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 | 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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