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 4395 | 186.4111 | 33.4884 | 185.79012 | 33.76517 | 170.810459 | 32.904029 | 162.54122992 | 81.55189464 | 303.1476 | 54253.6042013889 | 2007-06-02 14:30:03 | 54256.2981944444 | 2007-06-05 07:09:24 | 702001010 | 101.5075 | 100 | 101.5155 | 101.5075 | 0 | 101.5155 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 101.9292 | 101.9292 | 232.7198 | 4 | PROCESSED | 57538.8900694444 | 2016-05-30 21:21:42 | 54745 | 2008-10-06 00:00:00 | 54263.5438194445 | 2007-06-12 13:03:06 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 020001 | We propose a 100 ks observation of the intermediate mass black hole (IMBH) active nucleus in the dwarf Seyfert galaxy NGC 4395. Utilising the high-energy sensitivity of Suzaku will enable us to determine the shape of the intrinsic continuum, which is significantly absorbed below 10 keV. Constraining the shape of the continuum will allow us to investigate the more general problem of the relationship between AGN flux and apparent spectral slope. In addition, with a firm grasp of the intrinsic continuum properties, we can accurately determine the physical conditions of the warm absorber in NGC 4395. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | YASUO TANAKA | JAP | 2 | AO2 | UNCOVERING THE IMBH ACTIVE NUCLEUS IN THE DWARF SEYFERT GALAXY NGC 4395 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702001010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702001010'
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