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 | 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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