AGC DOCUMENTATION FILE: 06Apr23 THIS IS A PRIVATE VERSION. YOU SHOULD NOT BE USING IT UNLESS MARTHA OR RICCARDO SPECIFICALLY INSTRUCTED YOU TO USE THIS ONE. UNDER ABSOLUTELY NO CIRCUMSTANCES SHOULD YOU COPY THIS VERSION!!! The AGC files: The AGC files contain all of the information from D. Burstein's version of the UGC plus all galaxies with known redshift from the privately circulated catalogs of J. Huchra, L. daCosta and Giovanelli-Haynes. The file also contains HI data from the Fisher and Tully catalog (published) and other selected sources. The status of coverage is as follows: (For details, see AGCUPDATES.DOC) ********************************************************************** **** Many of the data contained herein are not published. ***** **** Many parameters are proprietary and should not be cited ***** **** or used without permission. ***** **** Please note that this file is not for public distribution ***** **** without the expressed consent of R. Giovanelli or M. Haynes ***** ********************************************************************** I. AGC.NORTH - Northern celestial hemisphere: Dec. >= 0. - all UGC galaxies included - other galaxies with redshifts from Huchra (Mar89 version) - all CGCG galaxies in PP region - all CGCG galaxies in +12d strip - selected other CGCG fields - cluster galaxies from Dressler for most clusters - HI from all of our sources, plus FT plus others (see list below) - HI from Richter and Huchtmeier II. AGC.SOUTH - Southern celestial hemisphere: Dec < 0. - all UGC galaxies - any galaxy with known redshift from Cfa (Mar89 version) - additional galaxies with redshifts from LN da Costa and Dressler's G.A. Survey and Pellegrini list. - MCG galaxies from Schuster-Haynes list (18-4 hours) - all MCG galaxies larger than 1.3 - Galaxies from Corwin's ESGC - Galaxies in ESO catalog - HI from FT and 300' and 140', Effelsberg and Nancay surveys: May88(140),Aug88(300),Feb89(140),Jul89(140),Oct89(E),Mar90(N), Sep90(N). - HI from Richter-Huchtmeier compilation --------------------------------------------------------------------------------- ------- LOCATION: Master versions of all files are found in ------------------ ------- the directory: /home/esperanza3/galaxy/cats ------------------ --------------------------------------------------------------------------------- There are several other ancillary files that work with the AGC files to include additional information (these are not yet released). AGC.NUMBERS contains records of last AGCNUMBER assigned per hour of RA for north and south separately (see below - BUT DO NOT ALTER THIS FILE WITHOUT CONSULTING MH!) ***** AGC CONTENTS AND FORMAT FOR agc.north AND agc.south *********** Variable name Format Data Content AGCNUMBER I6 AGC entry number. See note 1. 1-12943: UGC galaxy (corresponds to UGC number) 20001-33656: ESO sequence number 100000 - 399999 northern hemisphere 400000 - 799999 southern hemisphere WHICH A1 Identifier for multiple systems: a,b etc. RAH I2 R.A. hours RAM I2 R.A. minutes RAS10 I3 R.A. seconds *10. SIGN A1 Dec. sign DECD I2 Dec. degrees DECM I2 Dec. minutes DECS I2 Dec. seconds A100 I5 Blue major diameter *100. See note 15. B100 I4 Blue minor diameter *100. MAG10 I4 Zwicky magnitude *10. or RC3 ApparentBmag for decl<-3. See note 15 INCCODE I2 Nilson's inclination code POSANG I3 Nilson's position angle (or other measure on same system) DESCRIPTION A8 Morphological description BSTEINTYPE I3 Burstein type code (see gallib/sgal/typeesgc.f) VOPT I6 Radial velocity (helio) VERR I3 Error in radial velocity EXTRC3 I5 Galactic extinction *1000 either directly from RC3 or derived from nearest RC3 galaxy, following Burstein&Heiles (1978) & RC3. See note 17. EXTDIRBE I5 Galactic extinction ext*1000 from the DIRBE dust maps following Schlegel et al. 1998 Value is: E(B-V) in mags (*1000). See note 17. VSOURCE I3 Source for radial velocity measurement (follows Huchra for < 50; > 50 = H-G, probably out of date; -99 stands for NED; other negatives: see note (7).) NGCIC A8 NGC or IC number from Dressel and Condon or Fisher and Tully or other name from ZCAT or MGC name abbreviated (SEZ strip) as MsLNNMMM where M denotes MCG s is sign of strip L indicates 6 deg strip (as in MCG) NN is which field along strip MMM is galaxy entry number in field. The MCG would have listed sLLNNMMM. FLUX100 I5 Observed (uncorrected) 21 cm line flux (in Jy-km/s) * 100. RMS100 I4 Rms noise in mJy *100. V21 I5 21 cm heliocentric velocity. WIDTH I4 21 cm profile width. WIDTHERR I2 Error in 21 cm width. WIDTHCODE A4 Code for type of width measurement. See note (2). TELCODE A1 Telescope code. See note (3). DETCODE I1 Detection code. See note (4). HISOURCE I2 Code for source of 21 cm data. See note (5). STATUSCODE I1 Code for status of data. See note (6). SNRATIO I3 Signal-to-noise ratio*10 for 21 cm feature IBANDQUAL I1 Quality of I-band data. See note (8) IBANDSRC I2 Code for source of I-band data. See note (9). IRASFLAG I1 FLAG for inclusion in internal IRAS database See note (10). ICLUSTER I2 Cluster membership. See note (11). HIDATA I1 FLAG for inclusion in HI database (not yet implemented). See note (12). IPOSITION I1 A flag to indicate the source of the coordinates used in the AGC. See note (13). IPALOMAR I1 A flag to indicate that long slit spectroscopy has been obtained at Palomar. See note (14). RC3FLAG I1 A flag to indicate that the galaxy is included in the RC3. See note (15). IROTCAT I1 Included in rotcurve.cat rotation curve database See note (16) NEWSTUFF I2 UNUSED AGC records are now 125 characters in length: CHARACTER DESCRIPTION*8,NGCIC*8,WHICH*1,TELCODE*1,WIDTHCODE*4, * SIGN*1 INTEGER AGCNUMBER,RAH,RAM,RAS10,DECD,DECM,DECS, * A100,B100,MAG10,INCCODE,POSANG,BSTEINTYPE, * VOPT,VERR,EXTRC3,EXTDIRBE,VSOURCE, * FLUX100,RMS100,V21,WIDTH,WIDTHERR, * DETCODE,HISOURCE,STATUSCODE,SNRATIO, * IBANDQUAL,IBANDSRC,IRASFLAG,ICLUSTER,HIDATA, * IPOSITION,IPALOMAR,RC3FLAG,IROTCAT,NEWSTUFF READ(10,125) AGCNUMBER,WHICH,RAH,RAM,RAS10,SIGN,DECD,DECM,DECS, * A100,B100,MAG10,INCCODE,POSANG,DESCRIPTION,BSTEINTYPE, * VOPT,VERR,EXTRC3,EXTDIRBE,VSOURCE,NGCIC, * FLUX100,RMS100,V21,WIDTH,WIDTHERR,WIDTHCODE,TELCODE, * DETCODE,HISOURCE,STATUSCODE,SNRATIO, * IBANDQUAL,IBANDSRC,IRASFLAG,ICLUSTER,HIDATA, * IPOSITION,IPALOMAR,RC3FLAG,IROTCAT,NEWSTUFF 125 FORMAT(I6,A1,2I2.2,I3.3,A1,3I2.2,I5,2I4,I2,I3,A8,I3,I6,I3, * 2I5,I3,A8,I5,I4,I5,I4,I2,A4,A1,i1,I2,I1,I3,I1,I2,I1, * I2,5I1,I2) Note 1 The UGC is the Uppsala General Catalog (Nilson, 1973); a copy is available in the reading room. Further information on the entries can be obtained from reading Nilson's introduction to his catalog. The ESO catalog is a version based on Vince Ford's catalog and the entry number is simply a sequence number within that catalog (note it is meant to be used only as a pointer privately).. The ESGC catalog has been privately communicated by Harold Corwin. A permanent AGC is assigned when an object is added to the catalog. Sequencing is not retained if a position is updated, but assignment of numbers is made per hour of right ascension: 100001-109999 0-1h north 400001-409999 0-1h south 110001-119999 1-2h north 410001-419999 1-2h south etc. until 330001-339999 23-24h north 630001-639999 23-24h south The last number assigned per hour per catalog is listed in AGC.NUMBERS. Assignment of new numbers is done regularly using the program assign.f. Additional entries to the AGC should be entered first with sequence number "0". Assignment of new numbers should only be performed in consultation with MH. Note 2 Widths measured as follows: Code Measurement ' M50' 50% of the mean flux density ' P20' 20% of the peak flux density ' P50' 50% of peak flux density '5M2P' average of (50% of mean) and (20% of peak) widths '2P50' 50% of each of the two peaks (if double-horned) ' F50' 50% level of fit to slope on either side (using 1991 msr algorithm .825 .5 .5 .2 .5) ' A50' Similar to above, but using IDL_ALFALFA code Note 3 Telescope code: 0 - Arecibo circular feed - no corrections applied 1 - NRAO 91 m. - no corrections 2 - Bonn 100 m. - no corrections 3 - NRAO 42 m. - no corrections 4 - Arecibo flat feed. - no corrections 5 - Nancay. - corrected flux 6 - Parkes. - observed flux 7 - Hybrid - corrected flux 8 - Optical, or else unspecified radio dish (see Note 5, HI Source = 69) 9 - No observations made A - Arecibo non-detection WITHOUT known optical redshift B - Arecibo flat feed, corrected flux (normally mapping) C - Nancay, uncorrected flux (we should change this) D - VLA E - WSRT F - Australia Compact Array G - Arecibo Gregorian, 3.5arcmin beam, uncorrected. H - HIPASS/Parkes multibeam I - HIJASS/Jodrell multibeam J - AO/ALFA K - GBT L - ATCA M - GMRT Note 4 HI detection code: 0 - not detected/not observed 1 - detected. This is equivalent to CODE=1 in the ALFALFA scheme. 2 - marginally detected; everything uncertain. This is equivalent to CODE=3 in the ALFALFA scheme 3 - detection, but inadequate for FT purposes. This may mean width cannot be measured because of baseline or noise on edge, or the profile is very asymmetric or weird, or confusion is suspected. In this case, the flux and velocity are usually measured ok, but one is not certain what they all refer to. 4 - HI profile shows absorption. Flux certainly affected. 5 - Confused with obvious optical companion (i.e. confusion is certain). 6 - This means the width has been BOXCAR+HANNING not just simple Hanning. NOTE THIS IS AN UPDATE TO PREVIOUS DOCUMENTATION! 7 - Used for ALFALFA detections to indicate an object which is detected at low SN but with apriori redshift. This is equivalent to CODE=2 in the ALFALFA scheme. 8 - Profile obtained by some of us, but no parameters entered. 9 - preliminary measurement, not reprocessed through GALPAC Note 5 Source for 21 cm data: -3 - Misc from NED -2 - Entry from RC3 -1 - Entry from Richter catalog of March 1989. You must go look this reference up in the catalog and then in the original publication to be sure the number is right. 2 - Fisher and Tully 1981 Ap. J. Suppl. 47, 139. 10 - Hoffman et al. 1986, preprint Hoffman et al. 1994 (great wall preprint) etc. 11 - Bothun et al. 1985, A.J., 90, 2487 (redshifts only) 12 - Thuan et al. 1987, Ap.J.(Lett.) 315, L93 (redshifts only),Thuan and Seitzer, Thuan and Schneider 13 - Huchtmeier, various publications from old days 14 - Hoffman, Lewis, Helou & Salpeter 1987 (priv.comm.) (selected Sa's & Sc's only) Misc Hoffman et al. publications (mainly Virgo) 15 - Giovanardi 1987 (priv.comm.): selected Sa's & Sc's 16 - Lewis, Helou and Salpeter 1986, Ap.J.Suppl., 59, 161 17 - Salzer, Gavazzi and Murray 1989, preprint. 18 - Eder et al. 1989 Ap.J. 340, 29. (Dwarfs in PP) Eder, Schomber LSB's 2000 ApJSupp 19 - Schneider et al. 1990 Ap.J.Suppl. 72, 245. Note fluxes here are corrected for pointing because of poor coordinates. Schneider et al. 1991 Ap.J.Suppl. 20 - Balkowski et al. ZOA reference 21 - Chamaraux, south strip survey, private comm. 22 - Misc pub by Gavazzi Gavazzi 1989 ApJ 346, 59. Scodeggio and Gavazzi 1993 ApJ 409 110 Gavazzi et al 2000 Astro-ph Also GOLDMINE compilation 23 - Eder, Giovanelli and Haynes 1990 (High L S0's) 24 - B.Williams and Lynch, 1991, AJ 101, 1969 25 - Fouque et al. HI Survey of SGC sample (1990, AASup 86,473) Bottinelli et al. 1992 AASup 93, 173. 26 - Misc pubs by Lu et al. Hoffman, Lu and Salpeter 1991 (Gas Rich dwarfs outside LScl) Lu Ph.D. thesis 27 - Misc pubs by Bothun et al. Bothun et al. (Coma bubble) 1992 preprint Bothun et al. GA region ApJ 388 253 28 - Entry in RC3 29 - HI data from Mathewson et al. (1992) ApJS 81, 413. (Sheriff's data) 30 - MSR private comm early types 31 - Misc pub by Mould et al. Mould et al northern clusters ApJ 409 14 32 - Freudling A+AS 33 - Pantoja et al 1994 AJ108 Pantoja et al 1997 AJ113 34 - Gallagher, Mathews, etc southern dwarfs Mathews and Gallagher 1996, AJ 111, 1098 35 - Dickey, J.D. 1996 AJ (Hercules) 36 - Theureau et al. 1998 A&AS 130, 333. diNella et al. 1996 A&AS 118, 311 37 - WHISP database or publications: Kamphuis et al, 1996, A&AS 116, 15. Also WSRT Braun et al. 38 - Rosenberg & Schneider 2000 ApJS 130, 177 (ADBS) Note that parms can either be from ADBS or VLA obs. Also AHISS Zwaan et al 1997 Note that the fluxes for AHISS are unclear as they give MH and don't say how they calculated distances, Hnot etc. 39 - HIPASS (Parkes multibeam) HICAT Meyer et al. 2004 BGC Koribalski et al 2004 HIZOA Donley et al 2005 40 - Huchtmeier/Karachentsev dwarfs Huchtmeier et al. 2000 A&AS 141, 469 Huchtmeier et al. 2000, A&AS 147, 187. Huchtmeier et al. 2005, A&A 434, 887 41 Misc LSB pubs by KO & friends Monnier Ragaigne et al. 2003 A&A 408, 67 Conselice et al 2003 ApJ 591 42 HIJASS (Jodrell multibeam) 43 various GBT Garland et al. 2004 44 Slaz et al. KISS 45 Other ALFA: AGES, ZOA etc 50 - Haynes and Giovanelli 1984, A.J., 89, 758 51 - Giovanelli and Haynes 1983, A.J., 88, 881 Haynes and Giovanelli 1986, Ap.J. (to appear) VIRGO 52 - Haynes and Giovanelli 1986, A.J. (Pisces-Perseus) + data added in November 1986 53 - Giovanelli and Haynes 1985, Ap.J., 292, 404 (A1367/Coma, A2147/2151) 54 - Bicay and Giovanelli 1986, A.J. 91, 705-750 1987, A.J. 93, 1326 (Cancer region) 55 - Chincarini et al. 1979, A.J., 84, 1500 (N5416 group) Giovanelli and Haynes unpublished data in N5846 region 56 - Giovanelli and Haynes Green Bank 300-foot data (both high and low declinations) Haynes et al. 1988, A.J. 95, 607. - PP north + unpublished 10-22 hours. 57 - Freudling, Haynes, Giovanelli A.J. Dec. 1988 Hercules Supercluster 58 - Haynes 1981, A.J., 86, 1126 (HI streams) Giovanelli and Haynes unpublished maps of large angular diameter galaxies 59 - Magri and Haynes unpublished RSA Sa's and Sc's 60 - Haynes ZoA and IRAS extension (not included yet) 61 - Giovanelli and Helou IRAS galaxies (not included yet) 62 - Freudling, Haynes, Giovanelli Hercules Supercluster 63 - Cast of thousands Sc project. (This will be final code)! 64 - Cast of thousands Abell clusters project. 65 - Marcio's +12d slice 66 - Karachentsev thin galaxies. See also Kara Astro-ph/0107058 for compilation (may also include a few done by ORCs rather than HI) May also include Mathews et al flatgals in Kara compilation 67 - BCD/LSB/high M(HI)/L objects by vanZee, Haynes and Giovanelli. Next ones to be recoded as Mathewson: 67 - Preliminary results from Parkes/SS0 surveys. Some objects may be optical V(rot) not HI (can't tell from DSM's bookkeeping...) 68 - Preliminary results from 1988 GB surveys. Note that parameters may be changed later. (Both 140 and 300') 69 - Unspecified (i.e. an HI redshift is listed, and the rest of the HI parameters will be entered when we get around to it....) 70 - H293 71 - H304 72 - AO band Apr-May 2001 (BC) Sep 2001 (CS & BC: PPS) Nov 2001 (CS & BC: PPS) 73 - our VLA stuff 74 - Higher redshift AO observations March,October 2003 (BC & JG: SDSS) 75 - ALFA a1946 or a2010(!) 76 - Misc AO Gregorian, including A2010 followup a1904 Jan 2005 (Leo Group) Note 6 21 cm data status: 0 - No data. 1 - Published. 2 - Unpublished but available. 4 - Observed by source in reference but not available to public. 5 - Obtained from on-line compilation, such as GOLDMINE etc, may not be original source. Note 7 Extra codes used for velocity where not in ZCAT -11 - From McGraw-Hill observations - PP only for now -12 - MDM Sc observations; maybe very rough; or Palomar rot curve. -13 - Pierre, private comm. -14 - (Need to check) -15 - From lists sent by Pellegrini -16 - From RC3 -17 - Palomar redshifts, RG, GW, SS -18 - Palomar redshifts: Scodeggio, RG -20 - Willick et al. (1990) ApJ 355, 393. -21 - Moss and Dickens 1988, MN 232, 381. -22 - Lucey et al. 1991, MNRAS 248, 804. -23 - Cappi et al. 1991, AASupp 88, 349. -24 - Beers et al. 1991, AJ 102, 1581. -25 - Capelato et al. 1991, AASupp 90, 355. -26 - from Markarian listing. -27 - from Mathewson et al. 1992, ApJS 81, 413. or MFB96 (ORCs) -28 - RC3 -29 - Courteau thesis -30 - Pinkney et al. 1993, ApJ (A2634) -31 - Bottinelli et al 1992 AASup 93, 173. - Quintana,Fouque and Way 1994 A&A 283, 722 -32 - Tarenghi et al 1994 AJ 107, 1659. (Hercules) -33 - Palomar rotation curves Vogt or DD -34 - Thorstensen et al. CFA slice fainter 1995 preprint -35 - Marco's work -36 - SSRS2 -37 - Updated ZCAT '99 Falco et al. misc -38 - PSC-zed -39 - Gavazzi et al 2000 Astroph -40 - 2DF data release 7/01 -98 - SDSS SQL -99 - NED Note 8 IBANDQUAL - I1 - quality/status flag: 0 - Not observed 1 - Observed with photometric high quality (zpc*error < 0.05 mag) 2 - Observed; zpc error 0.05-0.10 mag 3 - Observed; zpc error 0.10-0.20 mag 4 - Observed; zpc error > 0.20 mag 6 - Fit performed on extant image is poor; image itself prob ok. Usually means that fit cannot be done well because of bar, face-on, asymm, etc. Correponds mostly to Q_EFIT=4. 7 - Unacceptable for imaging because of superimposed star, wrong morphology, etc. 8 - Observed; status unknown (data not yet reduced or unknown from other source) 9 - Must be reobserved for reasons other than poor photometry. Examples are: 1) Object too close to edge of frame 2) Image is trailed significantly 3) Background level is too high (moon) 4) Bad column of CCD passes through galaxy. *zpc = nightly photometric zero-point constant Note 9: Source for I-band ccd data 01 - Pierce and Tully, 1988Ap.J. 330, 579 02 - Bothun and Mould 03 - Willick (Pisces-Perseus) 04 - Courteau 05 - Mathewson et al. 06 - Han 1992 ApJS 81, 35 07 - Bernstein et al. (us!) Coma paper 50 - Sc primary sample (edge-ons only!) 51 - Pisces-Perseus sample 52 - Hercules data 53 - Within field of Sc2 images (This changed 11/30/00) 54 - Various multicolor (not I) from KPNO/CTIO e.g. Rband face/edge, BVR/Halpha Sa's etc. 60 - included on Sc2 skyfit tapes (jan98.agc) 61 - Jeremy 62 - Archive of multicolor (not I) from KPNO/CTIO e.g. Rband face/edge, BVR/Halpha Sa's etc. 90 - in final SFI table = opt980107 (agc980107) 91 - in final MFB reprocessed table = mfbagc97 (not id'd if also in SFI table) 92 - in final DD table (that's Danny "Arlo" Dale) 93 - in final MS table (that's Marco Scodeggio) 94 - in SF2 photometric sample (NB not final: beware!) Note 10: Flag indicating membership in database of IRAS data contained in /haynes/iras/coadds. This indicator is in the process of being implemented but will include all UGC entries from PSC as well as coadded scans for S0, Sa and Sc galaxies and Pisces-Perseus region. Note 11: Cluster membership. BEWARE: Code assignments may not be up to date! If you wish to use this for scientific purposes, discuss with MPH. The code refers to the cluster according to the following: 1 - 76 003712.0 063022 .0416 4 ad 001111 2 - 119 005351.0 -013203 .0440 21 778 ad 001001 3 - 151 010623.9 -154129 .0526 2 ad 000000 4 - 154 010821.0 172426 .0658 11 862 ad 000010 5 - 168 011233.7 -000144 .0452 13 581 ad 001111 6 - 189 012104.7 012353 .0335 3 000101 7 - 194 012302.3 -014612 .0178 60 435 1 ad 111001 8 - 260 014858.3 325523 .0348 2 000101 9 - 262 014957.0 355420 .0161 38 415 1 100101 10 - 347 022244.1 413901 .0187 19 586 1 100001 11 - 376 024240.1 363920 .0489 1 ad 001110 12 - 397 025409.0 154515 .0325 6 000101 13 - 400 025500.5 055010 .0232 21 423 1 ad 111111 14 - 426 031520.4 412013 .0183 108 1308 1 100001 15 - 484 041354.2 -074732 .0386 4 000001 16 - 496 043117.8 -132144 .0320 32 657 ad 011001 17 - 539 051353.7 062441 .0205 3 1 ad 111111 18 - 548 054503.0 -253840 .041 9 ad 001000 19 - 569 070523.6 484233 .0196 12 444 1 100001 20 - 576 071720.0 555000 .0381 47 914 000001 21 - 592 073953.5 092956 .0624 2 ad 000010 22 - 634 081029.2 581221 .0267 35 309 1 100001 23 - 754 090625.5 -092650 .0528 35 1048 ad 000000 24 - 779 091649.0 335914 .0226 13 755 1 100101 25 - 838 093433.8 -044722 .0507 1 ad 000000 26 - 957 101121.4 -004005 .044 1 ad 001110 27 - 978 101758.0 -061630 .0527 2 ad 000000 28 - 979 101756.6 -073830 .055 2 ad 000000 29 - 999 102040.8 130621 .0318 2 000101 30 - 1016 102426.7 111407 .0321 2 000101 31 - 1060 103427.7 -271626 .0114 78 676 000001 32 - 1069 103721.3 -082135 .063 2 ad 000000 33 - 1139 105529.2 014636 .0383 2 ad 011111 34 - 1142 105816.8 104930 .0353 35 417 ad 011111 35 - 1177 110646.4 215812 .0316 2 000101 36 - 1185 110808.6 285709 .0304 5 785 1 ad 111111 37 - 1213 111349.2 293258 .0468 12 598 1 100100 38 - 1228 111850.7 343650 .0350 6 306 1 100101 39 - 1257 112325.5 353643 .0339 1 100101 40 - 1267 112520.5 270841 .0321 2 100101 41 - 1314 113205.7 491932 .0341 16 701 1 100001 42 - 1367 114156.1 200723 .0215 75 832 1 100101 43 - 1377 114419.0 560122 .0514 13 488 ad 000000 44 - 1631 125010.9 -131003 .0508 4 ad 000000 45 - 1644 125436.5 -170555 .0449 3 ad 001000 46 - 1656 125723.5 281510 .0232 226 880 1 ad 111111 47 - 1736 132408.0 -265145 .035 2 ad 011001 48 - 1836 135858.0 -112244 .0363 1 000001 49 - 1837 135903.5 -105544 .0376 1 000001 50 - 1913 142429.1 165411 .0533 1 ad 000010 51 - 1983 145025.6 165726 .0441 8 433 ad 001110 52 - 1991 145210.3 185036 .0586 2 ad 000010 53 - 2040 151015.1 073721 .0456 1 ad 001110 54 - 2052 151415.7 071145 .0348 37 576 000101 55 - 2063 152036.6 084925 .0337 21 521 ad 011111 56 - 2147 160002.1 160252 .0356 30 1148 1 100101 57 - 2151 160258.0 175314 .0371 42 887 1 ad 111111 58 - 2152 160306.8 163515 .0374 22 1244 111111 59 - 2162 161029.6 294010 .0320 4 000101 60 - 2197 162628.4 410112 .0303 46 593 1 100001 61 - 2199 162651.2 393815 .0303 70 807 1 100001 62 - 2247 165157.8 813919 .0392 14 370 000001 63 - 2256 170635.8 784703 .0601 15 1257 ad 000000 64 - 2572 231555.5 182805 .0395 4 000101 65 - 2589 232127.3 163314 .0421 13 602 ad 001110 66 - 2634 233550.6 264532 .0312 17 899 1 ad 111111 67 - 2657 234220.2 085237 .0414 12 667 ad 001110 68 - 2666 234824.0 265241 .0265 15 261 1 111111 69 - 3381 70 - 3407 71 - 3528 72 - 3558 73 - 3656 74 - 3667 75 - 2295 76 - 3744 77 - 2457 78 - 114 79 - 160 80 - 505 81 - 295 82 - 2806 83 - 3193 84 - 3266 85 - 671 86 - 3408 87 - 3581 88 - 3571/2 89 - 3564/6 90 - 3716 91 - 2022 92 - 2593 93 - 2670 94 - 2870 95 - 2877 96 - 4038 97 - 2029 98 - 2218 99 - 1413 -1 -507 012048.0 330000 .02 3500 7000 2 -2 081730.0 211400 .02 3000 7000 3 -3 115400.0 493000 .01 -1000 3000 5 -4 122818.0 124000 .01 -1000 3000 5 -5 140000.0 094900 .01 5000 9000 2 -6 150357.0 114800 .01 -1000 3000 5 Note 12: Flag set to "1" indicates that there is a spectrum of this galaxy in the "final" HI digital archive and derived parameters are included in the HI results archive. Note 13: It is beneficial to know where the coordinates listed in the AGC came from. This 1-digit code will allow us to identify the source and hence the expected accuracy of the position entered into the AGC. We should make use of this code in the future. 1 -- From measurements made using digital pad 2 -- From POSS prints with OVERLAY only (either OSU overlays or our own). 3 -- From DSS by DD 5 -- Found using SKYVIEW 6 -- Published positions UGC objects: Cotton et al. 1999 ApJS 125, 409. 8 -- From SDSS SQL 9 -- NED positions with accuracy quoted to be <2" Note 14: Identifier for existence of data in Palomar long-slit DBS database. 9 means marginal or suspect data. Now updated so that highest number from below is set in AGC: 1 -- From Vogt thesis sample 2 -- From Dale thesis 3 -- From Jore thesis or misc Palomar Sa's 4 -- From Palomar band survey or other associated stuff 5 -- Included in MFB rotcurve database 6 -- TF scaling relations project (>= sep01), JD extinction etc 7 -- High z ORC's, either Palomar or KPNO 8 -- Observed and detected but only 300 seconds or not extended {This code not consistently implemented, but will be someday...} 9 -- ATTEMPT TO GET ORC FOUND NO LINES Note 15: Flag for objects that are listed in the RC3. A cross reference file is maintained in /galaxy/rc3/rc3agc.cross. It should be accurate except in some cases of confusion in multiple systems. In July 00, we updated magnitudes and diameters in the agc.south using RC3 scaling so that (a) for galaxies in the MCG strip with RC3FLAG=1 (-18 ext_I = 0.45*extrc3 DIRBE E(B-V) ==> ext_I = 1.962*extdirbe