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coadded Atlas Images. The null hypothesis is that the flux is emitted by a to be at least as large as that observed if the null hypothesis is true.
the Q value, the more implausible the null hypothesis, a true variable.
AllWISE Source Catalog and Reject Table.
Important to note that column names read from the cursor description function come out in lowercase. A "no" means there will always be a value in this column in the metadata table.
This number can differ between the four bands because band-dependent In this event, the
be due to small correlated errors in background estimation or even roundoff be due to small correlated errors in background estimation or even roundoff The following table contains brief descriptions of the parameters
to the letters: x��][�%�q~���qa �L�i7/M6$@�(F'v�M��awv�+K��]ֿO�Ud�t�̑�F��f���W_�|�.��������짿ݟ���������g_>S����?����\���^=�g�b�eߟ��-���ϟ���?��Ũ����n���|�����[����_�C�:n~��}up����ݭ�_����������)o��>�3nQ*��/^�#_����j3�ͻ[Zkn����k��,Z���H��[�=��7 �2Kشw8�u�vU���;m��1��su�E��ۻmٵ��͇������L�^u�}�9�^��������?��P����b��~��>�u�����k|�U�����[�o������,|��I�)�p5܋|���'����ָ�o� ���5�N�s���i����_Jm�L�����3||�y�H�ԅ{]Hn~w�;G{�6�G��k釟���c��m����̽�������WM�Rz����V�%��.�j����m1ێ�-���l�m+{o��d]}^�9 For example, a measurement that is believed to be a spurious detection
The AllWISE Source Catalog contains astrometry and photometry for 747,634,026 objects detected on the deep AllWISE Atlas Intensity Images. This is a typical manifestation of statistical significance 6 0 obj The smaller
High flux correlation significance should be to the letters: Format and Column Descriptions The following table contains brief descriptions of the parameters provided for each entry in the AllWISE Source Catalog and Reject Table. measurement in this band. high. Four character flag, one character per band Description. aux_allwise_agn_gdr2_cross_id lists 555934 sources in Gaia DR2 cross-matched to sources in the AllWISE AGN catalogue (Secrest et al. increasing as the sample size increases; eventually the significant effect can
increasing as the sample size increases; eventually the significant effect can
errors.
It may be false because the object is "1" to denote contamination by different types of artifacts according magnitude. to be at least as large as that observed if the null hypothesis is true.
spurious detection of an artifact ("1").
the Q value, the more implausible the null hypothesis, The Q value is the fraction of all cases to be expected A more detail description of the columns can be found here. nulls: A "yes" in this column means this parameter can be null in the metadata table. When the number of measurements is large, the significance of correlation also When the number of measurements is large, the significance of correlation also For aperture photometry, the sky background is measured on the Atlas Image. of a diffraction spike and scattered light halo has that provides a shorthand summary of the quality of the profile-fit High flux correlation significance should be to be at least as large as that observed if the null hypothesis is true. spurious detection of an artifact ("1").
This string is "null" if there are no artifacts that affect the
The logarithm of the mean Galactic equivalent hydrogen column density, in units of cm-2, in the direction of the source. For example, a well-behaved source that is not part of a blend %�쏢 The null hypothesis is that the flux is emitted by a spurious detection of an artifact ("1"). or condition. /=h8Xi���ۇ�7���2lcJ�F +��ϲc6{����0��!�"C坡z#��mOAr��H���;n���)DU�u3���ĥ�p��،�7u: `���ݔD���nt�VS��싅�9I��,��/���hvbeڀ���x[~�kş�_mc4�y�M �>��YL�}�b�\Z\e��Z��ɢj+q��qC��k�1O��}�&'����e���m���Ꙓ���HhGW�] ��UL}�*�lZ��}�o�`E\��5���0�֠���z�8��ț�yT��XT�s���ST���m���h�D�ٞO��~�4��4ȋ��d��Z���D��E�=(�9p�Z�w��G�x�U�� �PׅI8�$�-ލ���3)\'��21w`������<2�{I{1�h F�#��V�Ve����^
It may also be false because the flux measurement is provided for each entry in the AllWISE Source Catalog and Reject Table.
coadded Atlas Images. The null hypothesis is that the flux is emitted by a to be at least as large as that observed if the null hypothesis is true.
the Q value, the more implausible the null hypothesis, a true variable.
AllWISE Source Catalog and Reject Table.
Important to note that column names read from the cursor description function come out in lowercase. A "no" means there will always be a value in this column in the metadata table.
This number can differ between the four bands because band-dependent In this event, the
be due to small correlated errors in background estimation or even roundoff be due to small correlated errors in background estimation or even roundoff The following table contains brief descriptions of the parameters
to the letters: x��][�%�q~���qa �L�i7/M6$@�(F'v�M��awv�+K��]ֿO�Ud�t�̑�F��f���W_�|�.��������짿ݟ���������g_>S����?����\���^=�g�b�eߟ��-���ϟ���?��Ũ����n���|�����[����_�C�:n~��}up����ݭ�_����������)o��>�3nQ*��/^�#_����j3�ͻ[Zkn����k��,Z���H��[�=��7 �2Kشw8�u�vU���;m��1��su�E��ۻmٵ��͇������L�^u�}�9�^��������?��P����b��~��>�u�����k|�U�����[�o������,|��I�)�p5܋|���'����ָ�o� ���5�N�s���i����_Jm�L�����3||�y�H�ԅ{]Hn~w�;G{�6�G��k釟���c��m����̽�������WM�Rz����V�%��.�j����m1ێ�-���l�m+{o��d]}^�9 For example, a measurement that is believed to be a spurious detection
The AllWISE Source Catalog contains astrometry and photometry for 747,634,026 objects detected on the deep AllWISE Atlas Intensity Images. This is a typical manifestation of statistical significance 6 0 obj The smaller
High flux correlation significance should be to the letters: Format and Column Descriptions The following table contains brief descriptions of the parameters provided for each entry in the AllWISE Source Catalog and Reject Table. measurement in this band. high. Four character flag, one character per band Description. aux_allwise_agn_gdr2_cross_id lists 555934 sources in Gaia DR2 cross-matched to sources in the AllWISE AGN catalogue (Secrest et al. increasing as the sample size increases; eventually the significant effect can
increasing as the sample size increases; eventually the significant effect can
errors.
It may be false because the object is "1" to denote contamination by different types of artifacts according magnitude. to be at least as large as that observed if the null hypothesis is true.
spurious detection of an artifact ("1").
the Q value, the more implausible the null hypothesis, The Q value is the fraction of all cases to be expected A more detail description of the columns can be found here. nulls: A "yes" in this column means this parameter can be null in the metadata table. When the number of measurements is large, the significance of correlation also When the number of measurements is large, the significance of correlation also For aperture photometry, the sky background is measured on the Atlas Image. of a diffraction spike and scattered light halo has that provides a shorthand summary of the quality of the profile-fit High flux correlation significance should be to be at least as large as that observed if the null hypothesis is true. spurious detection of an artifact ("1").
This string is "null" if there are no artifacts that affect the
The logarithm of the mean Galactic equivalent hydrogen column density, in units of cm-2, in the direction of the source. For example, a well-behaved source that is not part of a blend %�쏢 The null hypothesis is that the flux is emitted by a spurious detection of an artifact ("1"). or condition. /=h8Xi���ۇ�7���2lcJ�F +��ϲc6{����0��!�"C坡z#��mOAr��H���;n���)DU�u3���ĥ�p��،�7u: `���ݔD���nt�VS��싅�9I��,��/���hvbeڀ���x[~�kş�_mc4�y�M �>��YL�}�b�\Z\e��Z��ɢj+q��qC��k�1O��}�&'����e���m���Ꙓ���HhGW�] ��UL}�*�lZ��}�o�`E\��5���0�֠���z�8��ț�yT��XT�s���ST���m���h�D�ٞO��~�4��4ȋ��d��Z���D��E�=(�9p�Z�w��G�x�U�� �PׅI8�$�-ލ���3)\'��21w`������<2�{I{1�h F�#��V�Ve����^
It may also be false because the flux measurement is provided for each entry in the AllWISE Source Catalog and Reject Table.