Mission Overview
WISE + Pan-STARRS1 Source Types and Redshifts with Machine Learning (WISE-PS1-STRM)
Primary Investigator: István Szapudi
HLSP Authors: Robert Beck, Curt Dodds
Released: 2022-09-14
Updated: 2022-09-14
Primary Reference(s): Beck et al. 2022
DOI: 10.17909/wf64-kq10
Citations: See ADS Statistics
Overview
WISE-PS1-STRM is a neural network source classification and photometric redshift catalog extracted from a cross-match between the WISE All-Sky and PS1 3π DR2 source catalogs. The resulting catalog has 354,590,570 objects, significantly fewer than the parent PS1 catalog, but its combination of optical and infrared colors facilitate both better source classification and photometric redshift estimation. A neural network classified objects into galaxies, quasars, and stars, then another network estimated photometric redshifts for the galaxies. The star sample purity and quasar sample completeness measures improve substantially, and the resulting photo-z ’s are significantly more accurate in terms of statistical scatter and bias than those calculated from PS1 properties alone. See the README file and the primary reference paper for a detailed description of the catalog metadata.
A related, earlier work using neural networks to classify PS1 sources (without WISE information) can be found as the PS1-STRM HLSP.
Data Products
Data file naming convention:
hlsp_wise-ps1-strm_ps1-wise_multi_<decmin>-<decmax>_multi_v1_cat.csv.gz
where:
- <decmin> = Minimum declination this file covers (in degrees). "m" and "p" represent negative and postive signs.
- <decmax> = Maximum declination this file covers (in degrees). "m" and "p" represent negative and postive signs.
An example file name that covers a declination range from -5 < dec < +0 degrees is:
hlsp_wise-ps1-strm_ps1-wise_multi_m05-p00_multi_v1_cat.csv.gz
Data file types:
_cat.csv.gz |
Portion of the catalog covering a given declination range. |
_sha256sum.txt |
Checksum file for all _cat.csv.gz files. |
_readme.txt |
README containing a description of the catalog and columns. |
Catalog Column Descriptions
Click the Expand All link to see a table describing the catalog column names, units, and descriptions.
Name | Unit | Data Type | Size | Description |
---|---|---|---|---|
objID | dimensionless | bigint | 8 | [PS1] The main PS1 source identifier, should be used to match with other PS1 tables. Not unique. |
raMean | deg | float | 8 | [PS1] Right ascension from single-epoch detections (weighted mean) in equinox J2000 at the mean epoch given by epochMean. |
raMeanErr | arcsec | real | 4 | [PS1] Right ascension standard deviation from single-epoch detections. |
decMean | deg | float | 8 | [PS1] Decl. from single-epoch detections (weighted mean) in equinox J2000 at the mean epoch given by epochMean. |
decMeanErr | arcsec | real | 4 | [PS1] Decl. standard deviation from single-epoch detections. |
l | deg | float | 8 | [PS1] Galactic longitude. |
b | deg | float | 8 | [PS1] Galactic latitude. |
distance_Deg | deg | float | 8 | The angular distance between the PS1 and WISE detections, in degrees. |
sqrErr_Arcsec | arcsec^2 | float | 8 | The combined PS1-WISE astrometric uncertainty, squared, in arcsec^2. |
BayesFactor | dimensionless | float | 8 | The Bayes factor (likelihood ratio) of the PS1-WISE cross-match (see Sect. 3.1 of B22). |
cntr | dimensionless | bigint | 8 | [WISE] Unique identification number for the Catalog source. Refer to https://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec2_2a.html for more information. |
HtmID | dimensionless | bigint | 8 | [PS1] Hierarchical triangular mesh (Szalay et al. 2007) index. |
ra | deg | float | 8 | [WISE] J2000 right ascension with respect to the 2MASS PSC reference frame |
dec | deg | float | 8 | [WISE] J2000 declination with respect to the 2MASS PSC reference frame. |
sigra | arcsec | float | 8 | [WISE] One-sigma uncertainty in right ascension coordinate. |
sigdec | arcsec | float | 8 | [WISE] One-sigma uncertainty in declination coordinate. |
sigradec | arcsec | float | 8 | [WISE] The co-sigma of the equatorial position uncertainties, sig_ra, sig_dec (-â+¦, -â+¦). The co-sigma is related to the covariance between the position errors V+¦+¦ by the formula V+¦+¦ = -â+¦+¦+ù|-â+¦+¦|. This maintains the sign information for the correlation, since -â+¦+¦ may be negative. It is more natural to carry the co-sigma along with the other uncertainties instead of the covariance because the former is in the same units as the other uncertainties. |
cc_flags | dimensionless | varchar | 4 | [WISE] Contamination and confusion flag. Four character string, one character per band [W1/W2/W3/W4], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact. |
ext_flg | dimensionless | smallint | 2 | [WISE] Extended source flag. This is an integer flag, the value of which indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band, or whether the source is associated with or superimposed on a previously known extended object from the 2MASS Extended Source Catalog (XSC). |
ph_qual | dimensionless | varchar | 4 | [WISE] Photometric quality flag. Four character flag, one character per band [W1/W2/W3/W4], that provides a shorthand summary of the quality of the profile-fit photometry measurement in each band, as derived from the measurement signal-to-noise ratio. |
moon_lev | dimensionless | varchar | 4 | [WISE] Scattered moonlight contamination flag. This is a four-character string, one character per band, in which the value is an integer indicates the fraction of single-exposure frames on which the source was measured that were possibly contaminated by scattered moonlight. |
w1mpro | mag | float | 8 | [WISE] W1 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W1 flux measurement has SNR<2. This column is null if the source is nominally detected in W1, but no useful brightness estimate could be made. |
w1sigmpro | mag | float | 8 | [WISE] W1 profile-fit photometric measurement uncertainty in mag units. This column is null if the W1 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable. |
w1rchi2 | dimensionless | float | 8 | [WISE] Reduced -ç2 of the W1 profile-fit photometry measurement. This column is null if the W1 magnitude is a 95% confidence upper limit (i.e. the source is not detected). |
w1sat | dimensionless | float | 8 | [WISE] Saturated pixel fraction, W1. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W1]~8 mag. Saturation may occur in fainter sources because of a charged particle strike. |
w1mag | mag | float | 8 | [WISE] W1 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w1mcor. |
w1sigm | mag | float | 8 | [WISE] Uncertainty in the W1 "standard" aperture magnitude. |
w1flg | dimensionless | smallint | 2 | [WISE] W1 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag value is an integer that is the combination of one or more of the following values that signify different conditions: |
w1mag_1 | mag | float | 8 | [WISE] W1 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w1sigm_1 | mag | float | 8 | [WISE] Uncertainty in the W1 5.5" radius aperture magnitude. |
w1flg_1 | dimensionless | smallint | 2 | [WISE] W1 5.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w1flg. |
w1mag_4 | mag | float | 8 | [WISE] W1 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w1sigm_4 | mag | float | 8 | [WISE] Uncertainty in the W1 13.75" radius aperture magnitude. |
w1flg_4 | dimensionless | smallint | 2 | [WISE] W1 13.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w1flg. |
w1mag_7 | mag | float | 8 | [WISE] W1 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w1sigm_7 | mag | float | 8 | [WISE] Uncertainty in the W1 22.0" radius aperture magnitude. |
w1flg_7 | dimensionless | smallint | 2 | [WISE] W1 22.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w1flg. |
w2mpro | mag | float | 8 | [WISE] W2 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W2 flux measurement has SNR<2. This column is null if the source is nominally detected in W2, but no useful brightness estimate could be made. |
w2sigmpro | mag | float | 8 | [WISE] W2 profile-fit photometric measurement uncertainty in mag units. This column is null if the W2 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable. |
w2rchi2 | dimensionless | float | 8 | [WISE] Reduced -ç2 of the W2 profile-fit photometry measurement. This column is null if the W2 magnitude is a 95% confidence upper limit (i.e. the source is not detected). |
w2sat | dimensionless | float | 8 | [WISE] Saturated pixel fraction, W2. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W2]~7 mag. Saturation may occur in fainter sources because of a charged particle strike. |
w2mag | mag | float | 8 | [WISE] W2 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w2mcor. |
w2sigm | mag | float | 8 | [WISE] Uncertainty in the W2 "standard" aperture magnitude. |
w2flg | dimensionless | smallint | 2 | [WISE] W2 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag value is an integer that is the combination of one or more of the following values that signify different conditions: |
w2mag_1 | mag | float | 8 | [WISE] W2 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w2sigm_1 | mag | float | 8 | [WISE] Uncertainty in the W2 5.5" radius aperture magnitude. |
w2flg_1 | dimensionless | smallint | 2 | [WISE] W2 5.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w2flg. |
w2mag_4 | mag | float | 8 | [WISE] W2 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w2sigm_4 | mag | float | 8 | [WISE] Uncertainty in the W2 13.75" radius aperture magnitude. |
w2flg_4 | dimensionless | smallint | 2 | [WISE] W2 13.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w2flg. |
w2mag_7 | mag | float | 8 | [WISE] W2 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w2sigm_7 | mag | float | 8 | [WISE] Uncertainty in the W2 22.0" radius aperture magnitude. |
w2flg_7 | dimensionless | smallint | 2 | [WISE] W2 22.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w2flg. |
w3mpro | mag | float | 8 | [WISE] W3 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W3 flux measurement has SNR<2. This column is null if the source is nominally detected in W3, but no useful brightness estimate could be made. |
w3sigmpro | mag | float | 8 | [WISE] W3 profile-fit photometric measurement uncertainty in mag units. This column is null if the W3 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable. |
w3rchi2 | dimensionless | float | 8 | [WISE] Reduced -ç2 of the W3 profile-fit photometry measurement. This column is null if the W3 magnitude is a 95% confidence upper limit (i.e. the source is not detected). |
w3sat | dimensionless | float | 8 | [WISE] Saturated pixel fraction, W3. The fraction of all pixels within the profile-fitting area source in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W3]~4 mag. Saturation may occur in fainter sources because of a charged particle strike. |
w3mag | mag | float | 8 | [WISE] W3 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w3mcor. |
w3sigm | mag | float | 8 | [WISE] Uncertainty in the W3 "standard" aperture magnitude. |
w3flg | dimensionless | smallint | 2 | [WISE] W3 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag value is an integer that is the combination of one or more of the following values that signify different conditions: |
w3mag_1 | mag | float | 8 | [WISE] W3 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w3sigm_1 | mag | float | 8 | [WISE] Uncertainty in the W3 5.5" radius aperture magnitude. |
w3flg_1 | dimensionless | smallint | 2 | [WISE] W3 5.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w3flg. |
w3mag_4 | mag | float | 8 | [WISE] W3 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w3sigm_4 | mag | float | 8 | [WISE] Uncertainty in the W3 13.75" radius aperture magnitude. |
w3flg_4 | dimensionless | smallint | 2 | [WISE] W3 13.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w3flg. |
w3mag_7 | mag | float | 8 | [WISE] W3 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w3sigm_7 | mag | float | 8 | [WISE] Uncertainty in the W3 22.0" radius aperture magnitude. |
w3flg_7 | dimensionless | smallint | 2 | [WISE] W3 22.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w3flg. |
w4mpro | mag | float | 8 | [WISE] W4 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W4 flux measurement has SNR<2. This column is null if the source is nominally detected in W4, but no useful brightness estimate could be made. |
w4sigmpro | mag | float | 8 | [WISE] W4 profile-fit photometric measurement uncertainty in mag units. This column is null if the W4 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable. |
w4rchi2 | dimensionless | float | 8 | [WISE] Reduced -ç2 of the W4 profile-fit photometry measurement. This column is null if the W4 magnitude is a 95% confidence upper limit (i.e. the source is not detected). |
w4sat | dimensionless | float | 8 | [WISE] Saturated pixel fraction, W4. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W4]~0 mag. Saturation may occur in fainter sources because of a charged particle strike. |
w4mag | mag | float | 8 | [WISE] W4 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w4mcor. |
w4sigm | mag | float | 8 | [WISE] Uncertainty in the W4 "standard" aperture magnitude. |
w4flg | dimensionless | smallint | 2 | [WISE] W4 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag value is an integer that is the combination of one or more of the following values that signify different conditions: |
w4mag_1 | mag | float | 8 | [WISE] W4 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w4sigm_1 | mag | float | 8 | [WISE] Uncertainty in the W4 11.0" radius aperture magnitude. |
w4flg_1 | dimensionless | smallint | 2 | [WISE] W4 11.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w4flg. |
w4mag_4 | mag | float | 8 | [WISE] W4 27.5" radius aperture magnitude. This is the calibrated source brightness measured in a 27.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w4sigm_4 | mag | float | 8 | [WISE] Uncertainty in the W4 27.5" radius aperture magnitude. |
w4flg_4 | dimensionless | smallint | 2 | [WISE] W4 27.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w4flg. |
w4mag_7 | mag | float | 8 | [WISE] W4 44.0" radius aperture magnitude. This is the calibrated source brightness measured in a 44.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. |
w4sigm_7 | mag | float | 8 | [WISE] Uncertainty in the W4 44.0" radius aperture magnitude. |
w4flg_7 | dimensionless | smallint | 2 | [WISE] W4 44.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag, w4flg. |
gFPSFMag | mag | real | 4 | [PS1] Magnitude from mean PSF flux from forced single-epoch g-filter detections. |
gFPSFMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean PSF flux from forced single-epoch g-filter detections. |
gFKronMag | mag | real | 4 | [PS1] Magnitude from thhe mean Kron (1980) flux from forced single-epoch g-filter detections. |
gFKronMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean Kron (1980) flux from forced single-epoch g-filter detections. |
gFApMag | mag | real | 4 | [PS1] Magnitude from the mean aperture flux from forced single-epoch g-filter detections. |
gFApMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean aperture flux from forced single-epoch g-filter detections. |
gFmeanMagR5 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch g-filter detections within an aperture of radius r = 3 00. |
gFmeanMagR5Err | mag | real | 4 | [PS1] Error in magnitude from the mean flux from forced single-epoch g-filter detections within an aperture of radius r = 3 00. |
gFmeanMagR6 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch g-filter detections within an aperture of radius r = 4 63. |
gFmeanMagR6Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch g-filter detections within an aperture of radius r = 4 63. |
gFmeanMagR7 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch g-filter detections within an aperture of radius r = 7 43. |
gFmeanMagR7Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch g-filter detections within an aperture of radius r = 7 43. |
gnTotal | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the g filter. |
gnIncPSFFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the PSF flux mean in the g filter. |
gnIncKronFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the Kron (1980) flux mean in the g filter. |
gnIncApFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the aperture flux mean in the g filter. |
gnIncR5 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R5 (r = 3 00) aperture flux mean in the g filter. |
gnIncR6 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R6 (r = 4 63) aperture flux mean in the g filter. |
gnIncR7 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R7 (r = 7 43) aperture flux mean in the g filter. |
gFlags | dimensionless | int | 4 | [PS1] Information flag bitmask indicating details of the photometry from forced single-epoch g-filter detections. Values listed in ObjectInfoFlags. |
gE1 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e1 = (Mxx GêÆ Myy)/(Mxx + Myy) from forced single-epoch g-filter detections. |
gE2 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e2 = (2Mxy)/(Mxx + Myy) from forced single-epoch g-filter detections. |
rFPSFMag | mag | real | 4 | [PS1] Magnitude from mean PSF flux from forced single-epoch r-filter detections. |
rFPSFMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean PSF flux from forced single-epoch r-filter detections. |
rFKronMag | mag | real | 4 | [PS1] Magnitude from thhe mean Kron (1980) flux from forced single-epoch r-filter detections. |
rFKronMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean Kron (1980) flux from forced single-epoch r-filter detections. |
rFApMag | mag | real | 4 | [PS1] Magnitude from the mean aperture flux from forced single-epoch r-filter detections. |
rFApMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean aperture flux from forced single-epoch r-filter detections. |
rFmeanMagR5 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch r-filter detections within an aperture of radius r = 3 00. |
rFmeanMagR5Err | mag | real | 4 | [PS1] Error in magnitude from the mean flux from forced single-epoch r-filter detections within an aperture of radius r = 3 00. |
rFmeanMagR6 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch r-filter detections within an aperture of radius r = 4 63. |
rFmeanMagR6Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch r-filter detections within an aperture of radius r = 4 63. |
rFmeanMagR7 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch r-filter detections within an aperture of radius r = 7 43. |
rFmeanMagR7Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch r-filter detections within an aperture of radius r = 7 43. |
rnTotal | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the r filter. |
rnIncPSFFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the PSF flux mean in the r filter. |
rnIncKronFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the Kron (1980) flux mean in the r filter. |
rnIncApFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the aperture flux mean in the r filter. |
rnIncR5 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R5 (r = 3 00) aperture flux mean in the r filter. |
rnIncR6 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R6 (r = 4 63) aperture flux mean in the r filter. |
rnIncR7 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R7 (r = 7 43) aperture flux mean in the r filter. |
rFlags | dimensionless | int | 4 | [PS1] Information flag bitmask indicating details of the photometry from forced single-epoch r-filter detections. Values listed in ObjectInfoFlags. |
rE1 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e1 = (Mxx GêÆ Myy)/(Mxx + Myy) from forced single-epoch r-filter detections. |
rE2 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e2 = (2Mxy)/(Mxx + Myy) from forced single-epoch r-filter detections. |
iFPSFMag | mag | real | 4 | [PS1] Magnitude from mean PSF flux from forced single-epoch i-filter detections. |
iFPSFMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean PSF flux from forced single-epoch i-filter detections. |
iFKronMag | mag | real | 4 | [PS1] Magnitude from thhe mean Kron (1980) flux from forced single-epoch i-filter detections. |
iFKronMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean Kron (1980) flux from forced single-epoch i-filter detections. |
iFApMag | mag | real | 4 | [PS1] Magnitude from the mean aperture flux from forced single-epoch i-filter detections. |
iFApMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean aperture flux from forced single-epoch i-filter detections. |
iFmeanMagR5 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch i-filter detections within an aperture of radius r = 3 00. |
iFmeanMagR5Err | mag | real | 4 | [PS1] Error in magnitude from the mean flux from forced single-epoch i-filter detections within an aperture of radius r = 3 00. |
iFmeanMagR6 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch i-filter detections within an aperture of radius r = 4 63. |
iFmeanMagR6Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch i-filter detections within an aperture of radius r = 4 63. |
iFmeanMagR7 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch i-filter detections within an aperture of radius r = 7 43. |
iFmeanMagR7Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch i-filter detections within an aperture of radius r = 7 43. |
inTotal | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the i filter. |
inIncPSFFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the PSF flux mean in the i filter. |
inIncKronFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the Kron (1980) flux mean in the i filter. |
inIncApFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the aperture flux mean in the i filter. |
inIncR5 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R5 (r = 3 00) aperture flux mean in the i filter. |
inIncR6 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R6 (r = 4 63) aperture flux mean in the i filter. |
inIncR7 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R7 (r = 7 43) aperture flux mean in the i filter. |
iFlags | dimensionless | int | 4 | [PS1] Information flag bitmask indicating details of the photometry from forced single-epoch i-filter detections. Values listed in ObjectInfoFlags. |
iE1 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e1 = (Mxx GêÆ Myy)/(Mxx + Myy) from forced single-epoch i-filter detections. |
iE2 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e2 = (2Mxy)/(Mxx + Myy) from forced single-epoch i-filter detections. |
zFPSFMag | mag | real | 4 | [PS1] Magnitude from mean PSF flux from forced single-epoch z-filter detections. |
zFPSFMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean PSF flux from forced single-epoch z-filter detections. |
zFKronMag | mag | real | 4 | [PS1] Magnitude from thhe mean Kron (1980) flux from forced single-epoch z-filter detections. |
zFKronMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean Kron (1980) flux from forced single-epoch z-filter detections. |
zFApMag | mag | real | 4 | [PS1] Magnitude from the mean aperture flux from forced single-epoch z-filter detections. |
zFApMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean aperture flux from forced single-epoch z-filter detections. |
zFmeanMagR5 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch z-filter detections within an aperture of radius r = 3 00. |
zFmeanMagR5Err | mag | real | 4 | [PS1] Error in magnitude from the mean flux from forced single-epoch z-filter detections within an aperture of radius r = 3 00. |
zFmeanMagR6 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch z-filter detections within an aperture of radius r = 4 63. |
zFmeanMagR6Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch z-filter detections within an aperture of radius r = 4 63. |
zFmeanMagR7 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch z-filter detections within an aperture of radius r = 7 43. |
zFmeanMagR7Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch z-filter detections within an aperture of radius r = 7 43. |
znTotal | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the z filter. |
znIncPSFFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the PSF flux mean in the z filter. |
znIncKronFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the Kron (1980) flux mean in the z filter. |
znIncApFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the aperture flux mean in the z filter. |
znIncR5 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R5 (r = 3 00) aperture flux mean in the z filter. |
znIncR6 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R6 (r = 4 63) aperture flux mean in the z filter. |
znIncR7 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R7 (r = 7 43) aperture flux mean in the z filter. |
zFlags | dimensionless | int | 4 | [PS1] Information flag bitmask indicating details of the photometry from forced single-epoch z-filter detections. Values listed in ObjectInfoFlags. |
zE1 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e1 = (Mxx GêÆ Myy)/(Mxx + Myy) from forced single-epoch z-filter detections. |
zE2 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e2 = (2Mxy)/(Mxx + Myy) from forced single-epoch z-filter detections. |
yFPSFMag | mag | real | 4 | [PS1] Magnitude from mean PSF flux from forced single-epoch y-filter detections. |
yFPSFMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean PSF flux from forced single-epoch y-filter detections. |
yFKronMag | mag | real | 4 | [PS1] Magnitude from thhe mean Kron (1980) flux from forced single-epoch y-filter detections. |
yFKronMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean Kron (1980) flux from forced single-epoch y-filter detections. |
yFApMag | mag | real | 4 | [PS1] Magnitude from the mean aperture flux from forced single-epoch y-filter detections. |
yFApMagErr | mag | real | 4 | [PS1] Error in magnitude from the mean aperture flux from forced single-epoch y-filter detections. |
yFmeanMagR5 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch y-filter detections within an aperture of radius r = 3 00. |
yFmeanMagR5Err | mag | real | 4 | [PS1] Error in magnitude from the mean flux from forced single-epoch y-filter detections within an aperture of radius r = 3 00. |
yFmeanMagR6 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch y-filter detections within an aperture of radius r = 4 63. |
yFmeanMagR6Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch y-filter detections within an aperture of radius r = 4 63. |
yFmeanMagR7 | mag | real | 4 | [PS1] Magnitude from the mean flux from forced single-epoch y-filter detections within an aperture of radius r = 7 43. |
yFmeanMagR7Err | mag | real | 4 | [PS1] Error in the magnitude from the mean flux from forced single-epoch y-filter detections within an aperture of radius r = 7 43. |
ynTotal | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the y filter. |
ynIncPSFFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the PSF flux mean in the y filter. |
ynIncKronFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the Kron (1980) flux mean in the y filter. |
ynIncApFlux | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the aperture flux mean in the y filter. |
ynIncR5 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R5 (r = 3 00) aperture flux mean in the y filter. |
ynIncR6 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R6 (r = 4 63) aperture flux mean in the y filter. |
ynIncR7 | dimensionless | smallint | 2 | [PS1] Number of forced single-epoch detections in the R7 (r = 7 43) aperture flux mean in the y filter. |
yFlags | dimensionless | int | 4 | [PS1] Information flag bitmask indicating details of the photometry from forced single-epoch y-filter detections. Values listed in ObjectInfoFlags. |
yE1 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e1 = (Mxx GêÆ Myy)/(Mxx + Myy) from forced single-epoch y-filter detections. |
yE2 | dimensionless | real | 4 | [PS1] Kaiser et al. (1995) polarization parameter e2 = (2Mxy)/(Mxx + Myy) from forced single-epoch y-filter detections. |
EBV_Planck | mag | float | 8 | Planck dust map E(B-V) value at the PS1 coordinates from Planck Collaboration et al., 2014, A&A, 571, A11. |
EBV_PS1 | mag | float | 8 | PS1 dust map E(B-V) value at the PS1 coordinates from Schlafly et al., 2014, ApJ, 789, 15. |
class | dimensionless | varchar | 8 | The class assigned to the source, using the fiducial decision boundary b=0.65 (see Sect. 4.1 of B22). Can take the following values: "GALAXY", "STAR", "QSO" or "UNSURE". |
prob_Galaxy | dimensionless | float | 8 | The probability-like neural network output for the galaxy class. Corresponds to the P_{class} general notation in the text. Refer to Sect. 4.1 of B22 for more details. |
prob_Star | dimensionless | float | 8 | The probability-like neural network output for the star class. Corresponds to the P_{class} general notation in the text. Refer to Sect. 4.1 of B22 for more details. |
prob_QSO | dimensionless | float | 8 | The probability-like neural network output for the quasar class. Corresponds to the P_{class} general notation in the text. Refer to Sect. 4.1 of B22 for more details. |
extrapolation_Class | dimensionless | int | 4 | The extrapolation flag for the classification, 0 if non-extrapolated, 1 if extrapolated. Definition: d_{SOM} > 4.233 (see Sect. 3.4 of B22). |
cellDistance_Class | dimensionless | float | 8 | The distance to the nearest SOM cell centre in the classification SOM. Denoted d_{SOM} in the text (see Sect. 3.4 of B22). |
cellID_Class | dimensionless | int | 4 | The identifier of the nearest SOM cell in the classification SOM (see Sect. 3.4 of B22). |
z_phot | dimensionless | float | 8 | The Monte-Carlo photometric redshift estimate z_{phot}. Slightly less accurate than z_{phot,0}. Refer to Sect. 3.5 and 4.2 of B22 for more details. |
z_photErr | dimensionless | float | 8 | The calibrated redshift error estimate \tilde{\Delta z}_{phot} = 1.986 \Delta z_{phot}. Refer to Sect. 3.5 and 4.2 of B22 for more details. |
z_phot0 | dimensionless | float | 8 | The base photometric redshift estimate z_{phot,0}. Refer to Sect. 3.5 and 4.2 of B22 for more details. |
extrapolation_Photoz | dimensionless | int | 4 | The extrapolation flag for the photo-z estimation, 0 if non-extrapolated, 1 if extrapolated. Definition: d_{SOM} > 3.702 (see Sect. 3.4 of B22). |
cellDistance_Photoz | dimensionless | float | 8 | The distance to the nearest SOM cell centre in the photo-z SOM. Denoted d_{SOM} in the text (see Sect. 3.4 of B22). |
cellID_Photoz | dimensionless | int | 4 | The identifier of the nearest SOM cell in the photo-z SOM (see Sect. 3.4 of B22). |
Data Access
WISE-PS1-STRM is available in MAST CasJobs for SQL queries, or can be downloaded as .csv.gz files based on strips of declination. There are two tables available in CasJobs: "catalogRecordRowStore" which is optimized for row extraction queries (queries where you want to retrieve a subset of the data) and "catalogRecordColumnStore" which is optimized for count() queries and should not be used for extracting subsets of the data. These tables can be found in the HLSP_WISE_PS1_STRM Context.
-
A web-based SQL interface to query and cross-match between catalogs. Export tables, saved queries, long query submissions.
NOTE: Each file in the table below is a few GB in size (~0.5-15 GB, depending on declination strip).