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. |
observation_id
|
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
|
exposure
|
awarded_exposure
|
resolve_exposure
|
xtend_exposure
|
resolve_data_mode
|
resolve_with_filter_be
|
resolve_with_filter_fe55
|
resolve_with_filter_nd
|
resolve_with_filter_poly
|
resolve_with_filter_open
|
resolve_with_filter_undef
|
is_resolve_gatevalve_closed
|
is_resolve_mxs1
|
is_resolve_mxs2
|
is_resolve_mxs3
|
is_resolve_mxs4
|
xtend_number_modes
|
xtend_dataclass_file1
|
xtend_dataclass_file2
|
xtend_window1_exposure
|
xtend_window2_exposure
|
xtend_window1_burst_exposure
|
xtend_window2_burst_exposure
|
xtend_code
|
resolve_code
|
gen_code
|
processing_status
|
processing_date
|
public_date
|
distribution_date
|
processing_version
|
caldb_version
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
proposal_type
|
proposal_title
|
observation_status
|
data_access_url
|
xtend_data_mode1
|
xtend_data_mode2
|
processing_count
|
remarks
|
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 300018010 | M81 | 148.89023 | 69.06487 | 147.86581 | 69.30187 | 119.49165 | 51.58025 | 142.09173 | 40.90089 | 286.83671 | 60438.36324 | 2024-05-08 08:43:04 | 60442.00352 | 2024-05-12 00:05:04 | 268.779 | 100.000 | 268.779 | 239.300 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 239.300 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2024-09-26 20:18:39 | 2025-08-31 00:00:00 | 2024-05-19 12:44:22 | 03.00.013.009 | gen20240315_xtd20240815_rsl20240815 | Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 | 000000036 | Up to 40% of all galaxies may harbor low-ionization nuclear emission region (LINERs) and low-luminosity AGN (LLAGN). Well-developed theory suggests that the inner flow should be advective and radiatively inefficient, with a standard thin disk truncated far from the black hole. Resolve spectroscopy of M81* offers the best chance to finally reveal the geometry and dynamics of a radiatively inefficient accretion flow (RIAF) onto a black hole. M81* is the brightest LINER /LLAGN in X-rays. Prior Chandra/HETG spectra reveal low-ionization and He-like and H-like Fe K emission lines that are likely redshifted. A 100 ks exposure with Resolve can make unique tests of RIAF models. | NON-JET-DOMINATED AGN | 3 | C | XRISM Collaboration | JAP | 0 | NOR | A RADIATIVELY INEFFICIENT ACCRETION FLOW IN THE LINER M81* | archived | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300018010/ | WINDOW1 | 4 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '300018010'
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