAS)degpos.eq.decJ/MNRAS/512/1091/table3Continuum fluxes and spectral indices from the initial reduction of the SCUBA-2 dataIRASIRAS PSC identifier (IRASPSC)meta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintF450JCMT/SCUBA2 450 um flux (SCUBA2_F450) (1)Jyphot.flux.density;em.mm.400-750GHz;obsdoublee_F450Uncertainty in JCMT/SCUBA2 450 um flux (SCUBA2_F450_err)Jystat.errordoublel_F450[-1/0] JCMT/SCUBA2 450 um flux quality flag, -1 if flux is 3{sigma} upper limit, 42 cases in our sample (SCUBA2_F450_qual)meta.code.errorintF850JCMT/SCUBA2 850 um flux (SCUBA2_F850) (1)Jyphot.flux.density;em.mm.200-400GHz;obsdoublee_F850Uncertainty in JCMT/SCUBA2 850 um flux (SCUBA2_F850_err)Jystat.errordoublel_F850[-1/0] JCMT/SCUBA2 850 um flux quality flag, -1 if flux is 3{sigma} upper limit, 38 cases in our sample (SCUBA2_F850_qual)meta.code.errorintalpha? Spectral index see Section 4.4 Anomalous detection of cold dust (alpha)spect.index;em.mmdoublenullableCIalphalow