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 GX 340+0 251.4463 -45.6133 250.537018 -45.522593 255.990327 -23.069192 339.58535361 -0.07953483 81.21 54892.2765740741 2009-03-02 06:38:16 54894.8168287037 2009-03-04 19:36:14 403060010 107.3127 100 107.3145 107.3127 0 107.3145 2 2 0 2 1 0 0 86.104 86.104 219.4467 1 PROCESSED 57545.7913541667 2016-06-06 18:59:33 55329 2010-05-13 00:00:00 54908.7293055556 2009-03-18 17:30:12 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031164 In this proposal we request to observe accreting neutron stars sources GX 340+0, GX 3+1 and GX 13+1. The observational goal of the observations is to collect high-spectral resolution data in the region of K$_alpha$ iron line. Our scientific motivation is to put the origin of the line emission under additional theoretical scrutiny. We wish to compare the performance of the wind-reprocessing model to relativistic model in as many sources as possible. This proposal is a part of our broader effort to investigate the origin of iron emission line in Galactic X-ray binaries, which includes a parallel proposal to observe WD binaries. GALACTIC POINT SOURCES 4 B NIKOLAI SHAPOSHNIKOV USA 3 AO3 IRON KALPHA EMISSION LINE DIAGNOSTICS IN ACCRETING NEUTRON STARS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403060010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403060010'

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