J/A+A/688/A209  Galactic post-AGB stars multi-phot. (Gonzalez-Santamaria+, 2024)

A search for Galactic post-asymptotic giant branch stars in Gaia DR3. Gonzalez-Santamaria I., Manteiga M., Manchado A., Villaver E., Ulla A., Dafonte C. <Astron. Astrophys. 688, A209 (2024)> =2024A&A...688A.209G 2024A&A...688A.209G (SIMBAD/NED BibCode)
ADC_Keywords: Stars, giant ; Photometry, ultraviolet ; Optical ; Photometry, infrared Keywords: virtual observatory tools - stars: AGB and post-AGB - stars: distances - stars: fundamental parameters - Hertzsprung-Russell and C-M diagrams Abstract: When low- and intermediate-mass stars leave the asymptotic giant branch (AGB) phase, and before they reach the planetary nebula stage, they enter a very brief and rather puzzling stellar evolutionary stage called post-AGB stage. The post-AGB phase lasts very briefly, about a few thousand years at most. The number of objects that are confirmed in this phase therefore is really small, and our understanding of this elusive stellar evolutionary stage is accordingly very limited. We provide a reliable catalogue of Galactic post-AGB stars together with their physical and evolutionary properties obtained through Gaia DR3 astrometry and photometry. As an added product, we provide information for a sample of other types of stellar objects, whose observational properties mimic those of post-AGB stars. Post-AGB stars are characterised by their infrared excesses and high luminosities. The publication of precise parallaxes in Gaia DR3 made it possible to calculate accurate distances and to revise the derivation of luminosities for post-AGB candidates, so that objects outside the expected luminosity range can be discarded. We started by identifying post-AGB stars or possible candidates from the bibliography, and we then searched for their Gaia DR3 counterpart sources. Using the available photometry, interstellar extinction, spectroscopically derived temperatures or spectral types and parallax-derived distances from the literature, we fitted their spectral energy distributions and estimated their luminosities and circumstellar extinctions. By a comparison to models, the luminosity values allowed us to determine which objects are likely post-AGB stars from other target types. Their position in the Hertzsprung-Russell diagram allows a direct comparison with updated post-AGB evolutionary tracks and an estimation of their masses and evolutionary ages. We obtained a sample of 69 reliable post-AGB candidates that meet our classification criteria, which provide their coordinates, distances, effective temperature, interstellar and circumstellar extinction, luminosity, mass, and evolutionary age. In addition, we provide similar data for other stellar objects in our initial compilation, such as supergiant stars and young stellar objects. Our identifications and parameters are compared with others found in the recent literature for the subject. We selected the data with the best precision in parallax and distance to obtain more accurate luminosities, which allowed us to confidently classify the objects of the sample in different stellar phases. In turn, this allowed us to provide a small but reliable sample of post-AGB objects. The derived mean evolutionary time and average mass values agree with theoretical expectations and with the mean mass value obtained in a previous work for the subsequent evolutionary stage, the planetary nebula stage. Description: Photometry data in multiple bands provided by spanish Virtual Observator y SED Analyzer (VOSA) for a catalogue of post-AGB stars is presented. Two tables are provided: one of them contains the photometry for 83 post-AGB stars located in the Galatctic Plane, and the other one contain s the photometry for 35 post-AGB stars located in the Halo. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 109 157 General data of the 157 post-AGB candidates tablea6.dat 3106 83 Photometry of post-AGB stars in the Plane tablea7.dat 3106 35 Photometry of post-AGB stars in the Halo -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq Sequential number 5- 27 A23 --- Star Simbad Name 29- 47 I19 --- GaiaEDR3 Gaia EDR3 identification number 49- 56 F8.4 deg RAdeg Right ascension (ICRS) at Ep=2016.0 58- 65 F8.4 deg DEdeg Declination (ICRS) at Ep=2016.0 67- 71 F5.2 mag Gmag Gaia G magnitude 73- 76 F4.2 --- AVis ?=- Interstellar extinction taken from Stassun (2018AJ....156..102S 2018AJ....156..102S, Cat. IV/38) 78- 91 A14 --- SpType Spectral Type taken from Simbad database 93- 97 A5 --- Ref Reference for Post-AGB origin (1) 99-109 A11 --- Flag Flag (2) -------------------------------------------------------------------------------- Note (1): References as follows: 1 = Simbad database 2 = Torun catalogue, https://fox.ncac.torun.pl/camkweb/postagb2.php 3 = Suarez et al. (2006A&A...458..173S 2006A&A...458..173S, Cat. J/A+A/458/173) Note (2): Binary reference (B), Variability reference (V) and Removed reason (R) as follows: B1 = Kluska et al. (2019A&A...631A.108K 2019A&A...631A.108K, Cat. J/A+A/631/A108) B2 = Torun catalogue (https://fox.ncac.torun.pl/camkweb/postagb2.php) B3 = Gallardo Cava et al. (2023A&A...671A..80G 2023A&A...671A..80G) B4 = Van Winckel et al. (2014A&A...563A..10C 2014A&A...563A..10C) B5 = Oomen et al. (2018A&A...620A..85O 2018A&A...620A..85O, Cat. J/A+A/620/A85) B6 = Doroshenko et al. (2016MNRAS.458.2565D 2016MNRAS.458.2565D) B7 = Kluska et al. (2022A&A...658A..36K 2022A&A...658A..36K, Cat. J/A+A/658/A36) B8 = Parthasarathy et al. (2022RNAAS...6..171P 2022RNAAS...6..171P) V1 = Kluska et al. (2022A&A...658A..36K 2022A&A...658A..36K, Cat. J/A+A/658/A36) V2 = Kamath et al. (2022ApJ...927L..13K 2022ApJ...927L..13K) V3 = Dubus et al. (2018A&A...617A..26D 2018A&A...617A..26D) V4 = Simbad database R1 = very hot star (Teff≥24000K) R2 = incorrect source identification R3 = without Gaia counterpart R4 = already in planetary nebula phase R5 = composite object, blended -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea6.dat tablea7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 23 A23 --- Star Star name 25- 32 E8.3 10mW/m2/nm F1250-1300 ?=- IUE/IUE.1250-1300 flux 35- 42 E8.3 10mW/m2/nm e_F1250-1300 ? IUE/IUE.1250-1300 flux error 44- 51 E8.3 10mW/m2/nm F1450-1500 ?=- IUE/IUE.1450-1500 flux 54- 61 E8.3 10mW/m2/nm e_F1450-1500 ? IUE/IUE.1450-1500 flux error 63- 70 E8.3 10mW/m2/nm FFUV ?=- GALEX/GALEX.FUV flux 73- 80 E8.3 10mW/m2/nm e_FFUV ? GALEX/GALEX.FUV flux error 82- 89 E8.3 10mW/m2/nm F1675-1725 ?=- IUE/IUE.1675-1725 flux 92- 99 E8.3 10mW/m2/nm e_F1675-1725 ? IUE/IUE.1675-1725 flux error 101- 108 E8.3 10mW/m2/nm F2150-2200 ?=- IUE/IUE.2150-2200 flux 111- 118 E8.3 10mW/m2/nm e_F2150-2200 ? IUE/IUE.2150-2200 flux error 120- 127 E8.3 10mW/m2/nm FNUV ?=- GALEX/GALEX.NUV flux 130- 137 E8.3 10mW/m2/nm e_FNUV ? GALEX/GALEX.NUV flux error 139- 146 E8.3 10mW/m2/nm F2395-2445 ?=- IUE/IUE.2395-2445 flux 149- 156 E8.3 10mW/m2/nm e_F2395-2445 ? IUE/IUE.2395-2445 flux error 158- 165 E8.3 10mW/m2/nm F2900-3000 ?=- IUE/IUE.2900-3000 flux 168- 175 E8.3 10mW/m2/nm e_F2900-3000 ? IUE/IUE.2900-3000 flux error 177- 184 E8.3 10mW/m2/nm FuGen ?=- Generic/Stromgren.u flux 187- 194 E8.3 10mW/m2/nm e_FuGen ? Generic/Stromgren.u flux error 196- 203 E8.3 10mW/m2/nm FuGCPD ?=- GCPD/Stromgren.u flux 206- 213 E8.3 10mW/m2/nm e_FuGCPD ? GCPD/Stromgren.u flux error 215- 222 E8.3 10mW/m2/nm FUGen ?=- Generic/Johnson.U flux 225- 232 E8.3 10mW/m2/nm e_FUGen ? Generic/Johnson.U flux error 234- 241 E8.3 10mW/m2/nm FuPar ?=- Paranal/OmegaCAM.u_SDSS flux 244- 251 E8.3 10mW/m2/nm e_FuPar ? Paranal/OmegaCAM.u_SDSS flux error 253- 260 E8.3 10mW/m2/nm FuSDSS ?=- SLOAN/SDSS.u flux 263- 270 E8.3 10mW/m2/nm e_FuSDSS ? SLOAN/SDSS.u flux error 272- 279 E8.3 10mW/m2/nm FJ0400 ?=- OAJ/JPAS.J0400 flux 282- 289 E8.3 10mW/m2/nm e_FJ0400 ? OAJ/JPAS.J0400 flux error 291- 298 E8.3 10mW/m2/nm FJ0410JPLUS ?=- OAJ/JPLUS.J0410 flux 301- 308 E8.3 10mW/m2/nm e_FJ0410JPLUS ? OAJ/JPLUS.J0410 flux error 310- 317 E8.3 10mW/m2/nm FvGen ?=- Generic/Stromgren.v flux 320- 327 E8.3 10mW/m2/nm e_FvGen ? Generic/Stromgren.v flux error 329- 336 E8.3 10mW/m2/nm FJ0410JPAS ?=- OAJ/JPAS.J0410 flux 339- 346 E8.3 10mW/m2/nm e_FJ0410JPAS ? OAJ/JPAS.J0410 flux error 348- 355 E8.3 10mW/m2/nm FvGCPD ?=- GCPD/Stromgren.v flux 358- 365 E8.3 10mW/m2/nm e_FvGCPD ? GCPD/Stromgren.v flux error 367- 374 E8.3 10mW/m2/nm FJ0420 ?=- OAJ/JPAS.J0420 flux 377- 384 E8.3 10mW/m2/nm e_FJ0420 ? OAJ/JPAS.J0420 flux error 386- 393 E8.3 10mW/m2/nm FBT ?=- TYCHO/TYCHO.B flux 396- 403 E8.3 10mW/m2/nm e_FBT ? TYCHO/TYCHO.B flux error 405- 412 E8.3 10mW/m2/nm FJ0430JPLUS ?=- OAJ/JPLUS.J0430 flux 415- 422 E8.3 10mW/m2/nm e_FJ0430JPLUS ? OAJ/JPLUS.J0430 flux error 424- 431 E8.3 10mW/m2/nm FBAPASS ?=- Misc/APASS.B flux 434- 441 E8.3 10mW/m2/nm e_FBAPASS ? Misc/APASS.B flux error 443- 450 E8.3 10mW/m2/nm FJ0430JPAS ?=- OAJ/JPAS.J0430 flux 453- 460 E8.3 10mW/m2/nm e_FJ0430JPAS ? OAJ/JPAS.J0430 flux error 462- 469 E8.3 10mW/m2/nm FBGen ?=- Generic/Johnson.B flux 472- 479 E8.3 10mW/m2/nm e_FBGen ? Generic/Johnson.B flux error 481- 488 E8.3 10mW/m2/nm FJ0440 ?=- OAJ/JPAS.J0440 flux 491- 498 E8.3 10mW/m2/nm e_FJ0440 ? OAJ/JPAS.J0440 flux error 500- 507 E8.3 10mW/m2/nm FJ0450 ?=- OAJ/JPAS.J0450 flux 510- 517 E8.3 10mW/m2/nm e_FJ0450 ? OAJ/JPAS.J0450 flux error 519- 526 E8.3 10mW/m2/nm FJ0460 ?=- OAJ/JPAS.J0460 flux 529- 536 E8.3 10mW/m2/nm e_FJ0460 ? OAJ/JPAS.J0460 flux error 538- 545 E8.3 10mW/m2/nm FbGen ?=- Generic/Stromgren.b flux 548- 555 E8.3 10mW/m2/nm e_FbGen ? Generic/Stromgren.b flux error 557- 564 E8.3 10mW/m2/nm FbGCPD ?=- GCPD/Stromgren.b flux 567- 574 E8.3 10mW/m2/nm e_FbGCPD ? GCPD/Stromgren.b flux error 576- 583 E8.3 10mW/m2/nm FgSDSS ?=- SLOAN/SDSS.g flux 586- 593 E8.3 10mW/m2/nm e_FgSDSS ? SLOAN/SDSS.g flux error 595- 602 E8.3 10mW/m2/nm FgPar ?=- Paranal/OmegaCAM.g_SDSS flux 605- 612 E8.3 10mW/m2/nm e_FgPar ? Paranal/OmegaCAM.g_SDSS flux error 614- 621 E8.3 10mW/m2/nm FJ0470 ?=- OAJ/JPAS.J0470 flux 624- 631 E8.3 10mW/m2/nm e_FJ0470 ? OAJ/JPAS.J0470 flux error 633- 640 E8.3 10mW/m2/nm FgJPAS ?=- OAJ/JPAS.gSDSS flux error 643- 650 E8.3 10mW/m2/nm e_FgJPAS ? OAJ/JPAS.gSDSS flux error 652- 659 E8.3 10mW/m2/nm FgZTF ?=- Palomar/ZTF.g flux 662- 669 E8.3 10mW/m2/nm e_FgZTF ? Palomar/ZTF.g flux error 671- 678 E8.3 10mW/m2/nm FgJPLUS ?=- OAJ/JPLUS.gSDSS flux 681- 688 E8.3 10mW/m2/nm e_FgJPLUS ? OAJ/JPLUS.gSDSS flux error 690- 697 E8.3 10mW/m2/nm FgDEC ?=- CTIO/DECam.g flux 700- 707 E8.3 10mW/m2/nm e_FgDEC ? CTIO/DECam.g flux error 709- 716 E8.3 10mW/m2/nm FJ0480 ?=- OAJ/JPAS.J0480 flux 719- 726 E8.3 10mW/m2/nm e_FJ0480 ? OAJ/JPAS.J0480 flux error 728- 735 E8.3 10mW/m2/nm FgPS1 ?=- PAN-STARRS/PS1.g flux 738- 745 E8.3 10mW/m2/nm e_FgPS1 ? PAN-STARRS/PS1.g flux error 747- 754 E8.3 10mW/m2/nm FJ0490 ?=- OAJ/JPAS.J0490 flux 757- 764 E8.3 10mW/m2/nm e_FJ0490 ? OAJ/JPAS.J0490 flux error 766- 773 E8.3 10mW/m2/nm FJ0500 ?=- OAJ/JPAS.J0500 flux 776- 783 E8.3 10mW/m2/nm e_FJ0500 ? OAJ/JPAS.J0500 flux error 785- 792 E8.3 10mW/m2/nm FBP ?=- GAIA/GAIA3.Gbp flux 795- 802 E8.3 10mW/m2/nm e_FBP ? GAIA/GAIA3.Gbp flux error 804- 811 E8.3 10mW/m2/nm FJ0510 ?=- OAJ/JPAS.J0510 flux 814- 821 E8.3 10mW/m2/nm e_FJ0510 ? OAJ/JPAS.J0510 flux error 823- 830 E8.3 10mW/m2/nm FJ0515 ?=- OAJ/JPLUS.J0515 flux 833- 840 E8.3 10mW/m2/nm e_FJ0515 ? OAJ/JPLUS.J0515 flux error 842- 849 E8.3 10mW/m2/nm FJ0520 ?=- OAJ/JPAS.J0520 flux 852- 859 E8.3 10mW/m2/nm e_FJ0520 ? OAJ/JPAS.J0520 flux error 861- 868 E8.3 10mW/m2/nm FJ0530 ?=- OAJ/JPAS.J0530 flux 871- 878 E8.3 10mW/m2/nm e_FJ0530 ? OAJ/JPAS.J0530 flux error 880- 887 E8.3 10mW/m2/nm FVT ?=- TYCHO/TYCHO.V flux 890- 897 E8.3 10mW/m2/nm e_FVT ? TYCHO/TYCHO.V flux error 899- 906 E8.3 10mW/m2/nm FVAPASS ?=- Misc/APASS.V flux 909- 916 E8.3 10mW/m2/nm e_FVAPASS ? Misc/APASS.V flux error 918- 925 E8.3 10mW/m2/nm FJ0540 ?=- OAJ/JPAS.J0540 flux 928- 935 E8.3 10mW/m2/nm e_FJ0540 ? OAJ/JPAS.J0540 flux error 937- 944 E8.3 10mW/m2/nm FyGCPD ?=- GCPD/Stromgren.y flux 947- 954 E8.3 10mW/m2/nm e_FyGCPD ? GCPD/Stromgren.y flux error 956- 963 E8.3 10mW/m2/nm FVGen ?=- Generic/Johnson.V flux 966- 973 E8.3 10mW/m2/nm e_FVGen ? Generic/Johnson.V flux error 975- 982 E8.3 10mW/m2/nm FyGen ?=- Generic/Stromgren.y flux 985- 992 E8.3 10mW/m2/nm e_FyGen ? Generic/Stromgren.y flux error 994-1001 E8.3 10mW/m2/nm FJ0550 ?=- OAJ/JPAS.J0550 flux 1004-1011 E8.3 10mW/m2/nm e_FJ0550 ? OAJ/JPAS.J0550 flux error 1013-1020 E8.3 10mW/m2/nm FJ0560 ?=- OAJ/JPAS.J0560 flux 1023-1030 E8.3 10mW/m2/nm e_FJ0560 ? OAJ/JPAS.J0560 flux error 1032-1039 E8.3 10mW/m2/nm FJ0570 ?=- OAJ/JPAS.J0570 flux 1042-1049 E8.3 10mW/m2/nm e_FJ0570 ? OAJ/JPAS.J0570 flux error 1051-1058 E8.3 10mW/m2/nm FF606W ?=- HST/ACS_WFC.F606W flux 1061-1068 E8.3 10mW/m2/nm e_FF606W ? HST/ACS_WFC.F606W flux error 1070-1077 E8.3 10mW/m2/nm FJ0580 ?=- OAJ/JPAS.J0580 flux 1080-1087 E8.3 10mW/m2/nm e_FJ0580 ? OAJ/JPAS.J0580 flux error 1089-1096 E8.3 10mW/m2/nm FG ?=- GAIA/GAIA3.G flux 1099-1106 E8.3 10mW/m2/nm e_FG ? GAIA/GAIA3.G flux error 1108-1115 E8.3 10mW/m2/nm FJ0590 ?=- OAJ/JPAS.J0590 flux 1118-1125 E8.3 10mW/m2/nm e_FJ0590 ? OAJ/JPAS.J0590 flux error 1127-1134 E8.3 10mW/m2/nm FJ0600 ?=- OAJ/JPAS.J0600 flux 1137-1144 E8.3 10mW/m2/nm e_FJ0600 ? OAJ/JPAS.J0600 flux error 1146-1153 E8.3 10mW/m2/nm FJ0610 ?=- OAJ/JPAS.J0610 flux 1156-1163 E8.3 10mW/m2/nm e_FJ0610 ? OAJ/JPAS.J0610 flux error 1165-1172 E8.3 10mW/m2/nm FrSDSS ?=- SLOAN/SDSS.r flux 1175-1182 E8.3 10mW/m2/nm e_FrSDSS ? SLOAN/SDSS.r flux error 1184-1191 E8.3 10mW/m2/nm FgR ?=- INT/IPHAS.gR flux 1194-1201 E8.3 10mW/m2/nm e_FgR ? INT/IPHAS.gR flux error 1203-1210 E8.3 10mW/m2/nm FrPS1 ?=- PAN-STARRS/PS1.r flux 1213-1220 E8.3 10mW/m2/nm e_FrPS1 ? PAN-STARRS/PS1.r flux error 1222-1229 E8.3 10mW/m2/nm FrJPAS ?=- OAJ/JPAS.rSDSS flux 1232-1239 E8.3 10mW/m2/nm e_FrJPAS ? OAJ/JPAS.rSDSS flux error 1241-1248 E8.3 10mW/m2/nm FrJPLU ?=- OAJ/JPLUS.rSDSS flux 1251-1258 E8.3 10mW/m2/nm e_FrJPLU ? OAJ/JPLUS.rSDSS flux error 1260-1267 E8.3 10mW/m2/nm FJ0620 ?=- OAJ/JPAS.J0620 flux 1270-1277 E8.3 10mW/m2/nm e_FJ0620 ? OAJ/JPAS.J0620 flux error 1279-1286 E8.3 10mW/m2/nm FrPar ?=- Paranal/OmegaCAM.r_SDSS flux 1289-1296 E8.3 10mW/m2/nm e_FrPar ? Paranal/OmegaCAM.r_SDSS flux error 1298-1305 E8.3 10mW/m2/nm FJ0630 ?=- OAJ/JPAS.J0630 flux 1308-1315 E8.3 10mW/m2/nm e_FJ0630 ? OAJ/JPAS.J0630 flux error 1317-1324 E8.3 10mW/m2/nm FrZTF ?=- Palomar/ZTF.r flux 1327-1334 E8.3 10mW/m2/nm e_FrZTF ? Palomar/ZTF.r flux error 1336-1343 E8.3 10mW/m2/nm FrDEC ?=- CTIO/DECam.r flux 1346-1353 E8.3 10mW/m2/nm e_FrDEC ? CTIO/DECam.r flux error 1355-1362 E8.3 10mW/m2/nm FJ0640 ?=- OAJ/JPAS.J0640 flux 1365-1372 E8.3 10mW/m2/nm e_FJ0640 ? OAJ/JPAS.J0640 flux error 1374-1381 E8.3 10mW/m2/nm FJ0650 ?=- OAJ/JPAS.J0650 flux 1384-1391 E8.3 10mW/m2/nm e_FJ0650 ? OAJ/JPAS.J0650 flux error 1393-1400 E8.3 10mW/m2/nm FHaINT ?=- INT/IPHAS.Ha flux 1403-1410 E8.3 10mW/m2/nm e_FHaINT ? INT/IPHAS.Ha flux error 1412-1419 E8.3 10mW/m2/nm FHaPar ?=- Paranal/OmegaCAM.Halpha flux 1422-1429 E8.3 10mW/m2/nm e_FHaPar ? Paranal/OmegaCAM.Halpha flux error 1431-1438 E8.3 10mW/m2/nm FJ0660JPLUS ?=- OAJ/JPLUS.J0660 flux 1441-1448 E8.3 10mW/m2/nm e_FJ0660JPLUS ? OAJ/JPLUS.J0660 flux error 1450-1457 E8.3 10mW/m2/nm FJ0660JPAS ?=- OAJ/JPAS.J0660 flux 1460-1467 E8.3 10mW/m2/nm e_FJ0660JPAS ? OAJ/JPAS.J0660 flux error 1469-1476 E8.3 10mW/m2/nm FRcGen ?=- Generic/Johnson.R flux 1479-1486 E8.3 10mW/m2/nm e_FRcGen ? Generic/Johnson.R flux error 1488-1495 E8.3 10mW/m2/nm FJ0670JPAS ?=- OAJ/JPAS.J0670 flux 1498-1505 E8.3 10mW/m2/nm e_FJ0670JPAS ? OAJ/JPAS.J0670 flux error 1507-1514 E8.3 10mW/m2/nm FJ0680 ?=- OAJ/JPAS.J0680 flux 1517-1524 E8.3 10mW/m2/nm e_FJ0680 ? OAJ/JPAS.J0680 flux error 1526-1533 E8.3 10mW/m2/nm FJ0690 ?=- OAJ/JPAS.J0690 flux 1536-1543 E8.3 10mW/m2/nm e_FJ0690 ? OAJ/JPAS.J0690 flux error 1545-1552 E8.3 10mW/m2/nm FJ0700 ?=- OAJ/JPAS.J0700 flux 1555-1562 E8.3 10mW/m2/nm e_FJ0700 ? OAJ/JPAS.J0700 flux error 1564-1571 E8.3 10mW/m2/nm FJ0710 ?=- OAJ/JPAS.J0710 flux 1574-1581 E8.3 10mW/m2/nm e_FJ0710 ? OAJ/JPAS.J0710 flux error 1583-1591 E9.3 10mW/m2/nm FJ0720 ?=- OAJ/JPAS.J0720 flux 1594-1601 E8.3 10mW/m2/nm e_FJ0720 ?=- OAJ/JPAS.J0720 flux error 1603-1610 E8.3 10mW/m2/nm FJ0730 ?=- OAJ/JPAS.J0730 flux 1613-1620 E8.3 10mW/m2/nm e_FJ0730 ? OAJ/JPAS.J0730 flux error 1622-1629 E8.3 10mW/m2/nm FJ0740 ?=- OAJ/JPAS.J0740 flux 1632-1639 E8.3 10mW/m2/nm e_FJ0740 ? OAJ/JPAS.J0740 flux error 1641-1648 E8.3 10mW/m2/nm FiSDSS ?=- SLOAN/SDSS.i flux 1651-1658 E8.3 10mW/m2/nm e_FiSDSS ? SLOAN/SDSS.i flux error 1660-1667 E8.3 10mW/m2/nm FJ0750 ?=- OAJ/JPAS.J0750 flux 1670-1677 E8.3 10mW/m2/nm e_FJ0750 ? OAJ/JPAS.J0750 flux error 1679-1686 E8.3 10mW/m2/nm FiPS1 ?=- PAN-STARRS/PS1.i flux 1689-1696 E8.3 10mW/m2/nm e_FiPS1 ? PAN-STARRS/PS1.i flux error 1698-1705 E8.3 10mW/m2/nm FiPar ?=- Paranal/OmegaCAM.i_SDSS flux 1708-1715 E8.3 10mW/m2/nm e_FiPar ? Paranal/OmegaCAM.i_SDSS flux error 1717-1724 E8.3 10mW/m2/nm FJ0760 ?=- OAJ/JPAS.J0760 flux 1727-1734 E8.3 10mW/m2/nm e_FJ0760 ? OAJ/JPAS.J0760 flux error 1736-1743 E8.3 10mW/m2/nm FiJPLUS ?=- OAJ/JPLUS.iSDSS flux 1746-1753 E8.3 10mW/m2/nm e_FiJPLUS ? OAJ/JPLUS.iSDSS flux error 1755-1762 E8.3 10mW/m2/nm FiKOS ?=- OAJ/JPAS.iSDSS flux 1765-1772 E8.3 10mW/m2/nm e_FiKOS ? OAJ/JPAS.iSDSS flux error 1774-1781 E8.3 10mW/m2/nm FRP ?=- GAIA/GAIA3.Grp flux 1784-1791 E8.3 10mW/m2/nm e_FRP ? GAIA/GAIA3.Grp flux error 1793-1800 E8.3 10mW/m2/nm FgI ?=- INT/IPHAS.gI flux 1803-1810 E8.3 10mW/m2/nm e_FgI ? INT/IPHAS.gI flux error 1812-1819 E8.3 10mW/m2/nm FJ0770 ?=- OAJ/JPAS.J0770 flux 1822-1829 E8.3 10mW/m2/nm e_FJ0770 ? OAJ/JPAS.J0770 flux error 1831-1838 E8.3 10mW/m2/nm FiDEC ?=- CTIO/DECam.i flux 1841-1848 E8.3 10mW/m2/nm e_FiDEC ? CTIO/DECam.i flux error 1850-1858 E9.3 10mW/m2/nm FJ0780 ?=- OAJ/JPAS.J0780 flux 1861-1868 E8.3 10mW/m2/nm e_FJ0780 ? OAJ/JPAS.J0780 flux error 1870-1877 E8.3 10mW/m2/nm FiZTF ?=- Palomar/ZTF.i flux 1880-1887 E8.3 10mW/m2/nm e_FiZTF ? Palomar/ZTF.i flux error 1889-1896 E8.3 10mW/m2/nm FID ?=- DENIS/DENIS.I flux 1899-1906 E8.3 10mW/m2/nm e_FID ? DENIS/DENIS.I flux error 1908-1915 E8.3 10mW/m2/nm FJ0790 ?=- OAJ/JPAS.J0790 flux 1918-1925 E8.3 10mW/m2/nm e_FJ0790 ? OAJ/JPAS.J0790 flux error 1927-1934 E8.3 10mW/m2/nm FF814W ?=- HST/ACS_WFC.F814W flux 1937-1944 E8.3 10mW/m2/nm e_FF814W ? HST/ACS_WFC.F814W flux error 1946-1953 E8.3 10mW/m2/nm FJ0800 ?=- OAJ/JPAS.J0800 flux 1956-1963 E8.3 10mW/m2/nm e_FJ0800 ? OAJ/JPAS.J0800 flux error 1965-1972 E8.3 10mW/m2/nm FJ0810 ?=- OAJ/JPAS.J0810 flux 1975-1982 E8.3 10mW/m2/nm e_FJ0810 ? OAJ/JPAS.J0810 flux error 1984-1991 E8.3 10mW/m2/nm FJ0820 ?=- OAJ/JPAS.J0820 flux 1994-2001 E8.3 10mW/m2/nm e_FJ0820 ? OAJ/JPAS.J0820 flux error 2003-2010 E8.3 10mW/m2/nm FJ0830 ?=- OAJ/JPAS.J0830 flux 2013-2020 E8.3 10mW/m2/nm e_FJ0830 ? OAJ/JPAS.J0830 flux error 2022-2029 E8.3 10mW/m2/nm FJ0840 ?=- OAJ/JPAS.J0840 flux 2032-2039 E8.3 10mW/m2/nm e_FJ0840 ? OAJ/JPAS.J0840 flux error 2041-2048 E8.3 10mW/m2/nm FJ0850 ?=- OAJ/JPAS.J0850 flux 2051-2058 E8.3 10mW/m2/nm e_FJ0850 ? OAJ/JPAS.J0850 flux error 2060-2067 E8.3 10mW/m2/nm FIGen ?=- Generic/Johnson.I flux 2070-2077 E8.3 10mW/m2/nm e_FIGen ? Generic/Johnson.I flux error 2079-2086 E8.3 10mW/m2/nm FGrvs ?=- GAIA/GAIA3.Grvs flux 2089-2096 E8.3 10mW/m2/nm e_FGrvs ? GAIA/GAIA3.Grvs flux error 2098-2105 E8.3 10mW/m2/nm FJ0860 ?=- OAJ/JPAS.J0860 flux 2108-2115 E8.3 10mW/m2/nm e_FJ0860 ? OAJ/JPAS.J0860 flux error 2117-2124 E8.3 10mW/m2/nm FJ0861 ?=- OAJ/JPLUS.J0861 flux 2127-2134 E8.3 10mW/m2/nm e_FJ0861 ? OAJ/JPLUS.J0861 flux error 2136-2143 E8.3 10mW/m2/nm FzPS1 ?=- PAN-STARRS/PS1.z flux 2146-2153 E8.3 10mW/m2/nm e_FzPS1 ? PAN-STARRS/PS1.z flux error 2155-2162 E8.3 10mW/m2/nm FJ0870 ?=- OAJ/JPAS.J0870 flux 2165-2172 E8.3 10mW/m2/nm e_FJ0870 ? OAJ/JPAS.J0870 flux error 2174-2181 E8.3 10mW/m2/nm FZPar ?=- Paranal/VISTA.Z flux 2184-2191 E8.3 10mW/m2/nm e_FZPar ? Paranal/VISTA.Z flux error 2193-2200 E8.3 10mW/m2/nm FZ ?=- UKIRT/UKIDSS.Z flux 2203-2210 E8.3 10mW/m2/nm e_FZ ? UKIRT/UKIDSS.Z flux error 2212-2219 E8.3 10mW/m2/nm FJ0880 ?=- OAJ/JPAS.J0880 flux 2222-2229 E8.3 10mW/m2/nm e_FJ0880 ? OAJ/JPAS.J0880 flux error 2231-2238 E8.3 10mW/m2/nm FJ0890 ?=- OAJ/JPAS.J0890 flux 2241-2248 E8.3 10mW/m2/nm e_FJ0890 ? OAJ/JPAS.J0890 flux error 2250-2257 E8.3 10mW/m2/nm FzSDSS ?=- SLOAN/SDSS.z flux 2260-2267 E8.3 10mW/m2/nm e_FzSDSS ? SLOAN/SDSS.z flux error 2269-2276 E8.3 10mW/m2/nm FzJPLUS ?=- OAJ/JPLUS.zSDSS flux 2279-2286 E8.3 10mW/m2/nm e_FzJPLUS ? OAJ/JPLUS.zSDSS flux error 2288-2295 E8.3 10mW/m2/nm FJ0900 ?=- OAJ/JPAS.J0900 flux 2298-2305 E8.3 10mW/m2/nm e_FJ0900 ? OAJ/JPAS.J0900 flux error 2307-2314 E8.3 10mW/m2/nm FJ0910 ?=- OAJ/JPAS.J0910 flux 2317-2324 E8.3 10mW/m2/nm e_FJ0910 ? OAJ/JPAS.J0910 flux error 2326-2333 E8.3 10mW/m2/nm FzDEC ?=- CTIO/DECam.z flux 2336-2343 E8.3 10mW/m2/nm e_FzDEC ? CTIO/DECam.z flux error 2345-2352 E8.3 10mW/m2/nm FJ1007 ?=- OAJ/JPAS.J1007 flux 2355-2362 E8.3 10mW/m2/nm e_FJ1007 ? OAJ/JPAS.J1007 flux error 2364-2371 E8.3 10mW/m2/nm FyPS1 ?=- PAN-STARRS/PS1.y flux 2374-2381 E8.3 10mW/m2/nm e_FyPS1 ? PAN-STARRS/PS1.y flux error 2383-2390 E8.3 10mW/m2/nm FYDEC ?=- CTIO/DECam.Y flux 2393-2400 E8.3 10mW/m2/nm e_FYDEC ? CTIO/DECam.Y flux error 2402-2409 E8.3 10mW/m2/nm FYPar ?=- Paranal/VISTA.Y flux 2412-2419 E8.3 10mW/m2/nm e_FYPar ? Paranal/VISTA.Y flux error 2421-2428 E8.3 10mW/m2/nm FY ?=- UKIRT/UKIDSS.Y flux 2431-2438 E8.3 10mW/m2/nm e_FY ? UKIRT/UKIDSS.Y flux error 2440-2447 E8.3 10mW/m2/nm FJD ?=- DENIS/DENIS.J flux 2450-2457 E8.3 10mW/m2/nm e_FJD ? DENIS/DENIS.J flux error 2458 A1 --- l_FJ2 Limit flag on FJ2 2459-2466 E8.3 10mW/m2/nm FJ2 ?=- 2MASS/2MASS.J flux 2469-2476 E8.3 10mW/m2/nm e_FJ2 ? 2MASS/2MASS.J flux error 2478-2485 E8.3 10mW/m2/nm FJPar ?=- Paranal/VISTA.J flux 2488-2495 E8.3 10mW/m2/nm e_FJPar ? Paranal/VISTA.J flux error 2497-2504 E8.3 10mW/m2/nm FJ ?=- UKIRT/UKIDSS.J flux 2507-2514 E8.3 10mW/m2/nm e_FJ ? UKIRT/UKIDSS.J flux error 2516-2523 E8.3 10mW/m2/nm FH ?=- UKIRT/UKIDSS.H flux 2526-2533 E8.3 10mW/m2/nm e_FH ? UKIRT/UKIDSS.H flux error 2535-2542 E8.3 10mW/m2/nm FHPar ?=- Paranal/VISTA.H flux 2545-2552 E8.3 10mW/m2/nm e_FHPar ? Paranal/VISTA.H flux error 2553 A1 --- l_FH2 Limit flag on FH2 2554-2561 E8.3 10mW/m2/nm FH2 ?=- 2MASS/2MASS.H flux 2564-2571 E8.3 10mW/m2/nm e_FH2 ? 2MASS/2MASS.H flux error 2573-2580 E8.3 10mW/m2/nm FKsPar ?=- Paranal/VISTA.Ks flux 2583-2590 E8.3 10mW/m2/nm e_FKsPar ? Paranal/VISTA.Ks flux error 2592-2599 E8.3 10mW/m2/nm FKsD ?=- DENIS/DENIS.Ks flux 2602-2609 E8.3 10mW/m2/nm e_FKsD ? DENIS/DENIS.Ks flux error 2610 A1 ---- l_FKs2 Limit flag on FKs2 2611-2618 E8.3 10mW/m2/nm FKs2 ?=- 2MASS/2MASS.Ks flux 2621-2628 E8.3 10mW/m2/nm e_FKs2 ? 2MASS/2MASS.Ks flux error 2630-2637 E8.3 10mW/m2/nm FK ?=- UKIRT/UKIDSS.K flux 2640-2647 E8.3 10mW/m2/nm e_FK ? UKIRT/UKIDSS.K flux error 2648 A1 --- l_FW1 Limit flag on FW1 2649-2656 E8.3 10mW/m2/nm FW1 ?=- WISE/WISE.W1 flux 2659-2666 E8.3 10mW/m2/nm e_FW1 ? WISE/WISE.W1 flux error 2668-2675 E8.3 10mW/m2/nm FIRAC1 ?=- Spitzer/IRAC.I1 flux 2678-2685 E8.3 10mW/m2/nm e_FIRAC1 ? Spitzer/IRAC.I1 flux error 2687-2694 E8.3 10mW/m2/nm FB1 ?=- MSX/MSX.B1 flux 2697-2704 E8.3 10mW/m2/nm e_FB1 ? MSX/MSX.B1 flux error 2706-2713 E8.3 10mW/m2/nm FB2 ?=- MSX/MSX.B2 flux 2716-2723 E8.3 10mW/m2/nm e_FB2 ? MSX/MSX.B2 flux error 2725-2732 E8.3 10mW/m2/nm FIRAC2 ?=- Spitzer/IRAC.I2 flux 2735-2742 E8.3 10mW/m2/nm e_FIRAC2 ? Spitzer/IRAC.I2 flux error 2743 A1 --- l_FW2 Limit flag on FW2 2744-2751 E8.3 10mW/m2/nm FW2 ?=- WISE/WISE.W2 flux 2754-2761 E8.3 10mW/m2/nm e_FW2 ? WISE/WISE.W2 flux error 2763-2770 E8.3 10mW/m2/nm FIRAC3 ?=- Spitzer/IRAC.I3 flux 2773-2780 E8.3 10mW/m2/nm e_FIRAC3 ? Spitzer/IRAC.I3 flux error 2782-2789 E8.3 10mW/m2/nm FIRAC4 ?=- Spitzer/IRAC.I4 flux 2792-2799 E8.3 10mW/m2/nm e_FIRAC4 ? Spitzer/IRAC.I4 flux error 2801-2808 E8.3 10mW/m2/nm FA ?=- MSX/MSX.A flux 2811-2818 E8.3 10mW/m2/nm e_FA ? MSX/MSX.A flux error 2820-2827 E8.3 10mW/m2/nm FS9W ?=- AKARI/IRC.S9W flux 2830-2837 E8.3 10mW/m2/nm e_FS9W ? AKARI/IRC.S9W flux error 2838 A1 --- l_F12 Limit flag on F12 2839-2846 E8.3 10mW/m2/nm F12 ?=- IRAS/IRAS.12mu flux 2849-2856 E8.3 10mW/m2/nm e_F12 ? IRAS/IRAS.12mu flux error 2857 A1 --- l_FW3 Limit flag on FW3 2858-2865 E8.3 10mW/m2/nm FW3 ?=- WISE/WISE.W3 flux 2868-2875 E8.3 10mW/m2/nm e_FW3 ? WISE/WISE.W3 flux error 2877-2884 E8.3 10mW/m2/nm FC ?=- MSX/MSX.C flux 2887-2894 E8.3 10mW/m2/nm e_FC ? MSX/MSX.C flux error 2896-2903 E8.3 10mW/m2/nm FD ?=- MSX/MSX.D flux 2906-2913 E8.3 10mW/m2/nm e_FD ? MSX/MSX.D flux error 2915-2922 E8.3 10mW/m2/nm FL19W ?=- AKARI/IRC.L18W flux 2925-2932 E8.3 10mW/m2/nm e_FL19W ? AKARI/IRC.L18W flux error 2934-2941 E8.3 10mW/m2/nm FE ?=- MSX/MSX.E flux 2944-2951 E8.3 10mW/m2/nm e_FE ? MSX/MSX.E flux error 2953-2961 E9.3 10mW/m2/nm F25 ?=- IRAS/IRAS.25mu flux 2964-2971 E8.3 10mW/m2/nm e_F25 ? IRAS/IRAS.25mu flux error 2972 A1 --- l_FW4 Limit flag on FW4 2973-2980 E8.3 10mW/m2/nm FW4 ?=- WISE/WISE.W4 flux 2983-2990 E8.3 10mW/m2/nm e_FW4 ? WISE/WISE.W4 flux error 2992 A1 --- l_F60 Limit flag on F60 2993-3000 E8.3 10mW/m2/nm F60 ?=- IRAS/IRAS.60mu flux 3003-3010 E8.3 10mW/m2/nm e_F60 ? IRAS/IRAS.60mu flux error 3012-3019 E8.3 10mW/m2/nm FN50 ?=- AKARI/FIS.N60 flux 3022-3029 E8.3 10mW/m2/nm e_FN50 ? AKARI/FIS.N60 flux error 3031-3039 E9.3 10mW/m2/nm FWIDE-S ?=- AKARI/FIS.WIDE-S flux 3042-3049 E8.3 10mW/m2/nm e_FWIDE-S ? AKARI/FIS.WIDE-S flux error 3050 A1 --- l_F100 Limit flag on F100 3051-3058 E8.3 10mW/m2/nm F100 ?=- IRAS/IRAS.100mu flux 3061-3068 E8.3 10mW/m2/nm e_F100 ? IRAS/IRAS.100mu flux error 3070-3077 E8.3 10mW/m2/nm FWIDE-L ?=- AKARI/FIS.WIDE-L flux 3080-3087 E8.3 10mW/m2/nm e_FWIDE-L ? AKARI/FIS.WIDE-L flux error 3089-3096 E8.3 10mW/m2/nm FN160 ?=- AKARI/FIS.N160 flux 3099-3106 E8.3 10mW/m2/nm e_FN160 ? AKARI/FIS.N160 flux error -------------------------------------------------------------------------------- Acknowledgements: Iker Gonzalez-Santamaria, iker.gonzalez(at)udc.es History: 23-Aug-2024: on-line version 05-May-2025: table A1 added
(End) I. Gonzalez-Santamaria [Univ. Coruna], P. Vannier [CDS] 04-Jul-2024
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line