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                      The Extended 12 Micron Galaxy Sample


                      (Rush, Malkan, and Spinoglio (1993))






                Documentation for the Computer-Readable Version


                                   Brian Rush









                         Doc. No. NSSDC/WDC-A-R&S 93-22



                                   July 1993








                  National Space Science Data Center (NSSDC)/
           World Data Center A for Rockets and Satellites (WDC-A-R&S)
                 National Aeronautics and Space Administration
                          Goddard Space Flight Center
                              Greenbelt, MD 20771



                                 Abstract


    The authors have used the IRAS data to compile a sample of 893
    galaxies, including 118 Seyfert galaxies. ADDSCAN/SCANPI inte-
    grated fluxes at 12, 25, 60, and 100 microns from the IRAS survey,
    along with redshifts and 1950 coordinates are given for all
    galaxies.

    1 Introduction

    The 12 Micron Galaxy Sample is an all-sky (b greater than or equal
    to 25 deg.) sample of 893 galaxies selected from the IRAS Faint
    Source Catalog, Version 2. The sample is 12-micron-flux-limited at
    0.22 Jy and is complete down to a 12mu flux of 0.30 Jy. It
    includes 55 Seyfert 1 galaxies (including QSOs and two blazars),
    63 Seyfert 2 galaxies, 38 high-far-IR-luminosity non-Seyferts, and
    29 LINERs. The flux densities presented are whole-galaxy fluxes
    obtained by the ADDSCAN/SCANPI process at IPAC. Observed radial
    velocities, mostly obtained from well-known extragalactic catalogs
    are also given.

    This document is intended to provide the information necessary to
    describe this catalog to a computer and to make it easy to use. A
    copy should accompany any further distribution of this version of
    the machine-readable catalog.


    2 Source Reference

    The Extended 12 Micron Galaxy Sample. Rush, B., Malkan, M., and
    Spinoglio, L. 1993, ApJS, 89, no.1 (in press)


    3 Structure

    3.1 File Structure

    The file given here has 893 lines with 76 bytes of data each. The
    data given are exactly the same as those found in tables 1-5 of
    the source reference (hereafter RMS), with two exceptions: (1) In
    RMS, tables 1-5 represent Seyfert 1s, Seyfert 2s,
    high-far-IR-luminosity non-Seyferts, LINERs, and normal galaxies,
    respectively, whereas all galaxy types here are in the same table,
    sorted by RA; (2) several flags are given, one of which indicates
    the galaxy type and, thus, the table in which it would appear in
    RMS.












                                    1



    3.2 File Format

    Table 1 gives a byte-by-byte description of the contents of the
    data file.

                 Bytes   Unit    Format      Item

                  2- 3    hr       I2      R.A. (1950)
                  4- 5    min      I2      R.A. (1950)
                  6- 9    sec     F4.1     R.A. (1950)
                 10-12    deg      I3      Dec (1950)
                 13-14     '       I2      Dec (1950)
                 15-16     "       I2      Dec (1950)
                 18-24    Jy      F7.2     12 mu flux
                 26-32    Jy      F7.2     25 mu flux
                 34-41    Jy      F8.2     60 mu flux
                 43-51    Jy      F9.2     100 mu flux
                 53-64     ...    A12      Name
                   66      ...     I1      Object type
                   67      ...     A1      Redshift type
                   68      ...     A1      Redshift reference
                 70-76     ...    F7.5     Redshift

                            Table 1: File Format


                            Notes to Table 1

    RA and Dec are 1950, from the IRAS Faint Source Catalog, Version
    2. (A few exceptions are explained in RMS.)

    Flux densities are obtained by the ADDSCAN/SCANPI process at IPAC
    for most objects; the exceptions are explained in RMS.

    Names and redshifts are taken from various extragalactic catalogs.

    Object type is as follows: 0, 1, 2, 3, or 4 for normal, Seyfert 1,
    Seyfert 2, high-far-IR-luminosity, and LINER galaxies,
    respectively. (How these objects are defined/identified is
    explained in RMS.)

    Redshift type is as follows: "S" if corrected for solar motion
    about the galactic center, and for the Galaxy's motion towards
    Virgo; "V" if NOT corrected.

    Redshift reference is listed in RMS, but a different labeling
    scheme is used here, as given below.










                                       2



                           REDSHIFT REFERENCES

     CODE         REFERENCE

      D            NED (NASA/IPAC Extragalactic Database)

      E            Lauberts (1982)

      F            NOT a real redshift: calculated as 75.0 x distance,
                   where the distance is in Mpc, from Rice et al.
                   (1988); for LMC, SMC, and M33 only

      G            Geller & Huchra (1983); group velocity

      H            Hewitt & Burbidge (1991)

      M            Strauss (1991) or Strauss et al. (1990 or 1992)

      N            Norris et al. (1990)

      P            Calculated from spectra taken by the authors at
                   Lick Observatory

      R            de Vaucouleurs, de Vaucouleurs & Corwin (1976; RC2)

      S            Spinoglio & Malkan (1989)

      V            Veron-Cetty & Veron (1991)

      W            Saunders (1991)

      Y            Geller & Huchra (1983); INDIVIDUAL (not group) velocity

      Z            ZCAT (Huchra et al. 1993)


    4 Additional Information

    In addition to tables 1-5, which contain the data described here,
    there are seven more tables of data in RMS. Tables 6-8 therein
    give the calculated 12 mu, Far-IR, and 60 mu luminosity functions,
    respectively. These three tables are short enough that it would be
    easy for those interested in using the actual data to simply type
    them in from RMS. Tables 9-12 list various objects that met the
    search criterion of the sample, but were excluded for various
    reasons (e.g., being galactic objects). These four tables are
    given in tables 2-5 in this document.








                                       3



               R.A.       Dec.               R.A.        Dec.
            002643.4     +093557           154726.5    -20119
            011541.6     -524857           155202.5    +040335
            011626.9     +200934           155427.5    -872526
            011955.4     -444034           161411.4    +031039
            021331.2     +075746           162022.2    -082029
            021417.2     -212052           171841.6    +434825
            025348.6     +195339           175833.9    +663806
            030437.0     +254424           182941.1    -741743
            030615.8     -653830           192641.5    -445751
            032327.8     -131432           192653.9    -455249
            032547.4     -014317           195731.7    -293504
            035201.9     -385742           202050.9    -193523
            041003.2     -652036           204359.6    -315112
            043043.3     -485444           205255.4    -123507
            043736.3     -323856           211052.9    +064409
            044333.7     -221801           212731.7    +115644
            052715.0     -633305           213817.2    -265928
            070246.5     -793424           214529.4    +000801
            084555.1     +140106           221811.6    -862423
            092941.9     +115918           224857.7    -774852
            101943.8     +615154           225916.1    +124859
            132419.4     +460449           231949.6    -023014
            144514.5     +265102



    Table 2: Stellar Objects Excluded by Examination of Plates

                R.A.        Dec.        Date    Note
            003444.5     +071241    12JAN91       1
            025520.7     +201806    12FEB91       1
            031513.6     +213249    12JAN91       1
            035245.4     +072636    12JAN91       1
            041155.9     -125153    12JAN91       1
            043231.9     -141919    19JAN91       2
            044508.0     -053926    12FEB91       1
            050505.0     -061418    12JAN91       3
            093712.0     +121230    12JAN91       1
            093931.7     -083832    12JAN91       1
            123148.3     +825001    19FEB91       1
            132435.4     -123044    12JAN91       1
            142603.7     -131547    12FEB91       1
            145940.0     -273852    19FEB91       1
            155439.3     -063547    12FEB91       1
            160115.9     +132843    12FEB91       1
            162753.6     -034541    12FEB91       1
            164300.9     +424903    12FEB91       1
            174440.5     +395718    12FEB91       1

    Table 3: Stellar Objects Excluded by Examination of Spectra




                                    4
     


                             Notes to Table 3

    (1) Optical spectrum of stars

    (2) Associated with MCG-2-12-42; optical spectrum contaminated by
    a strong late-type star; infrared fluxes contaminated by a nebular
    object 3 arcmin SE of the FSC-2 positionl.

    (3) stellar-like optical spectrum, infrared fluxes dominated by a
    galactic object.


              Name          R.A.         Dec.        z      Note

             N9880        023259.6     -093415     0.0050     1
             M-4-9-52     033951.1     -212357     0.0145     1
             M-1-24-1     090822.7     -084118     0.0061     1
             N3338        103927.2     +140033     0.0040     1
             N3395/6      104705.1     +331512     0.0064     6
                          130650.4     +071536                4
                          144353.5     +064510                5
             M-4-36-9     151609.3     -233821     0.0079     2
             M-4-36-14    152312.3     -220626     0.0077     1
             M+8-32-9     172940.8     +505439     0.0188     3
             IRAS         223738.8     +242626     0.0423     1

                         Table 4: Galaxies Excluded



                            Notes to Table 4

    (1) Excluded when looking at ADDSCANs, finding charts, and IRAS
    colors.

    (2) Excluded by IRAS colors and finding chart; the object itself
    is likely a star.

    (3) Excluded because an optical spectrum (Lick 1m tel.) and
    near-IR photometry (San Pedro Martir Obs., Mexico) showed the
    12 mu flux to be mostly from the very red M star just E of the
    galaxy.

    (4) ZCAT association and SAO association are both within 1 arcmin.
    SAO119793 at center, mostly covering the galaxy.

    (5) ZCAT association and SAO association are both within 1 arcmin.
    The galaxy is closer to the center, but SAO129652 appears large
    and is touching the galaxy just to the right.

    (6) Excluded because, upon viewing the finding chart and ADDSCANs
    two clearly separated galaxies are each contributing less than
    0.20 Jy of the 12 mu flux.



                                    5


        Name        R.A.        Dec     12mu   25mu   60um   100mu   Note

     F00028-2909  000253.9   -290935    0.29   0.36   0.45    0.45     1
     E539-G8      001904.9   -195724    0.36   0.17   1.89    4.09     -
     M-2-3-68     010054.8   -110720    0.25   0.33   1.37    2.76     -
     F01266-7331  012641.0   -733136    0.24   0.06   0.32    2.40     2
     E548-G36     033115.3   -214356    0.24   0.39   1.83    4.35     -
     CGCG313-016  102133.5   +673305    0.22   0.52   0.74    1.02     -
     M+15-1-12    115803.7   +882453    0.18   0.28   2.30    4.82     -
     F12335+6414  123330.4   +641450    0.22   0.14   1.61    5.11     -
     M-1-33-62    125715.2   -082834    0.30   0.26   1.58    6.35     -
     F17020+4544  170202.9   +454458    0.33   0.37   1.16    1.27     -
     F19518-8142  195148.3   -814211    0.42   0.29   1.95    6.63     -
     F20254-8152  202529.6   -815236    0.41   0.53   1.21    1.13     3
     N7665        232439.0   -093947    0.29   0.22   1.62    2.63     -

                        Table 5: Unidentified Objects



                            Notes to Table 5

    (1) Somewhat suspicious [25-12] color for a galaxy. It appears
    slightly extended in the optical plates. It can be either a galaxy
    or a star with some nebulosity.

    (2) Very suspicious IRAS colors for a galaxy. It is located within
    the boundaries of the SMC, but not identified by Schwering and
    Israel (1989).

    (3) IRAS colors consistent with being a galaxy.



    5 References


    de Vaucouleurs, G., de Vaucouleurs, A., and Corwin, H. G., Jr.
    1976, Second Reference Catalog of Bright Galaxies (Austin,
    University of Texas Press)

    Geller, M. J., and Huchra, J. P. 1983, ApJS, 52, 61

    Hewitt, A., and Burbidge, G. 1991, ApJS, 75, 297

    Huchra, J. P., Geller, M. J., Clemens, C., Tokarz, S., and Michel,
    A. 1993, in preparation (ZCAT)


    Lauberts, A. 1982, The ESO/Uppsala Survey of the ESO(B) Atlas
    (Munich, European Southern Observatory)

    Moshir, M., et al. 1991, Explanatory Supplement to the IRAS Faint
    Source Survey, Version 2. (Pasadena, JPL)



                                    6



    Norris, R. P., Allen, D. A., Sramek, R. A., Kesteven, M. J., and
    Troup, E. R. 1990, ApJ, 359, 291

    Rice, W., Lonsdale, C. J., Soifer, B. T., Neugebauer, G., Kopan,
    E. L., Lloyd, L. A., deJong, T., and Habing, H. J. 1988, ApJS, 68, 91

    Saunders, W. 1991, private communication

    Spinoglio, L., and Malkan, M. A. 1989, ApJ, 342, 83

    Strauss, M. A., Davis, M., Yahil, A., and Huchra, J. P. 1990, ApJ,
    361, 49

    Strauss, M. A. 1991, private communication

    Strauss, M. A., Huchra, J. P., Davis, M., Yahil, A., Fisher, K. B.,
    and Tonry, J. 1992, ApJS, 83, 29

    Veron-Cetty, M. P., and Veron, P. 1991, A Catalogue of Quasars and
    Active Nuclei, 5th edition. ESO Scientific Report No. 10 - October
    1991 (Munich, European Southern Observatory)



































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