J/A+A/690/A33    Core mass function in high-mass star formation  (Louvet+, 2024)

ALMA-IMF XV. Core mass function in the high-mass star formation regime. Louvet F., Sanhueza P., Stutz A., Men'shchikov A., Motte F., Galvan-Madrid R., Bontemps S., Pouteau Y., Ginsburg A., Csengeri T., Di Francesco J., Dell'Ova P., Gonzalez M., Didelon P., Braine J., Cunningham N., Thomasson B., Lesaffre P., Hennebelle P., Bonfand M., Gusdorf A., Alverez-Gutierrez R.H., Nony T., Busquet G., Olguin F., Bronfman L., Salinas J., Fernandez-Lopez M., Moraux E., Liu H.L., Lu X., Huei-Ru V., Towner A., Valeille-Manet M., Brouillet N., Herpin F., Lefloch B., Baug T., Maud L., Lopez-Sepulcre A., Svodoba B. <Astron. Astrophys. 690, A33 (2024)> =2024A&A...690A..33L 2024A&A...690A..33L (SIMBAD/NED BibCode)
ADC_Keywords: Milky Way ; Molecular clouds ; Infrared ; Millimetric/submm sources ; Morphology ; Stars, masses Keywords: methods: observational - techniques: interferometric - stars: formation - ISM: clouds - ISM: structure - submillimeter: ISM Abstract: The stellar initial mass function (IMF) is critical to our understanding of star formation and the effects of young stars on their environment. On large scales, it enables us to use tracers such as UV or Halpha emission to estimate the star formation rate of a system and interpret unresolved star clusters across the Universe. So far, there is little firm evidence of large-scale variations of the IMF, which is thus generally considered "universal". Stars form from cores, and it is now possible to estimate core masses and compare the core mass function (CMF) with the IMF, which it presumably produces. The goal of the ALMA-IMF large programme is to measure the core mass function at high linear resolution (2700au) in 15 typical Milky Way protoclusters spanning a mass range of 2500 to 32700M. In this work, we used two different core extraction algorithms to extract about 680 gravitationally bound cores from these 15 protoclusters. We adopted a per core temperature using the temperature estimate from the point-process mapping Bayesian method (PPMAP). A power-law fit to the CMF of the sub-sample of cores above the 1.64 Msun completeness limit (330 cores) through the maximum likelihood estimate technique yields a slope of 1.97±0.06, which is significantly flatter than the 2.35 Salpeter slope. Assuming a self-similar mapping between the CMF and the IMF, this result implies that these 15 high-mass protoclusters will generate atypical IMFs. This sample currently is the largest sample that was produced and analysed self-consistently, derived at matched physical resolution, with per core temperature estimates, and cores as massive as 150 Msun. We provide both the raw source extraction catalogues and the catalogues listing the source size, temperature, mass, spectral indices, and so on in the 15 protoclusters. Description: We provide the continuum source catalogues from the Atacama Large Millimetre/submillimetre Array (ALMA) large program ALMA-IMF. We observed 15 high-mass star-forming regions. For each region we provide the raw source extractions catalogues from two source extraction algorithms (getsf and GExt2D) at the observed angular resolution and at the smoothed angular resolution corresponding to a physical scale of 2700 au on target. We also provide the post-processed source catalogues at the native and smoothed angular resolution. That is 6 catalogues per regions, hence 90 catalogues in total. Objects: ------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------- 15 53 08.130 -54 37 08.60 G327.29 15 57 59.680 -53 57 57.43 G328.25 16 41 10.620 -47 08 02.90 G337.92 16 40 34.420 -45 41 40.60 G338.93 18 47 47.000 -01 54 26.00 W43-MM1 18 47 36.610 -02 00 51.10 W43-MM2 18 47 41.460 -02 00 27.60 W43-MM3 19 23 44.180 +14 30 29.50 W51-E 17 26 42.620 -36 09 22.47 G351.77 17 30 26.280 -34 41 51.67 G353.41 18 06 21.072 -21 37 14.84 G008.67 18 10 28.840 -19 55 48.30 G010.62 18 14 13.370 -17 55 47.17 G012.80 16 22 09.360 -50 06 00.87 G333.60 19 23 39.810 +14 31 03.50 W51-IRS2 ------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file g008cn.dat 214 22 Source features in G008 (native) g008cs.dat 214 20 Source features in G008 (smoothed) g008dn.dat 262 22 GExt2D source extraction in G008 (native) g008ss.dat 262 30 GExt2D source extraction in G008 (smoothed) g008gn.dat 638 24 getsf source extraction in G008 (native) g008gs.dat 638 25 getsf source extraction in G008 (smoothed) g010cn.dat 214 56 Source features in G008 (native) g010cs.dat 214 50 Source features in G008 (smoothed) g010dn.dat 262 51 GExt2D source extraction in G010 (native) g010ss.dat 262 59 GExt2D source extraction in G010 (smoothed) g010gn.dat 638 73 getsf source extraction in G010 (native) g010gs.dat 638 63 getsf source extraction in G010 (smoothed) g012cn.dat 214 81 Source features in G012 (native) g012cs.dat 214 57 Source features in G012 (smoothed) g012dn.dat 262 108 GExt2D source extraction in G012 (native) g012ss.dat 262 125 GExt2D source extraction in G012 (smoothed) g012gn.dat 638 89 getsf source extraction in G012 (native) g012gs.dat 638 67 getsf source extraction in G012 (smoothed) g327cn.dat 214 41 Source features in G327 (native) g327cs.dat 214 32 Source features in G327 (smoothed) g327dn.dat 262 41 GExt2D source extraction in G327 (native) g327ss.dat 262 49 GExt2D source extraction in G327 (smoothed) g327gn.dat 638 49 getsf source extraction in G327 (native) g327gs.dat 638 35 getsf source extraction in G327 (smoothed) g328cn.dat 214 17 Source features in G328 (native) g328cs.dat 214 11 Source features in G328 (smoothed) g328dn.dat 262 36 GExt2D source extraction in G328 (native) g328ss.dat 262 26 GExt2D source extraction in G328 (smoothed) g328gn.dat 638 20 getsf source extraction in G328 (native) g328gs.dat 638 11 getsf source extraction in G328 (smoothed) g333cn.dat 214 115 Source features in G333 (native) g333cs.dat 214 95 Source features in G333 (smoothed) g333dn.dat 262 177 GExt2D source extraction in G333 (native) g333ss.dat 262 175 GExt2D source extraction in G333 (smoothed) g333gn.dat 638 139 getsf source extraction in G333 (native) g333gs.dat 638 123 getsf source extraction in G333 (smoothed) g337cn.dat 214 36 Source features in G337 (native) g337cs.dat 214 22 Source features in G337 (smoothed) g337dn.dat 262 37 GExt2D source extraction in G337 (native) g337ss.dat 262 42 GExt2D source extraction in G337 (smoothed) g337gn.dat 638 47 getsf source extraction in G337 (native) g337gs.dat 638 25 getsf source extraction in G337 (smoothed) g338cn.dat 214 44 Source features in G338 (native) g338cs.dat 214 42 Source features in G338 (smoothed) g338dn.dat 262 32 GExt2D source extraction in G338 (native) g338ss.dat 262 50 GExt2D source extraction in G338 (smoothed) g338gn.dat 638 51 getsf source extraction in G338 (native) g338gs.dat 638 47 getsf source extraction in G338 (smoothed) g351cn.dat 214 24 Source features in G351 (native) g351cs.dat 214 19 Source features in G351 (smoothed) g351dn.dat 262 31 GExt2D source extraction in G351 (native) g351ss.dat 262 40 GExt2D source extraction in G351 (smoothed) g351gn.dat 638 34 getsf source extraction in G351 (native) g351gs.dat 638 24 getsf source extraction in G351 (smoothed) g353cn.dat 214 61 Source features in G353 (native) g353cs.dat 214 46 Source features in G353 (smoothed) g353dn.dat 262 65 GExt2D source extraction in G353 (native) g353ss.dat 262 68 GExt2D source extraction in G353 (smoothed) g353gn.dat 638 70 getsf source extraction in G353 (native) g353gs.dat 638 47 getsf source extraction in G353 (smoothed) w43mm1cn.dat 214 72 Source features in W43-MM1 (native) w43mm1cs.dat 214 71 Source features in W43-MM1 (smoothed) w43mm1dn.dat 262 89 GExt2D source extraction in W43-MM1 (native) w43mm1ss.dat 262 94 GExt2D source extraction in W43-MM1 (smoothed) w43mm1gn.dat 638 81 getsf source extraction in W43-MM1 (native) w43mm1gs.dat 638 76 getsf source extraction in W43-MM1 (smoothed) w43mm2cn.dat 214 39 Source features in W43-MM2 (native) w43mm2cs.dat 214 40 Source features in W43-MM2 (smoothed) w43mm2dn.dat 262 31 GExt2D source extraction in W43-MM2 (native) w43mm2ss.dat 262 34 GExt2D source extraction in W43-MM2 (smoothed) w43mm2gn.dat 638 46 getsf source extraction in W43-MM2 (native) w43mm2gs.dat 638 48 getsf source extraction in W43-MM2 (smoothed) w43mm3cn.dat 214 33 Source features in W43-MM3 (native) w43mm3cs.dat 214 37 Source features in W43-MM3 (smoothed) w43mm3dn.dat 262 20 GExt2D source extraction in W43-MM3 (native) w43mm3ss.dat 262 21 GExt2D source extraction in W43-MM3 (smoothed) w43mm3gn.dat 638 38 getsf source extraction in W43-MM3 (native) w43mm3gs.dat 638 42 getsf source extraction in W43-MM3 (smoothed) w51ecn.dat 214 49 Source features in W51-E (native) w51ecs.dat 214 31 Source features in W51-E (smoothed) w51edn.dat 262 64 GExt2D source extraction in W51-E (native) w51ess.dat 262 75 GExt2D source extraction in W51-E (smoothed) w51egn.dat 638 69 getsf source extraction in W51-E (native) w51egs.dat 638 41 getsf source extraction in W51-E (smoothed) w51ir2cn.dat 214 111 Source features in W51-IRS2 (native) w51ir2cs.dat 214 109 Source features in W51-IRS2 (smoothed) w51ir2dn.dat 262 130 GExt2D source extraction in W51-IRS2 (native) w51ir2ss.dat 262 136 GExt2D source extraction in W51-IRS2 (smoothed) w51ir2gn.dat 638 129 getsf source extraction in W51-IRS2 (native) w51ir2gs.dat 638 127 getsf source extraction in W51-IRS2 (smoothed) ori/* . 91 Original files -------------------------------------------------------------------------------- Byte-by-byte Description of file: *c[ns].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Proto-cluster name 10- 12 I3 --- Seq Number of the source 15- 31 A17 --- CoreName Name of the source (JDDD.dddd+DD.dddd) 37- 38 I2 h RAh Right Ascension of the source (J2000) 40- 41 I2 min RAm Right Ascension of the source (J2000) 43- 47 F5.2 s RAs Right Ascension of the source (J2000) 51 A1 --- DE- Declination sign of the source (J2000) 52- 53 I2 deg DEd Declination sign of the source (J2000) 55- 56 I2 arcmin DEm Declination sign of the source (J2000) 58- 62 F5.2 arcsec DEs Declination sign of the source (J2000) 66- 69 F4.2 arcsec amaj1.3mm Size of the source at 1.3mm 70 A1 --- --- [x] 71- 74 F4.2 arcsec bmin1.3mm Size of the source at 1.3mm 77- 79 I3 deg PA1.3mm Position angle of the source at 1.3mm 82- 87 F6.1 mJy/beam Speak1.3mm Peak flux of the source at 1.3mm 89- 92 F4.1 mJy/beam e_Speak1.3mm Peak flux of the source at 1.3mm error 97-102 F6.1 mJy Sint1.3mm Integrated intensity of the source at 1.3mm 104-107 F4.1 mJy e_Sint1.3mm Integrated intensity of the source at 1.3mm error 112-115 F4.2 arcsec amaj3mm ? Size of the source at 3mm 116 A1 --- --- [x] 117-120 F4.2 arcsec bmin3mm ? Size of the source at 3mm 123-125 I3 deg PA3mm ? Position angle of the source at 3mm 130-134 F5.1 mJy/beam Speak3mm ? Peak flux of the source at 3mm 136-139 F4.1 mJy/beam e_Speak3mm ? Peak flux of the source at 3mm error 141-146 F6.1 mJy Sint3mm ? Integrated intensity of the source at 3mm 148-151 F4.1 mJy e_Sint3mm ? Integrated intensity of the source at 3mm error 158-160 I3 K T ? Temperature of the source 162-164 I3 K e_T ? Temperature of the source error 167-171 F5.1 Msun Mass ? Mass of the source 173-175 F3.1 Msun e_Mass ? Mass of the source error 185-188 I4 au Size Size of the source at 1.3mm 193 A1 --- l_alphaBE Limit flag on alphaBE 194-197 F4.2 --- alphaBE ? Bonnor-Ebert virial parameter 204-207 F4.1 --- alpha ? Spectral index of the source 214 A1 --- GExt2D indicate if the source was detected by GExt2D, True (T) or False (F) -------------------------------------------------------------------------------- Byte-by-byte Description of file: *dn.dat *ss.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Proto-cluster name 13- 15 I3 --- Seq Number of the source 19- 21 I3 --- Seqori Original Number of the source 24- 34 F11.7 deg RAdeg Right Ascension of the source (J2000) 37- 47 F11.7 deg DEdeg Declination of the source (J2000) 51- 55 F5.3 arcsec dx1 B6 band (1.3mm) Size of the source 59- 63 F5.3 arcsec dy1 B6 band (1.3mm) Size of the source 65- 70 F6.1 deg PA1 [] B6 band (1.3mm) Position angle of the source 76- 80 F5.2 --- snr1 B6 band (1.3mm) Signal-to-noise ratio 86- 90 F5.2 --- snrpeak1 B6 band (1.3mm) Peak Signal-to-noise ratio 95-102 F8.3 mJy/beam Speak1 B6 band (1.3mm) Peak flux of the source 109-114 F6.3 mJy/beam e_Speak1 B6 band (1.3mm) Peak flux of the source error 119-126 F8.3 mJy SInt1 B6 band (1.3mm) Integrated intensity of the source 132-138 F7.3 mJy e_SInt1 B6 band (1.3mm) Integrated intensity of the source error 144-150 F7.3 mJy Bkg1 B6 band (1.3mm) background 154-159 F6.2 --- Qual B6 band (1.3mm) quality flag 162-167 F6.3 arcsec dx2 ?=-1 B3 band (3mm) Size of the source 170-175 F6.3 arcsec dy2 ?=-1 B3 band (3mm) Size of the source 177-182 F6.1 deg PA2 []?=-1 B3 band (3mm) Position angle of the source 188-192 F5.2 --- snr2 ?=-1 B3 band (3mm) Signal-to-noise ratio 198-202 F5.2 --- snrpeak2 ?=-1 B3 band (3mm) Peak Signal-to-noise ratio 208-214 F7.3 mJy/beam Speak2 ?=-1 B3 band (3mm) Peak flux of the source 221-226 F6.3 mJy/beam e_Speak2 ?=-1 B3 band (3mm) Peak flux of the source error 231-238 F8.3 mJy SInt2 ?=-1 B3 band (3mm) Integrated intensity of the source 244-250 F7.3 mJy e_SInt2 ?=-1 B3 band (3mm) Integrated intensity of the source error 256-262 F7.3 mJy Bkg2 ?=-1 B3 band (3mm) background -------------------------------------------------------------------------------- Byte-by-byte Description of file: *g[ns].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Proto-cluster name 13- 15 I3 --- Seq Source running number 17- 18 I2 --- S1 Number of the smallest scale where source first appears 20- 21 I2 --- S2 Number of the largest scale where source still exists 23- 24 I2 --- SX Number of the footprinting scale for current source 28- 33 F6.1 pix Xcop X-coordinate relative to the lower-left pixel (1,1) 36- 41 F6.1 pix Ycop Y-coordinate relative to the lower-left pixel (1,1) 44- 54 F11.7 deg RAdeg WCS (J2000) right ascension of current source 57- 67 F11.7 deg DEdeg WCS (J2000) declination of current source 70 I1 --- FG Flag describing global properties over all wavelengths (1) 73- 81 E9.4 --- Signi Global detection significance over all wavelengths, Signi=sqrt(sum(SigniM2)) 84- 92 E9.4 --- Good Global goodness combining significance and S/N, Good = sqrt(sum(GoodM2)) 97- 98 I2 --- FM01 1.001mm Flag describing monochromatic properties (2) 101-109 E9.4 --- SigniM01 1.001mm Detection significance from monochromatic single scales, SigniM=SSPeak/SSTdev single-scale analog of S/N ratio (3) 112-120 E9.4 --- GoodM01 1.001mm Monochromatic goodness combining significance and S/N (4) 122-131 E10.4 Jy/beam Speak01 1.001mm Peak intensity (5) 134-142 E9.4 Jy/beam e_Speak01 1.001mm Peak intensity error (5) 144-153 E10.4 Jy Ftot01 1.001mm Total flux 156-164 E9.4 Jy e_Ftot01 1.001mm Total flux error 166-175 E10.4 Jy Falt01 1.001mm Total flux (Gaussian) or MASS 178-186 E9.4 arcsec Scale01 1.001mm Characteristic size (FWHM) or ALPHABE 189-197 E9.4 arcsec AFWHM01 1.001mm Major size at half-maximum (FWHM) interpolated from intensities at half-maximum 200-208 E9.4 arcsec BFWHM01 1.001mm Minor size at half-maximum (FWHM) interpolated from intensities at half-maximum 211-219 E9.4 arcsec AsizeE01 1.001mm Major size from intensity moments below half-maximum for non-Gaussian sources 222-230 E9.4 arcsec Bsize01 1.001mm Minor size from intensity moments below half-maximum for non-Gaussian sources 233-241 E9.4 deg theta01 1.001mm Angle of the major axis (east of vertical) position angle (east of north) 243-252 E10.4 --- FOFA01 1.001mm Footprint expansion scaling factor 255-263 E9.4 arcsec FOOA01 1.001mm Full major axis of an elliptical footprint 266-274 E9.4 arcsec FOOB01 1.001mm Full minor axis of an elliptical footprint 279-280 I2 --- FM02 1.002mm Flag describing monochromatic properties (2) 283-291 E9.4 --- SigniM02 1.002mm Detection significance from monochromatic single scales, SigniM=SSPeak/SSTdev single-scale analog of S/N ratio (3) 294-302 E9.4 --- GoodM02 1.002mm Monochromatic goodness combining significance and S/N (4) 304-313 E10.4 Jy/beam Speak02 1.002mm Peak intensity (5) 316-324 E9.4 Jy/beam e_Speak02 1.002mm Peak intensity error (5) 326-335 E10.4 Jy Ftot02 1.002mm Total flux 338-346 E9.4 Jy e_Ftot02 1.002mm Total flux error 348-357 E10.4 Jy Falt02 1.002mm Total flux (Gaussian) or MASS 360-368 E9.4 arcsec Scale02 1.002mm Characteristic size (FWHM) or ALPHABE 371-379 E9.4 arcsec AFWHM02 1.002mm Major size at half-maximum (FWHM) interpolated from intensities at half-maximum 382-390 E9.4 arcsec BFWHM02 1.002mm Minor size at half-maximum (FWHM) interpolated from intensities at half-maximum 393-401 E9.4 arcsec AsizeE02 1.002mm Major size from intensity moments below half-maximum for non-Gaussian sources 404-412 E9.4 arcsec Bsize02 1.002mm Minor size from intensity moments below half-maximum for non-Gaussian sources 415-423 E9.4 deg theta02 1.002mm Angle of the major axis (east of vertical) position angle (east of north) 425-434 E10.4 --- FOFA02 1.002mm Footprint expansion scaling factor 437-445 E9.4 arcsec FOOA02 1.002mm Full major axis of an elliptical footprint 448-456 E9.4 arcsec FOOB02 1.002mm Full minor axis of an elliptical footprint 461-462 I2 --- FM03 3.002mm Flag describing monochromatic properties (2) 465-473 E9.4 --- SigniM03 3.002mm Detection significance from monochromatic single scales, SigniM=SSPeak/SSTdev single-scale analog of S/N ratio (3) 476-484 E9.4 --- GoodM03 3.002mm Monochromatic goodness combining significance and S/N (4) 486-495 E10.4 Jy/beam Speak03 3.002mm Peak intensity (5) 498-506 E9.4 Jy/beam e_Speak03 3.002mm Peak intensity error (5) 508-517 E10.4 Jy Ftot03 3.002mm Total flux 520-528 E9.4 Jy e_Ftot03 3.002mm Total flux error 530-539 E10.4 Jy Falt03 3.002mm Total flux (Gaussian) or MASS 542-550 E9.4 arcsec Scale03 3.002mm Characteristic size (FWHM) or ALPHABE 553-561 E9.4 arcsec AFWHM03 3.002mm Major size at half-maximum (FWHM) interpolated from intensities at half-maximum 564-572 E9.4 arcsec BFWHM03 3.002mm Minor size at half-maximum (FWHM) interpolated from intensities at half-maximum 575-583 E9.4 arcsec AsizeE03 3.002mm Major size from intensity moments below half-maximum for non-Gaussian sources 586-594 E9.4 arcsec Bsize03 3.002mm Minor size from intensity moments below half-maximum for non-Gaussian sources 597-605 E9.4 deg theta03 3.002mm Angle of the major axis (east of vertical) position angle (east of north) 607-616 E10.4 --- FOFA03 3.002mm Footprint expansion scaling factor 619-627 E9.4 arcsec FOOA03 3.002mm Full major axis of an elliptical footprint 630-638 E9.4 arcsec FOOB03 3.002mm Full minor axis of an elliptical footprint -------------------------------------------------------------------------------- Note (1): Flag FG as follows: 0 = source is isolated: not blended with any other source in any waveband 1 = source is blended: footprints intersect by more than 20% in at least one waveband 2 = source is sub-structured: its footprint area contains at least one other source 3 = source is sub-structuring: causing a larger source to be sub-structured Note (2): Flag FM as follows: 0 = source has no problems identified in waveband 1 = source sizes are suspicious: sqrt(AFWHM*BFWHM)/BEAM<0.95 or AFWHM/AsizeE>1.4 or BFWHM/Bsize>1.4 2 = source is larger than the desired maximum size: sqrt(FOOA*FOOB)/FOFA > SRCMAXSIZE = 2.0 2.0 1.5 arcsec 4 = source is too much elongated: AFWHM/BFWHM>2 or AFWHM/FOOA is too close to 1 10 = source peak intensity is not measurable: Speak/FXP_ERR<2 20 = source total flux is not measurable: Ftot/FXT_ERR<2 40 = source peak intensity Speak<0 or Speak and total flux Ftot have opposite signs 100 = source is sub-structured: its footprint area contains at least one mesurable source Note (3): SigniM has a special value of 9.999E-31 if a source is not visible in clean single scales, 7.777E-31 if a source has deconvolved peak intensity equal zero Note (4): GoodM=(SigniM/SigniMmin)*sqrt(SNRP/SNRPmin*SNRT/SNRT_min)*(BFWHM/AFWHM) Note (5): Peak intensity conversion: G008 : conversion from MJy/sr: 1.1742E-05 1.1742E-05 7.0911E-06 G008 : conversion from MJy/sr: 1.6790E-05 1.6790E-05 1.6790E-05 G010 : conversion from MJy/sr: 5.7092E-06 5.7092E-06 3.4900E-06 G010 : conversion from MJy/sr: 7.9106E-06 7.9106E-06 7.9106E-06 G012 : conversion from MJy/sr: 2.0437E-05 2.0437E-05 4.7323E-05 G012 : conversion from MJy/sr: 3.3707E-05 3.3707E-05 4.7323E-05 G327 : conversion from MJy/sr: 1.1601E-05 1.1601E-05 4.2187E-06 G327 : conversion from MJy/sr: 3.1064E-05 3.1064E-05 3.1064E-05 G328 : conversion from MJy/sr: 7.8237E-06 7.8237E-06 6.9271E-06 G328 : conversion from MJy/sr: 3.1064E-05 3.1064E-05 3.1064E-05 G333 : conversion from MJy/sr: 8.2035E-06 8.2035E-06 5.5379E-06 G333 : conversion from MJy/sr: 1.1011E-05 1.1011E-05 1.1011E-05 G337 : conversion from MJy/sr: 7.8526E-06 7.8526E-06 3.6855E-06 G337 : conversion from MJy/sr: 2.6633E-05 2.6633E-05 2.6633E-05 G338 : conversion from MJy/sr: 7.6800E-06 7.6800E-06 4.7428E-06 G338 : conversion from MJy/sr: 1.2753E-05 1.2753E-05 1.2753E-05 G351 : conversion from MJy/sr: 1.5832E-05 1.5832E-05 5.2648E-05 G351 : conversion from MJy/sr: 4.8538E-05 4.8538E-05 5.2648E-05 G353 : conversion from MJy/sr: 1.6579E-05 1.6579E-05 3.9381E-05 G353 : conversion from MJy/sr: 4.8538E-05 4.8538E-05 4.8538E-05 W43-MM1 : conversion from MJy/sr: 4.9015E-06 4.9015E-06 4.3684E-06 W43-MM1 : conversion from MJy/sr: 6.4206E-06 6.4206E-06 6.4206E-06 W43-MM2 : conversion from MJy/sr: 5.7834E-06 5.7834E-06 1.9704E-06 W43-MM2 : conversion from MJy/sr: 6.4206E-06 6.4206E-06 6.4206E-06 W43-MM3 : conversion from MJy/sr: 6.2905E-06 6.2905E-06 3.2625E-06 W43-MM3 : conversion from MJy/sr: 6.4206E-06 6.4206E-06 6.4206E-06 W51-E : conversion from MJy/sr: 2.4613E-06 2.4613E-06 2.0141E-06 W51-E : conversion from MJy/sr: 6.6582E-06 6.6582E-06 6.6582E-06 W51-IRS2 : conversion from MJy/sr: 6.0343E-06 6.0343E-06 2.0731E-06 W51-IRS2 : conversion from MJy/sr: 6.6582E-06 6.6582E-06 6.6582E-06 -------------------------------------------------------------------------------- Acknowledgements: Fabien Louvet, fabien.louvet(at)univ-grenoble-alpes.fr
(End) Patricia Vannier [CDS] 23-Aug-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