The author inserts a macro to the LaTeX source of the paper: 

\documentstyle[twoside, epsfig]{article}

\input ibvs2.sty

\begin{document}

\IBVShead{5488}{16 December 2003}

\IBVStitle{Superhumps in the 2003 UV P\lowercase{er} Superoutburst}

\IBVSauth{Price, A.$^{1}$; Cook, L.$^{2}$; Vanmunster, T.$^{3}$; Messier, D.$^{4
}$; Boyd, D.$^{5}$; Oksanen, A.$^{6}$; Gary, B.$^{7}$; Billings, G.$^{8}$; Graha
m, K.$^{9}$; Goff, B.$^{1}$; West, D$.^{10}$; Schmeer, P.$^{11}$; Henden, A.$^{1
2}$; Zissell, R.$^{13}$; Templeton, M. R.$^{1}$; Mattei, J. A.$^{1}$}

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UBVRI field calibration was performed on multiple nights
using the USNO-FS 1.0m telescope along with a large set of Landolt
standards of wide color and airmass.  In Table 1 we present the
comparison stars used by observers and their V-R colors used to minimize
the possibility that they may be variable. A complete table of field
stars, including complete UBVRI data, is given in 5488-t3.txt.

\IBVSedata{5488-t3.txt}
%%\IBVSdataKey{5488-t3.txt}{UV Per}{photometry}
\AladinChart{5488-t3}


     A linear fit was applied to the datasets
from each separate observing session to remove the overall fading behavior and
zero point differences between filtered and unfiltered observers. The combined d
ata

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... and submits the sequence in a simple ASCII text file: 


#ID: IBVS 5488-t3.txt
#Author: Price, A. et al.
#Observer: Henden, A.
#Description: UV Per field
#UCD:ID_MAIN POS_EQ_RA_MAIN --- POS_EQ_DEC_MAIN --- --- PHOT_JHN_V PHOT_JHN_B-V PHOT_JHN_U-B PHOT_JHN_V-R PHOT_JHN_R-I --- --- --- --- ---
#unit:--- h:m:s --- d:m:s --- --- mag mag mag mag mag --- --- --- --- ---
#name:Name    _RAJ2000   raerr  _DEJ2000  decerr  nobs   V     B-V     U-B     V-R     R-I     V_error B-V_error U-B_error V-R_error R-I_error
UV_PER_1      32.363750  0.000  57.132525  0.002    2 14.928 --- --- --- ---  0.002  ---  ---  ---  ---
UV_PER_2      32.364955  0.000  57.171565  0.002    2 16.799  1.194 --- --- ---  0.003  0.000  ---  ---  ---
UV_PER_3      32.365550  0.000  57.169280  0.002    2 18.185 --- --- --- ---  0.004  ---  ---  ---  ---
UV_PER_4      32.365600  0.001  57.227325  0.002    2 18.234  0.975 --- --- ---  0.001  0.000  ---  ---  ---
UV_PER_5      32.365853  0.045  57.263990  0.094    3 17.511  0.627 --- --- ---  0.004  0.006  ---  ---  ---
UV_PER_6      32.365957  0.011  57.224263  0.114    3 17.776  0.807 --- --- ---  0.064  0.044  ---  ---  ---
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... which will appear in the HTML paper as a link...

IBVS 5488 (16 December 2003)

COMMISSIONS 27 AND 42 OF THE IAU
INFORMATION BULLETIN ON VARIABLE STARS
Number 5488

Konkoly Observatory
Budapest
16 December 2003
HU ISSN 0374 - 0676  (print)
HU ISSN 1587 - 2440  (on-line)

Superhumps in the 2003 UV Per Superoutburst

Price, A.1; Cook, L.2; Vanmunster, T.3; Messier, D.4; Boyd, D.5; Oksanen, A.6; Gary, B.7; Billings, G.8; Graham, K.9; Goff, B.1; West, D.10; Schmeer, P.11; Henden, A.12; Zissell, R.13; Templeton, M. R.1; Mattei, J. A.1

(1) American Association of Variable Star Observers (AAVSO), Clinton B. Ford Astronomical Data & Research Center 25 Birch St., Cambridge, MA 02138, USA; email: aavso@aavso.org

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(12) Universities Space Research Association/U. S. Naval Obs ervatory, Flagstaff, AZ 86001 USA;
email: aah@nofs.navy.mil

(13) Williston Observatory, Mount Holyoke College, South Had ley, MA 0175, USA;
e-mail: rzissell@mhc.mtholyoke.edu

SIMBAD object(s):    UV Per

Type(s):    UGSU

Keyword(s):    stars: activity: superoutburst - stars: variables

Abstract:   UV Per was detected in outburst on November 04.767, 2003 (2452948.267). On November 07.8330, 2003 (2452951.3330) UT superhumps were detected indicating that this was a superoutburst. The superoutburst continued until around November 19, 2003 (2452963) UT. 11,545 CCD observations were reported to the AAVSO during the superoutburst providing a superhump period of 95.92 +/- 0.006 minutes with a decline of 0.05% per day and an amplitude decline of 3.1% per day. In addition, a supercycle of 871 +/- 379 days was calculated based on the past 40 years of superoutburst behavior.

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UBVRI field calibration was performed on multiple nights using the USNO-FS 1.0m telescope along with a large set of Landolt standards of wide color and airmass. In Table 1 we present the comparison stars used by observers and their V-R colors used to minimize the possibility that they may be variable. A complete table of field stars, including complete UBVRI data, is given in 5488-t3.txt.

Data file: /pub/ibvs//5488-t3.txt
AladinChart: 5488-t3

A linear fit was applied to the datasets from each separate observing session to remove the overall fading behavior and .
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... clicking on the link (which contains a little script in it) instructs Aladin to request a specific file from the IBVS server. The request starts at IBVS a CGI program which (using a Perl script written by A. Sragli) converts tha text table to VOTable XML on-the-fly:

... and sends it to the Aladin sky atlas, which displays the IBVS table overlayed on the default image: