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 1915+105 288.7933 10.9535 288.203422 10.865162 292.134883 32.961388 45.37037141 -0.21130356 67.354 54227.6113657407 2007-05-07 14:40:22 54229.0717476852 2007-05-09 01:43:19 402071010 65.6568 37 65.6568 65.8039 0 65.6728 1 2 0 1 1 0 0 56.8973 56.8973 126.168 1 PROCESSED 57538.6640972222 2016-05-30 15:56:18 54702 2008-08-24 00:00:00 54235.5321759259 2007-05-15 12:46:20 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021132 We have discovered a connection between Fe line strength and QPO phase in RXTE observations of GRS 1915+105. This connection independently ties Fe lines to radii less than 100 R_Schw. QPO-phase-resolved Suzaku spectra will enable us to detect changes in the relativistic line profile (inner radius, equivalent width), to extend the connection to the broadband disk reflection spectrum, and to test models for the Fe line - QPO connection. Moreover, at CCD resolution, the connection can be used to over-constrain disk radii - a first step toward mapping the inner disk. We therefore request a 37 ksec TOO observation of GRS 1915+105. Understanding black hole accretion is fundamental to NASA's "SEU" theme. GALACTIC POINT SOURCES 4 A JON MILLER USA 2 AO2-TOO THE RELATIVISTIC IRON LINE - QPO CONNECTION IN GRS 1915+105 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402071010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402071010'

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