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
1 SDSS J1723+5553 260.8912 55.8942 260.65651 55.938805 243.54174 78.493359 83.89291292 34.34970174 8.0654 54986.3677777778 2009-06-04 08:49:36 54986.8148032407 2009-06-04 19:33:19 704051010 35.9368 30 35.9448 35.9368 0 35.9528 1 1 0 1 1 0 0 29.0393 29.0393 38.6159 0 PROCESSED 57547.4618865741 2016-06-08 11:05:07 55364 2010-06-17 00:00:00 54998.1759722222 2009-06-16 04:13:24 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/ver3.0/704051010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '704051010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏