DW-NOMINATE Scores With Bootstrapped Standard Errors

Royce Carroll, Jeff Lewis, James Lo, Nolan McCarty, Keith Poole, and Howard Rosenthal

Updated 17 February 2013

This updated release of the DW-NOMINATE scores for the 1^st to the 112^th Congresses (1789 - 2012) contains parametric bootstrapped standard errors. For an explanation of the basic theory of the parametric bootstrap see:

Political Analysis

This research was made possible by NSF Grant 0611880 to Jeffrey B. Lewis, Keith T. Poole, and Howard Rosenthal. This work was also supported in part by the Rice Terascale Cluster funded by NSF under Grant EIA-0216467, and a partnership between Rice University, Intel, and HP. We thank the National Science Foundation, Rice University, and the San Diego Supercomputer Center for their support. The files below contain DW-NOMINATE scores for the 1^st to the 112^th Congresses (1789 - 2012). For an explanation of how the data is organized and formatted read this text file.

As Poole and Rosenthal explain in Ideology & Congress (the 2^nd edition of Congress: A Political-Economic History of Roll Call Voting), the first dimension can be interpreted in most periods as government intervention in the economy or liberal-conservative in the modern era. The 2^nd dimension picks up the conflict between North and South on Slavery before the Civil War and from the late 1930s through the mid-1970s, civil rights for African-Americans. After 1980 there is considerable evidence that the South realigns and the 2^nd dimension is no longer important. See our discussion of this period in our monograph: Income Redistribution and the Realignment of American Politics (joint with Nolan McCarty, 1997, AEI Press). Further discussion can also be found in Spatial Models of Parliamentary Voting by Keith Poole and in Polarized America (joint with Nolan McCarty).

In the House scaling, the second dimension weight is 0.4088 and the Beta parameter (proportional to 1/s where s is the standard deviation of the error) is 7.355. The correct classification was 87.60 percent with an APRE of 0.6308 and a geometric mean probability of 0.758. The corresponding values for the Senate scaling are .5513 and 9.0609, for the second dimension weight and Beta, respectively. The correct classification was 86.00 percent with an APRE of 0.5866 and a geometric mean probability of 0.742.

In order to calculate distances from the DW-NOMINATE scores you must multiply the second dimension by the weight parameter. To calculate the choice probabilities you must apply both the second dimension weight and the Beta parameter. Use the Yea and Nay outcome coordinates with considerable caution because, as we explain in Congress: A Political Economic History of Roll Call Voting, they are poorly identified. However, the cutting line is identified and can be used safely.

If you have used previous releases of the DW-NOMINATE scores please go to the Current vs. Past Releases of DW-NOMINATE Scores page. The scores computed for the 1^st to the 112^th (through 2010) are essentially identical to the previous release (i.e., the corresponding scores for Congresses 1 to 111). However, when a new Congress is added to the dataset this will slightly change the scores for more recent members because their scores are estimated using their entire voting history. This will also slightly change the overall means of the dimensions. Finally, the past few Congresses are nearly unidimensional with correct classifications of 90 percent or better. Consequently, the overall fit of the DW-NOMINATE estimation has increased as recent Congresses have been added to the dataset. Also note that the 2^nd dimension weight can vary somewhat from scaling to scaling because the 2^nd dimension coordinates can be contracted/expanded slightly. The weight will compensate for this. The Current vs. Past Releases of DW-NOMINATE Scores page shows the corrections necessary to map the past scalings into the current scalings along with STATA files containing the current and past releases.

Please note that the House files now contain scores for most Presidents. For Presidents prior to Eisenhower these are based on roll calls corresponding to Presidential requests. These roll calls were compiled by an NSF project headed by Elaine Swift ( Study No. 3371, Database of Congressional Historical Statistics, 1789-1989). Many of these scores are based upon a small number of roll calls so use them with caution!

If you have questions or need help with these files please send us e-mail at jblewis@ucla.edu (Jeff Lewis) or ktpoole@uga.edu (Keith Poole).

To see a QuickTime Movie of the DW-NOMINATE scalings download this movie file:

Two Dimensional Movie of the 1^st to 111^th Houses and Senates (through 2009, high resolution, 458 Megabytes!!)

The format of the legislator files is:

1. Congress Number
2. ICPSR ID Number: 5 digit code assigned by the ICPSR as
corrected by Howard Rosenthal and myself.
3. State Code: 2 digit ICPSR State Code.
4. Congressional District Number (0 if Senate)
5. State Name
6. Party Code: 100 = Dem., 200 = Repub. (See PARTY3.DAT for a full set of codes of minor and historical parties)
7. Name
8. 1st Dimension Coordinate
9. 2nd Dimension Coordinate
10. 1st Dimension Bootstrapped Standard Error
11. 2nd Dimension Bootstrapped Standard Error
12. Correlation Between 1st and 2nd Dimension Bootstrapped Estimates over the 1000 trials (for computing the ellipsoid of estimated points)
13. Log-Likelihood
14. Number of Votes
15. Number of Classification Errors
16. Geometric Mean Probability

The format of the roll call files is:

1. Congress Number
2. Roll Call Number
3. "H" if House, "S" if Senate
4. Number of Yeas
5. Number of Nays
6. Month of Roll Call
7. Day of Roll Call
8. Year of Roll Call
9. Number Correctly Classified
10. Predicted Yea/Actual Yea
11. Predicted Yea/Actual Nay
12. Predicted Nay/Actual Yea
13. Predicted Nay/Actual Nay
14. Proportion Correctly Classified (#9 divided by #4 + #5)
15. Proportional Reduction in Error (PRE) -- (Min. on RC - Error)/Min. on RC
16. Geometric Mean Probability
17. Spread on 1st Dimension -- if the roll call was not scaled, there
18. Midpoint on 1st Dimension -- are 0.000's in all four fields
19. Spread on 2nd Dimension --
20. Midpoint on 2nd Dimension --

Legislator Estimates 1^st to 112^th Houses (Text File, 37,077 lines)
Legislator Estimates 1^st to 112^th Houses (Stata File, 37,077 lines)
Legislator Estimates 1^st to 112^th Houses (Stata 9 File, 37,077 lines)
Legislator Estimates 1^st to 112^th Houses (Eviews File, 37,077 lines)
Legislator Estimates 1^st to 112^th Houses (Excel File, 37,077 lines)

Roll Call Estimates 1^st to 112^th Houses (Text File, 52,328 lines)
Roll Call Estimates 1^st to 112^th Houses (Stata File, 52,328 lines)
Roll Call Estimates 1^st to 112^th Houses (Stata 9 File, 52,328 lines)
Roll Call Estimates 1^st to 112^th Houses (Eviews File, 52,328 lines)
Roll Call Estimates 1^st to 112^th Houses (Excel File, 52,328 lines)

Roll Call Estimates 83^rd to 110^th Houses merged with Rohde/PIPC House Roll Database (STATA 9 file, 23,672 lines) -- the format of the PIPC data is outlined in the PIPC Codebook. The DW-NOMINATE roll call coordinates are tacked onto the end of the PIPC data in the same format as listed above.

Senator Estimates 1^st to 112^th Senates (Text File, 8,958 lines)
Senator Estimates 1^st to 112^th Senates (Stata File, 8,958 lines)
Senator Estimates 1^st to 112^th Senates (Stata 9 File, 8,958 lines)
Senator Estimates 1^st to 112^th Senates (Eviews File, 8,958 lines)
Senator Estimates 1^st to 112^th Senates (Excel File, 8,958 lines)

Roll Call Estimates 1^st to 112^th Senates (Text File, 48,619 lines)
Roll Call Estimates 1^st to 112^th Senates (Stata File, 48,619 lines)
Roll Call Estimates 1^st to 112^th Senates (Stata 9 File, 48,619 lines)
Roll Call Estimates 1^st to 112^th Senates (Eviews File, 48,619 lines)
Roll Call Estimates 1^st to 112^th Senates (Excel File, 48,619 lines)

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DW-NOMINATE Scores With Bootstrapped Standard Errors

Royce Carroll, Jeff Lewis, James Lo, Nolan McCarty, Keith Poole, and Howard Rosenthal Updated 17 February 2013

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Royce Carroll, Jeff Lewis, James Lo, Nolan McCarty, Keith Poole, and Howard Rosenthal

Updated 17 February 2013