<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2024-10-31T12:55:21Z" status="active" updated="2026-02-20T09:44:50Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:ssap="http://www.ivoa.net/xml/SSA/v1.1" xmlns:vg="http://www.ivoa.net/xml/VORegistry/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://dc.g-vo.org/ColStats-1 http://vo.ari.uni-heidelberg.de/docs/schemata/Colstats.xsd http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/SSA/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/SSA.xsd http://www.ivoa.net/xml/VORegistry/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VORegistry.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>ROME/REA Timeseries Photometry Data Release 1</title><shortName>rome SSAP</shortName><identifier>ivo://org.gavo.dc/rome/q/ssa</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Street, R.A.</name></creator><creator><name>Bachelet, E.</name></creator><creator><name>Tsapras, Y.</name></creator><creator><name>Hundertmark, M.P.G.</name></creator><creator><name>Bozza, V.</name></creator><creator><name>Bramich, D.M.</name></creator><creator><name>Cassan, A.</name></creator><creator><name>Dominik, M.</name></creator><creator><name>Figuera Jaimes, R.</name></creator><creator><name>Horne, K.</name></creator><creator><name>Mao, S.</name></creator><creator><name>Saha, A.</name></creator><creator><name>Wambsganss, J.</name></creator><creator><name>Zang, W.</name></creator><date role="Updated">2026-02-20T09:44:41Z</date><contact><name>GAVO Data Centre Team</name><address>Mönchhofstrasse 12-14, D-69120 Heidelberg</address><email>gavo@ari.uni-heidelberg.de</email><telephone>+49 6221 54 1837</telephone></contact></curation><content><subject>broad-band-photometry</subject><subject>ccd-photometry</subject><subject>light-curves</subject><subject>multi-color-photometry</subject><subject>photometry</subject><subject>sloan-photometry</subject><subject>stellar-photometry</subject><subject>gravitational-microlensing</subject><subject>variable-stars</subject><description> The ROME/REA (Robotic Observations of Microlensing Events/Reactive
Event Assessment) Survey was a Key Project at Las Cumbres Observatory
(hereafter LCO) which continuously monitored 20 selected fields (3.76
sq.deg.) in the Galactic Bulge throughout their seasonal visibility
window over a three-year period, between March 2017 and March 2020.
Observations were made in three optical passbands (SDSS g', r', i'),
and LCO's multi-site telescope network enabled the survey to achieve a
typical cadence of ~10hrs in i' and ~15hrs in g' and r'.     In
addition, intervals of higher cadence (&lt;1hr) data were obtained during
monitoring of key microlensing events within the fields.        This
catalog includes the full timeseries photometry for all ~8 million
stars, down to a limiting magnitude of i~18mag.</description><source format="bibcode">2024PASP..136f4501S</source><referenceURL>http://dc.g-vo.org/rome/q/ssa/info</referenceURL><type>Survey</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://org.gavo.dc/__system__/obscore/obscore">GAVO Data Center Obscore</relatedResource><relatedResource ivo-id="ivo://org.gavo.dc/tap">GAVO Data Center TAP service</relatedResource></relationship></content><rights rightsURI="https://spdx.org/licenses/CC-BY-SA-4.0.html">The ROME/REA data is licensed under the `Creative Commons Attribution Share-Alike 4.0 License &lt;http://creativecommons.org/licenses/by-sa/4.0/&gt;`_

.. image:: /static/img/ccbysa.png
   :alt: [CC-BY-SA]
</rights><rights>
This data release is a public product of the ROME/REA Key Project survey
conducted on the robotic telescope network of the Las Cumbres Observatory
(LCO).  Individual images used in the data reduction are freely available
for download on the LCO archive (https://archive.lco.global/).

It is important to clarify that the light curves available through this
data release are not optimized photometric reductions of individual
objects.  Researchers intending to utilize this data set for publications
are kindly requested to acknowledge this source by citing the present paper
(Street et al 2024 :bibcode:`2024PASP..136f4501S`) along with the original
work by Tsapras et al 2019 :bibcode:`2019PASP..131l4401T`.

For research work that requires enhanced photometry for specific targets
within this catalog, we encourage reaching out to us directly.
Collaboration opportunities are sincerely welcomed, and we look forward to
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Event Assessment) Survey was a Key Project at Las Cumbres Observatory
(hereafter LCO) which continuously monitored 20 selected fields (3.76
sq.deg.) in the Galactic Bulge throughout their seasonal visibility
window over a three-year period, between March 2017 and March 2020.
Observations were made in three optical passbands (SDSS g', r', i'),
and LCO's multi-site telescope network enabled the survey to achieve a
typical cadence of ~10hrs in i' and ~15hrs in g' and r'.     In
addition, intervals of higher cadence (&lt;1hr) data were obtained during
monitoring of key microlensing events within the fields.        This
catalog includes the full timeseries photometry for all ~8 million
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Event Assessment) Survey was a Key Project at Las Cumbres Observatory
(hereafter LCO) which continuously monitored 20 selected fields (3.76
sq.deg.) in the Galactic Bulge throughout their seasonal visibility
window over a three-year period, between March 2017 and March 2020.
Observations were made in three optical passbands (SDSS g', r', i'),
and LCO's multi-site telescope network enabled the survey to achieve a
typical cadence of ~10hrs in i' and ~15hrs in g' and r'.     In
addition, intervals of higher cadence (&lt;1hr) data were obtained during
monitoring of key microlensing events within the fields.        This
catalog includes the full timeseries photometry for all ~8 million
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column</description><ucd>meta.unit</ucd><utype>ssa:Char.SpectralAxis.Unit</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>ssa_fluxsi</name><description>Flux/magnitude conversion factor in Osuna-Salgado convention</description><utype>ssa:Dataset.FluxSI</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_fluxucd</name><description>UCD of the flux column</description><ucd>meta.ucd</ucd><utype>ssa:Char.FluxAxis.Ucd</utype><stats><option freq="1">phot.mag;em.opt</option></stats><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>ssa_fluxunit</name><description>Unit of the flux column</description><ucd>meta.unit</ucd><utype>ssa:Char.FluxAxis.Unit</utype><stats><option freq="1">mag</option></stats><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>ssa_dstype</name><description>Type of data (spectrum, time series, etc)</description><utype>ssa:Dataset.Type</utype><stats><option freq="1">spectrum</option></stats><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_publisher</name><description>Publisher of the datasets included here.</description><ucd>meta.curation</ucd><utype>ssa:Curation.Publisher</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>ssa_creator</name><description>Creator of the datasets included here.</description><utype>ssa:DataID.Creator</utype><dataType arraysize="*" xsi:type="vs:VOTableType">unicodeChar</dataType><flag>nullable</flag></column><column><name>ssa_collection</name><description>A short handle naming the collection this spectrum belongs to.</description><utype>ssa:DataID.Collection</utype><stats><option freq="1">ROME/REA time series</option></stats><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_instrument</name><description>Instrument or code used to produce these datasets</description><ucd>meta.id;instr</ucd><utype>ssa:DataID.Instrument</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_datasource</name><description>Method of generation for the data (one of survey, pointed, theory, custom, artificial).</description><utype>ssa:DataID.DataSource</utype><stats><option freq="1">pointed</option></stats><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_creationtype</name><description>Process used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)</description><utype>ssa:DataID.CreationType</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_reference</name><description>URL or bibcode of a publication describing this data.</description><ucd>meta.bib.bibcode</ucd><utype>ssa:Curation.Reference</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_fluxstaterror</name><description>Statistical error in flux</description><ucd>stat.error;phot.flux.density;em</ucd><utype>ssa:Char.FluxAxis.Accuracy.StatError</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_fluxsyserror</name><description>Systematic error in flux</description><ucd>stat.error.sys;phot.flux.density;em</ucd><utype>ssa:Char.FluxAxis.Accuracy.SysError</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_fluxcalib</name><description>Type of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).</description><utype>ssa:Char.FluxAxis.Calibration</utype><stats><option freq="1">ABSOLUTE</option></stats><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_binsize</name><description>Bin size in wavelength</description><unit>m</unit><ucd>em.wl;spect.binSize</ucd><utype>ssa:Char.SpectralAxis.Accuracy.BinSize</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_spectstaterror</name><description>Statistical error in wavelength</description><unit>m</unit><ucd>stat.error;em</ucd><utype>ssa:Char.SpectralAxis.Accuracy.StatError</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_spectsyserror</name><description>Systematic error in wavelength</description><unit>m</unit><ucd>stat.error.sys;em</ucd><utype>ssa:Char.SpectralAxis.Accuracy.SysError</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_speccalib</name><description>Type of wavelength calibration</description><ucd>meta.code.qual</ucd><utype>ssa:Char.SpectralAxis.Calibration</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_specres</name><description>Resolution (in meters of wavelength) on the spectral axis</description><unit>m</unit><ucd>spect.resolution;em.wl</ucd><utype>ssa:Char.SpectralAxis.Resolution</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_spaceerror</name><description>Statistical error in position</description><unit>deg</unit><ucd>stat.error;pos.eq</ucd><utype>ssa:Char.SpatialAxis.Accuracy.StatError</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_spacecalib</name><description>Type of calibration in spatial coordinates</description><ucd>meta.code.qual</ucd><utype>ssa:Char.SpatialAxis.Calibration</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ssa_spaceres</name><description>Spatial resolution of data</description><unit>deg</unit><ucd>pos.angResolution</ucd><utype>ssa:Char.SpatialAxis.Resolution</utype><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ssa_region</name><description>Rough coverage based on location and aperture.</description><ucd>pos.outline;obs.field</ucd><dataType arraysize="*" extendedType="polygon" xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>rome_id</name><description>Local unique identifier for this object within ROME/REA: field*10'000'000+quadrant*1'000'000'+quadrant_id</description><ucd>meta.id;meta.main</ucd><stats><min>11000001</min><percentile03>13039417.57</percentile03><median>112033866.5</median><percentile97>202117348.43</percentile97><max>204121664</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>upstream_name</name><description>Upstream has a field/field_id naming scheme skipping the quadrants. This column can be used to go from our data to upstream's.</description><ucd>meta.id</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>ra</name><description>ICRS right ascension of this object</description><unit>deg</unit><ucd>meta.id;meta.main</ucd><stats><min>267.582</min><percentile03>267.845</percentile03><median>269.363</median><percentile97>270.949</percentile97><max>271.091</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>dec</name><description>ICRS declination of this object</description><unit>deg</unit><ucd>meta.id;meta.main</ucd><stats><min>-30.4776</min><percentile03>-30.2599</percentile03><median>-29.0399</median><percentile97>-27.9015</percentile97><max>-27.7591</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>hjd_min</name><description>Earliest observation represented in the time series</description><unit>d</unit><ucd>time.epoch;stat.min</ucd><stats><min>2.45783e+06</min><percentile03>2.45785e+06</percentile03><median>2.45786e+06</median><percentile97>2.45834e+06</percentile97><max>2.45874e+06</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>hjd_max</name><description>Latest observation represented in the time series</description><unit>d</unit><ucd>time.epoch;stat.max</ucd><stats><min>2.45785e+06</min><percentile03>2.45828e+06</percentile03><median>2.45874e+06</median><percentile97>2.45877e+06</percentile97><max>2.45902e+06</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>mag_i_min</name><description>Minimal (brightest) magnitude measured in the SDSS i' band.</description><unit>mag</unit><ucd>phot.mag;em.opt.i;stat.min</ucd><stats><min>2.91403</min><percentile03>11.3486</percentile03><median>15.6404</median><percentile97>17.7778</percentile97><max>29.3848</max><fillFactor>0.937083</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>mag_i_max</name><description>Maximal (faintest) magnitude measured the SDSS i' band.</description><unit>mag</unit><ucd>phot.mag;em.opt.i;stat.max</ucd><stats><min>8.67236</min><percentile03>15.3517</percentile03><median>19.4292</median><percentile97>24.6511</percentile97><max>40.195</max><fillFactor>0.937083</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>mag_i_mean</name><description>Mean magnitude of the SDSS i' lightcurve.</description><unit>mag</unit><ucd>phot.mag;em.opt.i;stat.mean</ucd><stats><min>8.67236</min><percentile03>14.7281</percentile03><median>17.4295</median><percentile97>19.6047</percentile97><max>29.3848</max><fillFactor>0.937083</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>np_i</name><description>Number of measurements in the SDSS i' lightcurve.</description><ucd>meta.number;obs</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>137.0</median><percentile97>535.0</percentile97><max>754</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>mag_g_min</name><description>Minimal (brightest) magnitude measured in the SDSS g' band.</description><unit>mag</unit><ucd>phot.mag;em.opt.v;stat.min</ucd><stats><min>6.77246</min><percentile03>15.8543</percentile03><median>18.3894</median><percentile97>20.4182</percentile97><max>30.0845</max><fillFactor>0.55899</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mag_g_max</name><description>Maximal (faintest) magnitude measured the SDSS g' band.</description><unit>mag</unit><ucd>phot.mag;em.opt.v;stat.max</ucd><stats><min>12.4383</min><percentile03>17.5561</percentile03><median>20.7964</median><percentile97>25.3226</percentile97><max>39.1674</max><fillFactor>0.55899</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mag_g_mean</name><description>Mean magnitude of the SDSS g' lightcurve.</description><unit>mag</unit><ucd>phot.mag;em.opt.v;stat.mean</ucd><stats><min>11.8468</min><percentile03>17.1248</percentile03><median>19.6377</median><percentile97>21.6244</percentile97><max>30.0845</max><fillFactor>0.55899</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>np_g</name><description>Number of measurements in the SDSS g' lightcurve.</description><ucd>meta.number;obs</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>7.0</median><percentile97>193.0</percentile97><max>222</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>mag_r_min</name><description>Minimal (brightest) magnitude measured in the SDSS r' band.</description><unit>mag</unit><ucd>phot.mag;em.opt.r;stat.min</ucd><stats><min>5.52769</min><percentile03>14.2391</percentile03><median>17.0227</median><percentile97>19.1476</percentile97><max>30.5101</max><fillFactor>0.761248</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mag_r_max</name><description>Maximal (faintest) magnitude measured the SDSS r' band.</description><unit>mag</unit><ucd>phot.mag;em.opt.r;stat.max</ucd><stats><min>10.3503</min><percentile03>16.2028</percentile03><median>19.4742</median><percentile97>24.4083</percentile97><max>38.0622</max><fillFactor>0.761248</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mag_r_mean</name><description>Mean magnitude of the SDSS r' lightcurve.</description><unit>mag</unit><ucd>phot.mag;em.opt.r;stat.mean</ucd><stats><min>10.3503</min><percentile03>15.807</percentile03><median>18.3151</median><percentile97>20.483</percentile97><max>30.5101</max><fillFactor>0.761248</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>np_r</name><description>Number of measurements in the SDSS r' lightcurve.</description><ucd>meta.number;obs</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>62.0</median><percentile97>214.0</percentile97><max>294</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>field</name><description>ROME field the object was observed in</description><ucd>meta.id;obs.field</ucd><stats><min>1</min><percentile03>1.0</percentile03><median>11.0</median><percentile97>20.0</percentile97><max>20</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>quadrant</name><description>Quadrant of this object (for purely technical reasons, ROME has split each field into four quadrants).</description><ucd>meta.id;obs.field</ucd><stats><min>1</min><percentile03>1.0</percentile03><median>2.0</median><percentile97>4.0</percentile97><max>4</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>quadrant_id</name><description>Identifier for this object within its quadrant</description><ucd>meta.id</ucd><stats><min>1</min><percentile03>3560.0</percentile03><median>49191.0</median><percentile97>106596.0</percentile97><max>127612</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>gaia_source_id</name><description>Gaia DR3 source_id for this object</description><ucd>meta.id.cross</ucd><stats><min>4050387497117365632</min><percentile03>4.05620800677535e+18</percentile03><median>4.0622685448858225e+18</median><percentile97>4.0627713352638607e+18</percentile97><max>4063522576563088000</max><fillFactor>0.50245965</fillFactor></stats><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>