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 GRS 1758-258 270.2971 -25.679 269.522467 -25.678561 270.258372 -2.238361 4.56169204 -1.32563061 89.3817 55263.8983333333 2010-03-08 21:33:36 55266.0711111111 2010-03-11 01:42:24 404060010 82.6827 80 82.6827 82.6827 0 82.6827 2 2 0 2 1 0 0 71.1789 71.1789 187.7097 1 PROCESSED 57550.8664583333 2016-06-11 20:47:42 55647 2011-03-27 00:00:00 55279.5468402778 2010-03-24 13:07:27 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041244 We propose an 80 ks observation to obtain a broadband spectrum of the Galactic microquasar GRS 1758-258 while in the low-hard state with Suzaku. Here we aim to constrain the nature and geometry of the accretion flow via measurements of the various disc reflection features, which are detectable for the first time due to the unique capabilities of Suzaku. As this system is known to power large radio jets, its study will also aid our understanding of the conditions necessary for the formation of relativistic outflows and how these relate to the accretion geometry in the low-hard state. GALACTIC POINT SOURCES 4 B MARK REYNOLDS USA 4 AO4 CONSTRAINING DISC REFLECTION IN THE MICROQUASAR GRS 1758-258 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404060010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404060010'

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