AAVSO Photometric All Sky Survey (APASS) DR10apass.dr10ivo://org.gavo.dc/apass/q/dr10The GAVO DC teamHenden, Arne A.Levine, StephenTerrell, DirkWelch, Douglas L.Munari, UlisseKloppenborg, Brian K.2020-03-04T10:28:17ZGAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837surveysvariable-stars
AAVSO Photometric All-Sky Survey (APASS), underway since 2010,
covers the entire sky from 7.5 < V < 16.5 magnitude, and in the BVugrizY
bandpasses. A northern and a southern site are used, each with twin ASA
20cm astrographs and Apogee Aspen CG16m cameras, covering 2.9x2.9 square
degrees with 2.6arcsec pixels. Landolt and SDSS standards are used for
all-sky solutions, with typical 0.02mag calibration errors on the bright
end.
Data Release 10 is a complete reprocessing of all 500K images taken with
the system, including hundreds of nights not part of DR9. Sextractor is
used for star finding and centroiding; DAOPHOT is used for aperture
photometry; the astrometry.net plate-solving library is used for basic
astrometry, supplanted with more precise WCS that utilizes knowledge of the
optical train distortions. With these changes, DR10 includes many more
stars than prior releases.
More information is available at http://www.aavso.org/apass.https://dc.zah.uni-heidelberg.de/tableinfo/apass.dr10CatalogResearchAmateurApogee Aspen CG16m0/4-11 1/0-2,4,6-7,12-13 2/12,20,32-34,36,40,61,63
3/53-55,58-62,84,88,90-91,95,140-142,168,170,187,224-226,228,240-241,243,249
4/209,211,229-231,252-254,340-341,343-346,373,375-376,378-379,572-574,592-594,601,606,608-610,628,630,637-639,656-658,669-671,686-689,691,693-694,698-699,702-703,706-707,710,712-713,717-719,723,730-731,741,745-746,752,757,761-763,765,767,908-910,916-917,919-920,928-930,936,957-959,968-970,993-995,1000-1001,1004-1005,1007
5/832-834,840,842-843,896-898,900-901,904,906-907,909-913,915,1020-1022,1368-1370,1388-1390,1395,1397,1399,1401,1404-1405,1407,1424-1426,1432,1434,1437-1439,1472-1474,1480,1482-1484,1486,1491,1497,1499,1508,1510,2300-2302,2380-2382,2384-2386,2395-2396,2398-2402,2408-2410,2416-2418,2421,2423,2444-2446,2448-2450,2464-2466,2501-2504,2506,2508-2509,2511,2518,2524,2527-2528,2530,2533,2536-2537,2539,2543-2544,2547,2636-2638,2640-2642,2653,2655-2658,2664,2666-2667,2671,2673,2675,2704-2706,2708-2709,2712,2714-2716,2718,2736-2738,2740-2741,2743,2761,2768-2769,2780,2782-2786,2788,2804-2805,2807,2822,2834-2835,2838-2839,2844,2847,2856-2857,2859-2860,2862-2864,2866-2867,2884-2885,2887-2888,2890-2891,2896-2898,2900-2901,2903-2904,2906,2912-2914,2916-2917,2933,2935,2937-2938,2940-2941,2943-2944,2946-2950,2952,2954-2955,2960-2962,2972-2973,2976-2978,2989-2991,3012,3023,3033-3037,3039,3042-3043,3056-3057,3059,3066-3067,3644-3646,3674-3675,3685,3688-3689,3692-3694,3696,3702-3703,3705-3709,3711,3724-3726,3728-3730,3752-3753,3756,3765,3770-3771,3780,3797-3799,3807-3808,3823,3827,3884,3886-3887,3968-3969,3971,4008-4010,4012-4013,4015,4024-4025
6/3340-3342,3366-3367,3596-3598,3608-3609,3612-3613,3615,3620,3622-3623,3635,3656-3658,4092,4094,5485-5487,5564,5568,5573,5575,5579,5584-5586,5592,5594,5601,5603,5609,5612-5614,5625,5627,5708-5710,5712-5714,5716-5717,5719,5725-5727,5741-5743,5745-5747,5900-5902,5904,5906,5915,5918,5924,5926-5927,5940,5942,5948,5950,5957-5959,5961,5963,5985,5993-5995,6045-6047,9212-9214,9532-9534,9548-9550,9552-9554,9556,9562-9563,9568-9570,9573-9575,9577-9579,9591,9612-9614,9644,9648-9649,9651-9653,9655,9661,9663,9676,9678-9680,9712,9714,9716-9717,9720,9788-9790,9804-9806,9808-9810,9824-9826,9847,9853,9855,9868-9870,9872-9874,9888-9890,9940-9941,9943,9949-9951,9972-9973,9975,9981,9984,9995,10003,10020,10022,10028,10030,10040-10041,10043,10066-10067,10103-10104,10107,10116,10126-10127,10129,10140,10152-10153,10155,10160,10162,10167-10168,10171,10180,10183,10187,10556-10558,10572-10574,10576-10578,10591-10594,10617,10619,10636-10638,10640-10642,10660,10662-10663,10677-10679,10681-10683,10697-10699,10828-10830,10841,10844-10845,10847,10853-10855,10868-10870,10878-10879,10956,10958,10969,10971,11041,11050-11051,11053-11055,11080,11082-11083,11085-11087,11124,11127,11148,11150-11151,11156,11161-11164,11166-11167,11201,11204-11205,11207,11210,11224-11225,11227,11275-11276,11278-11279,11293-11295,11330-11331,11334,11345-11348,11350,11380,11383-11384,11387,11432-11433,11435,11444-11445,11447,11460,11463,11521,11524,11531,11534,11544-11545,11547,11556,11558-11559,11596,11598,11609,11611,11620,11622,11628,11633,11636,11660,11662-11663,11673-11676,11678,11712,11725-11727,11731,11737-11739,11745,11747,11756-11758,11769,11771,11781-11783,11804-11806,11814-11815,11832,11834-11835,11838-11839,11852-11853,11855,11877,11882-11883,11886-11887,11897-11900,11902-11903,11916-11917,11919,11953-11955,12052-12054,12056-12058,12064,12091,12103,12109,12111,12131,12152,12154-12155,12163,12166-12167,12232-12233,12258-12259,12261-12263,14588-14590,14688-14690,14693-14695,14736-14738,14746-14747,14750,14761,14764-14765,14767,14780,14782-14783,14788-14790,14792-14793,14796,14799,14801,14804-14805,14819,14840-14841,14908-14910,14924-14926,14928-14930,14944-14946,14975,14992-14994,15002,15016-15017,15020-15021,15028,15032,15035,15038-15039,15059,15096,15098,15109-15111,15117,15124-15126,15128-15129,15146-15147,15150-15151,15169,15172,15181-15183,15185-15187,15205,15216-15217,15220,15223,15227,15236,15287,15291,15303,15307,15540,15542-15543,15880-15881,15883,16044,16046,16056-16057,16059,16104-16106,16111OpticalInfraredapassAAVSO Photometric All Sky Survey (APASS) DR10
AAVSO Photometric All-Sky Survey (APASS), underway since 2010,
covers the entire sky from 7.5 < V < 16.5 magnitude, and in the BVugrizY
bandpasses. A northern and a southern site are used, each with twin ASA
20cm astrographs and Apogee Aspen CG16m cameras, covering 2.9x2.9 square
degrees with 2.6arcsec pixels. Landolt and SDSS standards are used for
all-sky solutions, with typical 0.02mag calibration errors on the bright
end.
Data Release 10 is a complete reprocessing of all 500K images taken with
the system, including hundreds of nights not part of DR9. Sextractor is
used for star finding and centroiding; DAOPHOT is used for aperture
photometry; the astrometry.net plate-solving library is used for basic
astrometry, supplanted with more precise WCS that utilizes knowledge of the
optical train distortions. With these changes, DR10 includes many more
stars than prior releases.
More information is available at http://www.aavso.org/apass.
apass.dr10
AAVSO Photometric All-Sky Survey (APASS), underway since 2010,
covers the entire sky from 7.5 < V < 16.5 magnitude, and in the BVugrizY
bandpasses. A northern and a southern site are used, each with twin ASA
20cm astrographs and Apogee Aspen CG16m cameras, covering 2.9x2.9 square
degrees with 2.6arcsec pixels. Landolt and SDSS standards are used for
all-sky solutions, with typical 0.02mag calibration errors on the bright
end.
Data Release 10 is a complete reprocessing of all 500K images taken with
the system, including hundreds of nights not part of DR9. Sextractor is
used for star finding and centroiding; DAOPHOT is used for aperture
photometry; the astrometry.net plate-solving library is used for basic
astrometry, supplanted with more precise WCS that utilizes knowledge of the
optical train distortions. With these changes, DR10 includes many more
stars than prior releases.
More information is available at http://www.aavso.org/apass.130000000idAPASS DR10 identifier formed as (SPD zone)-(star number)meta.id;meta.maincharindexedprimaryraICRS right ascension for this object.pos.eq.ra;meta.maindoubleindexednullabledecICRS declination for this object.pos.eq.dec;meta.maindoubleindexednullablera_errorEstimated error in ra (there will be additional systematics especially in crowded fields).degstat.error;pos.eq.rafloatnullabledec_errorEstimated error in dec (there will be additional systematics especially in crowded fields).degstat.error;pos.eq.decfloatnullablenobs_bNumber of observations that went into mag_bmeta.number;obs;em.opt.Bshortmag_bMagnitude in Johnson B (Vega system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Bfloatnullableerr_mag_bEstimated error in mag_b. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Bfloatnullablenobs_vNumber of observations that went into mag_vmeta.number;obs;em.opt.Vshortmag_vMagnitude in Johnson V (Vega system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Vfloatnullableerr_mag_vEstimated error in mag_v. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Vfloatnullablenobs_uNumber of observations that went into mag_umeta.number;obs;em.opt.Ushortmag_uMagnitude in Sloan u' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Ufloatnullableerr_mag_uEstimated error in mag_u. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Ufloatnullablenobs_gNumber of observations that went into mag_gmeta.number;obs;em.opt.Vshortmag_gMagnitude in Sloan g' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Vfloatnullableerr_mag_gEstimated error in mag_g. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Vfloatnullablenobs_rNumber of observations that went into mag_rmeta.number;obs;em.opt.Rshortmag_rMagnitude in Sloan r' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Rfloatnullableerr_mag_rEstimated error in mag_r. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Rfloatnullablenobs_iNumber of observations that went into mag_imeta.number;obs;em.opt.Ishortmag_iMagnitude in Sloan i' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Ifloatnullableerr_mag_iEstimated error in mag_i. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Ifloatnullablenobs_z_sNumber of observations that went into mag_z_smeta.number;obs;em.opt.Ishortmag_z_sMagnitude in Sloan z_s (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Ifloatnullableerr_mag_z_sEstimated error in mag_z_s. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Ifloatnullablenobs_yNumber of observations that went into mag_ymeta.number;obs;em.opt.Ishortmag_yMagnitude in Sloan Y (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.Ifloatnullableerr_mag_yEstimated error in mag_y. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.Ifloatnullable