DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | SDSS J0943+5417 | 145.8252 | 54.2751 | 144.963883 | 54.504193 | 127.754031 | 37.9036 | 161.23003018 | 46.41565232 | 274.2141 | 54975.5889236111 | 2009-05-24 14:08:03 | 54976.3473611111 | 2009-05-25 08:20:12 | 704052010 | 34.2264 | 30 | 34.2264 | 34.2264 | 0 | 34.2264 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 32.0591 | 32.0591 | 65.5179 | 2 | PROCESSED | 57546.6638773148 | 2016-06-07 15:55:59 | 55358 | 2010-06-11 00:00:00 | 54992.6588888889 | 2009-06-10 15:48:48 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 041422 | BALQSOs can be used to probe geometric and evolutionary models of quasars and AGN feedback. Recent studies have found larger (~2X) BALQSO fractions in NIR selected samples compared to those in optical samples and have suggested that the NIR samples of BALQSOs better represent the general population of BALQSOs. We propose to observe three bright, red 2MASS selected BALQSOs with Suzaku, to complement archival X-ray observations of BALQSOs that may have been biased by their selection on optical properties only. Combined with the archival sample, we will measure the average X-ray properties of BALQSOs. By comparing the hard X-ray to K_s band flux ratios at a range of optical to infrared colors, we will test the robustness of NIR selection and the origin of the large NIR BALQSO fraction. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | XINYU DAI | USA | 4 | AO4 | X-RAY PROPERTIES OF 2MASS SELECTED BALQSOS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704052010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '704052010'
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