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 1448 | 56.1426 | -44.6942 | 55.730836 | -44.850191 | 33.469346 | -61.660504 | 251.59735556 | -51.37690943 | 264.6522 | 54879.3481828704 | 2009-02-17 08:21:23 | 54880.4501041667 | 2009-02-18 10:48:09 | 703062010 | 52.9653 | 50 | 52.9653 | 52.9653 | 0 | 52.9653 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 55.0869 | 55.0869 | 95.202 | 1 | PROCESSED | 57545.5960763889 | 2016-06-06 14:18:21 | 55330 | 2010-05-14 00:00:00 | 54893.4451041667 | 2009-03-03 10:40:57 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 032018 | We propose for a 50 ks Suzaku observation of NGC 1448, a nearby (15 Mpc) gas-rich and dust-obscured Scd galaxy that is optically classified as an HII galaxy. From our Spitzer-IRS mid-IR spectroscopy, we have found the first evidence for an obscured AGN in NGC 1448. On the basis of this data, NGC 1448 appears to be harboring a rapidly growing small obscured black hole (M_BH ~ 6x10^5 M_Sun; Eddington ratio of >0.1), and therefore appears to be an analog of the nearby Compton-thick AGN NGC 4945. To date, no sensitive hard X-ray constraints exist for NGC 1448, which are required to provide a direct measurement of the absorption and mass accretion rate, and thus to test if NGC 1448 is also a Compton-thick AGN. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | DAVID ALEXANDER | EUR | 3 | AO3 | NGC 1448: A MISSING COMPTON-THICK AGN IN OUR BACKYARD? | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703062010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703062010'
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