January 19 2021

- converted entire file to fits format. Descriptions of columns embedded in file. 
- included new columns for systemic proper motions
- error fixed for Leo IV, declination changes from 0 32 0.0 to -0 32 0.0
- added Centaurus 1 (Mau et al. 2020)
- added DESJ0225+0304 (Luque et al. 2017)
- new distance+uncertainties for Pisces 2 and Leo5 (Sand et al. 2012)
- updated parameters plus radial velocity for Draco 2 (Longeard et al. 2018)
- updated distance and metallicity for Cetus 2 (Conn et al. 2018)
- updated parameters for Sag 2 (Longeard et al. 2019)
- updated radial velocity and metallicity for Tri2 (Kirby et al. 2017)
- updated radial velocities and metallicity for Tuc4, TucV, Grus2, plus structural parameters for Tuc4, Tuc5 (Simon et al. 2019)
- updated radial velocities and metallicities for Phoenix (Kacharov et al. 2017); updated structural parameters from Battagloa et al. (2012)

October 25 2019

- Error fixed that had incorrectly substititued the Sersic index in place of the half-light radius, for all those galaxies for which I had adopted values from Munoz et al. 2019

October 11 2019

- Small changes to format of table (now entirely space-delimited). Also removed the Galaxy and Andromeda (M31) from the table
- Changed name of "Indus I" (at declination -46) to Indus 2, consistent with revised discovery paper
- Added Hydra 1 (Grillmair 2011, Hargis et al. 2016)
- Added Pictor 2 (Drlica-Wagner et al. 2016)
- Added Virgo 1 (Homma et al. 2016)
- Added Crater 2 (Torrealba et al. 2016a)
- Added Aquarius 2 (Torrealba et al. 2016b)
- Added Carina 2 (Torrealba et al. 2018)
- Added Carina 3 (Torrealba et al. 2018)
- Added Hydrus 1 (Koposov et al. 2018)
- Added Cetus 3 (Homma et al. 2018)
- Added Bootes 4 (Homma et al. 2019)
- Added Antlia 2 (Torrealba et al. 2019)
- Added kinematics of Carina 2 and Carina 3 (Li et al. 2018)
- Added kinematics of Crater 2 (Caldwell et al. 2017)
- Added kinematics of Horologium 2, Reticulum 3, Columba 1, Phoenix 2 (Fritz et al. 2019)
- Added kinematics of Pegasus 3 (Kim et al. 2016)
- Added kinematics of Eridanus 2 (Li et al. 2017)
- Added kinematics of Sagittarius 2 (Longeard et al. 2019)
- Added kinematics of Pisces 2 (Kirby et al. 2015)
- Added kinematics of Tucana 2 and Grus 1 (Walker et al. 2016)
- Added kinematics of Tucana 3 (Simon et al. 2017)
- Added kinematics of Reticulum 2 and Horologium 1 (Koposov et al. 2015)
- Updated position angle, ellipticity, half-light radius, V magnitude and central surface brightnesses of galaxies in the Munoz et al. 2019 sample (adopting the best-fit Sersic parameters). See their tables 5 and 6 (applies to Sculptor, Segue2, Fornax, Carina, UrsaMajor2, LeoT, Segue(1), Leo1, UrsaMajor(1), Willman1, Leo2, Leo5, Leo4, ComaBerenices, CanesVenatici2, Bootes2, Bootes(1), UrsaMinor, Hercules, Draco, Pisces2, Eridanus3, Horologium1, Horologium2, Reticulum2, Eridanus2, Pictoris1, Hydra2, Indus1, Grus1, Phoenix2)

September 20 2015

- Important note: There are an increasing number of very faint objects with an ambiguous nature (globular cluster or dwarf?). As such, I now include an asterix in front of every such object and leave it to individuals to determine if they want to include these objects in their sample or not.
- In addition to some new entries, Canis Major, Bootes III are now marked as ambiguous objects (i.e., inserted asterix)
- Added KK258 (Karachentsev et al. 2014), with some structural information from Karachentsev et al. 2013)
- Added KKs3 (Karachentsev et al. 2015a), plus velocity and structural information from Karachentsev et al. (2015b) and Karachentsev et al. (2013)
- Added Antlia B (Sand et al. 2015)
- Added Triangulum II/Leavens II (Leavens et al. 2015a)
- Added Hydra II (Martin et al. 2015), and velocity information from Kirby et al. (2015)
- Added Sagittarius II and Draco II (Leavens et al. 2015b)
- Added Reticulum 2, Eridanus 2, Horologium 1, Pictoris 1, Phoenix 2, Eridanus 3, Tucana 2 (Koposov et al. 2015, Bechtol et al. 2015) 
- Added Indus 1 (Kim et al. 2015a, Koposov et al. 2015, Bechtol et al. 2015)
- Added Grus 1 (Koposov et al. 2015)
- Added Pegasus 3 (Kim et al. 2015b)
- Added Horologium 2 (Kim & Jerjen 2015)
- Added Grus II, Tucana III, Columba I, Tucana IV, Reticulum III, Tucana V, Indus I, Cetus II (The DES Collaboration, 2015)
- Updated Leo P distance (McQuinn et al. 2015)

February 15 2014

- Added Perseus I (AndXXXIII) (Martin et al 2013b)
- Added systemic velocity and stellar velocity dispersion for AndXXIX (Tollerud et al. 2013)
- Added/updated systemic velocity, stellar velocity dispersions for IC1613, NGC6822, UGC4879, Pegasus dIrr, Leo A, Cetus and Aquarius from Kirby et al. 2013. Also included stellar rotation for Pegasus measured in the same paper.

June 17 2013
-Error corrected for SagDIG: declination changed from "-17 40 41" to "-17 40 51"
-Error corrected for Leo IV; declination changed from "0 32 0" to "-0 32 0"
-Error corrected for IC1613; the values for the HI velocity dispersion and the HI rotational velocity were incorrectly switched around in the published version. 

May 30 2013
- Added Casseopeia II (And XXX) dwarf (see Conn et al. 2012 and Collins et al. 2013)
- Added Leo P dwarf (Giovanelli et al. 2013)
- Added Lacerta I (And XXXI) and Casseopeia III (And XXXII) (Martin et al. 2013a)
- Added velocities and stellar velocity dispersions for And XVII, XIX, XX, XXIII, XXIV, XXV, XXVII, XXVIII. Added velocity for And XXVI (dispersion is very poorly constrained). Updated velocities and stellar velocity dispersions for And VI and XXI (Collins et al. 2013). Updated velocity and stellar velocity dispersion for And XXII (Chapman et al. 2013; see also Collins et al. 2013)
- Updated/added metallicity estimates for And V, VI, XI, XII, XIII, XVII, XVIII, XIX, XX, XXI, XXII, XXIII, XXIV, XXV, XXVI, XXVII, XXVIII, XXX (Collins et al. 2013) (note: I have favored spectroscopic metallicities over photometric metallicities, even if formal uncertainties are larger). Also note that inconsistent values are given in Tables 4 and 5 of Collins et al. 2013 for several of the metallicities, but the correct values have been adopted for each galaxy (M. Collins, private communication).
- Corrected Vmag values for Andromeda I, II, III, V, VI, VII and Cetus. Previously, values derived by McConnachie & Irwin (2006) that were uncorrected for reddening were cited in the table as being already corrected for reddening. The values have now been explicitly corrected (using A_V = 3.315 * E(B-V) ). Thanks to Luis Vargas for notifying me about this error!

November 12 2012
- Andromeda X, XII, XIV, XV, XVI, XVII, XVIII, XIX, XX, XXI, XXII (Conn et al. 2012): Updated distance estimates.  
- Andromeda XI, XIII (Yang et al. 2012): Updated distances (now HST RR Lyrae estimates)
- Andromeda II (Ho et al. 2012): Updated mean systemic velocity, average stellar velocity dispersion, mean metallicity. Added stellar rotation velocity.
- WLM (Leaman et al. 2012): Updated ellipticity, position angle, half-light radius, stellar rotation velocity, metallicity.
- KKR 25 (Makarov et al. 2012): Updated distance modulus, magnitude, central SB, ellipticity, half-light radius and radial velocity. 

August 23 2012
- Error corrected in "References.dat": Reference to "Brown et al. 2007" in Tables 2 and 4 of published tables corrected in reference file to "Brown, W.~R., Geller, M.~J., Kenyon, S.~J., \& Kurtz, M.~J.\ 2007, \apj, 666, 231"

June 16 2012
- Andromeda I, III, VII, IX, X, XIII, XIV, XV, XVI, XVIII, XXI, XXII (Tollerud et al. 2012): Updated systemic velocities and stellar velocity dispersions
- NGC205: Changed value for central SB to 19.2: (B band; see Geha et al. 2006) (previous value based on extrapolation of de Vaucouleurs profile into central region, and overestimated the central flux density)
- UGC4879 (Kirby et al. 2012): added stellar RV; sigma_s; Fe/H.

April 3 2012 
- No changes compared to published values in McConnachie (2012, AJ, 144, 4)