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 SKY(270, +25) 270.2558 25.1504 269.745742 25.150381 270.337589 48.59021 50.99920401 21.68976417 70.6538 55284.5620023148 2010-03-29 13:29:17 55285.2994791667 2010-03-30 07:11:15 404041010 1.7019 25 1.9266 2.0944 0 1.7019 2 2 0 2 1 0 0 5.6211 5.6211 63.7139 1 PROCESSED 57551.0540277778 2016-06-12 01:17:48 55284 2010-03-29 00:00:00 55301.2652314815 2010-04-15 06:21:56 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041222 Suzaku has recently revealed relativistically broadened Fe Kalpha emission lines in the spectra of neutron star low-mass X-ray binaries (LMXBs). We have now seen these lines in 10 neutron star LMXBs that we have examined, allowing measurements of the inner accretion disk radius, and hence an upper limit on the neutron star radius in all these objects. Only with the sensitivity of Suzaku, its high effective area in the Fe K band, and its broad bandpass has it been possible to robustly determine the shape of the lines. With a longer-term aim of completing a census of iron lines in neutron star LMXBs, we request a total of 200 ks to observe 5 neutron star low-mass X-ray binaries to study the relativistic broadening in the Fe Kalpha emission line profiles. GALACTIC POINT SOURCES 4 C EDWARD CACKETT USA 4 AO4 AN FE KALPHA EMISSION LINE SURVEY OF NEUTRON STAR LMXBS HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404041010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404041010'

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