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 NGC 3718 173.2341 53.1118 172.54734 53.387989 147.276263 44.880657 146.87581124 60.21394242 142.7392 55128.8497800926 2009-10-24 20:23:41 55130.255775463 2009-10-26 06:08:19 704048010 59.8882 60 59.9202 59.8882 0 59.9202 2 2 0 2 1 0 0 52.4392 52.4392 121.4599 0 PROCESSED 57548.9845138889 2016-06-09 23:37:42 55507 2010-11-07 00:00:00 55141.3212384259 2009-11-06 07:42:35 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041415 The SWIFT BAT hard (14-195 KeV) survey is performing the first unbiased hard X-ray survey of the entire sky with follow-up observations with the Swift XRT to fully identify the sample. In this survey we have found two very low luminosity nearby hard X-ray sources which show little, if any, evidence for nuclear activity in the optical or UV band, and have very low apparent Eddington ratios. We propose Suzaku observations of these objects to determine whether there is an X-ray spectral signature of a low Eddington ratio, as predicted if these objects are indeed in a radiatively inefficient accretion flow. EXTRAGALACTIC COMPACT SOURCES 7 B RICHARD MUSHOTZKY USA 4 AO4 SUZAKU OBSERVATIONS OF NGC4138 AND NGC3718 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704048010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '704048010'

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