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Takahiro Tsutsumi authored faf86256bc7
A minor help doc update as asteroid models has been update in

the data repository
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gcwrap/tasks/setjy.xml

Modified
488 488 Moons: Jupiter: Io, Europa, Ganymede, Callisto
489 489 Saturn: Titan
490 490
491 491 Asteroids: Ceres, Lutetia, Pallas**, Vesta**, Juno**<!-- only in the 2010 , Victoria***,
492 492 Davida*** -->
493 493
494 494 ******************************************************************************************
495 495 * New asteroid models for Ceres, Pallas, and Vesta were put into CASA 4.7. *
496 496 * A model is also available for Lutetia but we do not advise using this source for ALMA *
497 497 * absolute flux calibration. These new models are used (automatically chosen) *
498 - * for data taken after 2015 January 1 0h UT. The models are time variable and based on *
498 + * for data taken after 2014 January 1 0h UT. The models are time variable and based on *
499 499 * thermophysical modeling by Th. Mueller (private communication). *
500 500 * These are tabulated for 30, 80, 115, 150, 200, 230, 260, 300, 330, 360, 425, 650, *
501 501 * 800, 950, and 1000 GHz; cubic frequency interpolation is employed to derive the flux *
502 502 * density at other frequencies. There is no line emission included in these models. *
503 503 * The available model files can be listed with the command, *
504 504 * setjy(standard='Butler-JPL-Horizons 2012', listmodels=T). *
505 505 ******************************************************************************************
506 506
507 507 * Venus: model for ~300MHz to 350GHz, no atmospheric lines (CO,H2O,HDO, etc)
508 508 * Mars: tabulated as a function of time and frequency (30 - 1000GHz) based on
509 509 Rudy et al (1988), no atmospheric lines (CO, H20, H2O2, HDO, etc)
510 510 * Jupiter: model for 30-1020GHz, does not include synchrotron emission
511 511 * Uranus: model for 60-1800GHz, contains no rings or synchrotron.
512 512 * Neptune: model for 2-2000GHz, the broad CO absorption line
513 513 is included, but contains no rings or synchrotron.
514 514 * Titan: model for 53.3-1024.1GHz, include many spectral lines
515 515
516 - ** not recommended when the old model is used (i.e. for the data prior to 2015.01.01)
516 + ** not recommended when the old model is used (i.e. for the data prior to 2014.01.01)
517 517 (The temperature is not yet adjusted for
518 518 varying distance from the Sun. The model data can be scaled
519 519 after running setjy, but it is an involved process.)
520 520
521 521 The 'field' parameter must match the case of the field name(s)
522 522 in vis (as shown by listobs).
523 523
524 524 Flux density calculation with Solar System objects depends on
525 525 ephemerides. The setjy task looks for the data in
526 526 <!--setjy looks, in order, in

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