apass.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 Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@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.2018AAS...23222306Hhttps://dc.g-vo.org/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 6/3340-3342,3366-3367,3596-3598,3608-3609,3612-3613,3615,3620,3622-3623,3635,3656-3658,4092,4094,5485-5487,5564,5568,5573,5575,5579,5584-5586,5592,5594,5601,5603,5609,5612-5614,5625,5627,5708-5710,5712-5714,5716-5717,5719,5725-5727,5741-5743,5745-5747,5900-5902,5904,5906,5915,5918,5924,5926-5927,5940,5942,5948,5950,5957-5959,5961,5963,5985,5993-5995,6045-6047,9212-9214,9532-9534,9548-9550,9552-9554,9556,9562-9563,9568-9570,9573-9575,9577-9579,9591,9612-9614,9644,9648-9649,9651-9653,9655,9661,9663,9676,9678-9680,9712,9714,9716-9717,9720,9788-9790,9804-9806,9808-9810,9824-9826,9847,9853,9855,9868-9870,9872-9874,9888-9890,9940-9941,9943,9949-9951,9972-9973,9975,9981,9984,9995,10003,10020,10022,10028,10030,10040-10041,10043,10066-10067,10103-10104,10107,10116,10126-10127,10129,10140,10152-10153,10155,10160,10162,10167-10168,10171,10180,10183,10187,10556-10558,10572-10574,10576-10578,10591-10594,10617,10619,10636-10638,10640-10642,10660,10662-10663,10677-10679,10681-10683,10697-10699,10828-10830,10841,10844-10845,10847,10853-10855,10868-10870,10878-10879,10956,10958,10969,10971,11041,11050-11051,11053-11055,11080,11082-11083,11085-11087,11124,11127,11148,11150-11151,11156,11161-11164,11166-11167,11201,11204-11205,11207,11210,11224-11225,11227,11275-11276,11278-11279,11293-11295,11330-11331,11334,11345-11348,11350,11380,11383-11384,11387,11432-11433,11435,11444-11445,11447,11460,11463,11521,11524,11531,11534,11544-11545,11547,11556,11558-11559,11596,11598,11609,11611,11620,11622,11628,11633,11636,11660,11662-11663,11673-11676,11678,11712,11725-11727,11731,11737-11739,11745,11747,11756-11758,11769,11771,11781-11783,11804-11806,11814-11815,11832,11834-11835,11838-11839,11852-11853,11855,11877,11882-11883,11886-11887,11897-11900,11902-11903,11916-11917,11919,11953-11955,12052-12054,12056-12058,12064,12091,12103,12109,12111,12131,12152,12154-12155,12163,12166-12167,12232-12233,12258-12259,12261-12263,14588-14590,14688-14690,14693-14695,14736-14738,14746-14747,14750,14761,14764-14765,14767,14780,14782-14783,14788-14790,14792-14793,14796,14799,14801,14804-14805,14819,14840-14841,14908-14910,14924-14926,14928-14930,14944-14946,14975,14992-14994,15002,15016-15017,15020-15021,15028,15032,15035,15038-15039,15059,15096,15098,15109-15111,15117,15124-15126,15128-15129,15146-15147,15150-15151,15169,15172,15181-15183,15185-15187,15205,15216-15217,15220,15223,15227,15236,15287,15291,15303,15307,15540,15542-15543,15880-15881,15883,16044,16046,16056-16057,16059,16104-16106,16111OpticalInfraredapass 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.main0.00010522.3253214.135339.4993601doubleindexednullabledecICRS declination for this object.pos.eq.dec;meta.main-89.9695-71.1344-17.654762.918788.73171doubleindexednullablera_errorEstimated error in ra (there will be additional systematics especially in crowded fields).degstat.error;pos.eq.ra02.72222e-050.0001086110.0002636110.002310561floatnullabledec_errorEstimated error in dec (there will be additional systematics especially in crowded fields).degstat.error;pos.eq.dec02.27778e-058.52778e-050.0002116670.001908331floatnullablenobs_bNumber of observations that went into mag_bmeta.number;obs;em.opt.B00.03.013.012781.0shortmag_bMagnitude in Johnson B (Vega system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.B5.13313.15816.82218.20923.6320.787311floatnullableerr_mag_bEstimated error in mag_b. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.B00.0120.0980.3069.9990.787311floatnullablenobs_vNumber of observations that went into mag_vmeta.number;obs;em.opt.V00.03.013.012831.0shortmag_vMagnitude in Johnson V (Vega system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.V5.14412.36415.86717.42624.5320.787853floatnullableerr_mag_vEstimated error in mag_v. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.V00.010.0730.2279.9990.787853floatnullablenobs_uNumber of observations that went into mag_umeta.number;obs;em.opt.U00.00.00.001.0shortmag_uMagnitude in Sloan u' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.U0floatnullableerr_mag_uEstimated error in mag_u. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.U0floatnullablenobs_gNumber of observations that went into mag_gmeta.number;obs;em.opt.V01.04.016.012771.0shortmag_gMagnitude in Sloan g' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.V5.72713.00416.6518.23529.7460.978378floatnullableerr_mag_gEstimated error in mag_g. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.V00.010.0710.2619.9990.978378floatnullablenobs_rNumber of observations that went into mag_rmeta.number;obs;em.opt.R01.04.015.012681.0shortmag_rMagnitude in Sloan r' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.R4.91812.31515.81917.421.2190.97411floatnullableerr_mag_rEstimated error in mag_r. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.R00.0110.0830.2499.5450.97411floatnullablenobs_iNumber of observations that went into mag_imeta.number;obs;em.opt.I00.03.014.012651.0shortmag_iMagnitude in Sloan i' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.I3.68811.72915.11816.50821.2240.772479floatnullableerr_mag_iEstimated error in mag_i. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.I00.0140.110.3329.9990.772479floatnullablenobs_z_sNumber of observations that went into mag_z_smeta.number;obs;em.opt.I00.00.02.03941.0shortmag_z_sMagnitude in Sloan z_s (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.I2.2079.62712.83313.96519.9190.0984147floatnullableerr_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.I00.0080.1060.3889.9990.0984147floatnullablenobs_yNumber of observations that went into mag_ymeta.number;obs;em.opt.I00.00.00.001.0shortmag_yMagnitude in Sloan Y (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.I0floatnullableerr_mag_yEstimated error in mag_y. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.I0floatnullable